PDS_VERSION_ID = PDS3
LABEL_REVISION_NOTE = "2004-09-23 KW: Initial draft.
2005-12-09 AC: Orbiter Information
Updated Added Inst_host
for lander References TBD
2006-01-10 AC: Removed special
characters
2006-02-15 PG: Added Inst_host for
lander
2007-01-26 MB: 70 char line length
2007-08-14 MB: remove not ascii symbols
2008-02-02 Maud Barthelemy
2008-04-11 JL Vazquez, SA
2008-05-09, MB
2010-02-15, MB
2011-06-07, MB, editorial
2012-06-06, M. Barthelemy after AST2
review;
2017-04-26, M. Barthelemy missing
reference and Lander updates.
"
RECORD_TYPE = STREAM
OBJECT = INSTRUMENT_HOST
INSTRUMENT_HOST_ID = RO
OBJECT = INSTRUMENT_HOST_INFORMATION
INSTRUMENT_HOST_NAME = "ROSETTA-ORBITER"
INSTRUMENT_HOST_TYPE = SPACECRAFT
INSTRUMENT_HOST_DESC = "
TABLE OF CONTENTS
----------------------------------
= Spacecraft Overview
= Mission Requirements and Constraints
= Platform Definition
= Subsystem Accommodation
= Rosetta Spacecraft Frames
= Structure Design
- Solar Array
- Reaction Wheels
- Propellant Tanks
- Helium Tanks
- Thrusters
- High Gain Antenna
- Gyros
= Mechanisms Design
- Solar Array Drive Mechanism (SADM)
- Solar Array Deployment Mechanisms
- HGA Antenna Pointing Mechanism (APM)
- Experiment Boom Mechanisms
- Louvres
= Thermal Control Design
- Thermal Control Concept
- Thermal control design
- General Heater Control Concept
- Micrometeoroid and Cometary Dust Protection
= Propulsion Design
- Operation
= Telecommunication Design
- High Gain Antenna Major Assembly
- High Gain Antenna Frame
- Medium Gain Antenna
- MGAS
- MGAX
= Power Design
- Power Conditioning Unit (PCU)
- Payload Power Distribution Unit (PL-PDU)
- Subsystems Power Distribution Unit (SS-PDU)
- Batteries
- Solar Array Generator
- Mechanical Design of the Solar Panels
- Rosetta Solar Array Frames
= Power Constraints in Deep Space
= Harness Design
= Avionics Design
- Data Management Subsystem (DMS)
- Solid State Mass Memory (SSMM)
- Attitude and Orbit Control Measurement System (AOCMS)
- Avionics external interface
= Avionics modes
- Stand-By Mode
- Sun Acquisition Mode
- Safe/Hold Mode
- Normal Mode
- Thruster Transition Mode
- Orbit Control Mode
- Asteroid Fly-By Mode
- Near Sun Hibernation Mode
- Spin-up Mode
- Sun Keeping Mode
= System Level Modes
- Pre-launch Mode
- Activation Mode
- Active Cruise Mode
- Deep Space Hibernation Mode
- Near Sun Hibernation Mode
- Asteroid Fly-by Mode
- Near Comet Mode
- Safe Mode
- Survival Mode
= Ground Segment
- New Norcia
- Cebreros
- Kouru
- NASA DSN
= Acronyms
Spacecraft Overview
=====================================================================
Please note: The ROSETTA spacecraft was originally designed for a
mission to the comet Wirtanen. Due to a delay of the launch a new
comet (Churyumow-Gerasimenko) had been selected. The compliance of
the design was checked and where necessary adapted for this new
mission. Therefore in the following all the details and
characteristics for this new mission are used (like min and max
distance to Sun).
The Rosetta design is based on a box-type central structure, 2.8 m x
2.1 m x 2.0 m, on which all subsystems and payload equipment are
mounted. The two solar panels have a combined area of 64 m2 (32.7m
tip to tip), with each extending panel measuring 14 m in length.
The 'top' of the spacecraft accommodates the payload instruments, and
the 'base' of the spacecraft the subsystems. The spacecraft can be
physically separated into two main modules:
* A Payload Support Module (PSM)
* A Bus Support Module (BSM)
The Lander is attached to the rear face (-X), opposite the two-axes
steerable high-gain antenna (HGA). The two solar wings extend from
the side faces(+/-Y). The instrument panel points almost always
towards the comet, while the antennas and solar arrays point towards
the Sun and Earth (at such great distances the Earth is relatively
speaking in the same direction). The spacecraft attitude concept is
such that the side and back panels are shaded throughout all nominal
mission phases, offering a good location for radiators and louvres.
This will normally be facing away from the comet, minimising the
effects of cometary dust.
The spacecraft is built around a vertical thrust tube, whose diameter
corresponds to the 1194 mm Ariane-5 interface. This tube contains two
large, equally sized, propellant tanks, the upper one containing
fuel, and the lower one containing the (heavier) oxidiser. At launch
the total amount of stored propellant was roughly 1670 kg.
A coarse overview on the spacecraft main characteristics is
summarised hereafter:
Total launch mass requirement: 3065 kg
Propellant mass: 1718 kg
Overall size (xyz)
Launch configuration: 225x256x318 cm
SA deployed: 32.7 m tip-to-tip
power provided by SA: 440 W at max dist from sun (5.3 AU)
energy provided by 3 Batteries: 500 Wh
data management: operation of s/c according to an on-
board master schedule and real-time
via ground-link
Mission Requirements and Constraints
=====================================================================
In the following, the stringent mission requirements are summarised
and related to their consequences on the spacecraft system design.
The ambitious scientific goals of the ROSETTA mission require:
* a large number of complex scientific instruments, to be
accommodated on one side of the spacecraft, that shall, in the
operational phase, permanently face the comet. During cruise the
instruments shall be served for survival.
* one Surface Science Package (SSP), to be accommodated, suitable for
cruise survival and proper, independent ejection from the orbiter
(spacecraft). In addition, the orbiter shall provide the capability
for SSP data relay to Earth.
* a complex spacecraft navigation at low altitude orbits around an
irregular celestial body with weak, asymmetric, rotating gravity
field, rendered by dust and gas jets. These primary mission
requirements are design driving for most of the spacecraft layout and
performance features, as:
* data rate (DMS, TTC)
* pointing accuracy (AOCMS, Structure)
* thermal layout
* closed loop target tracking (AOCMS, NAV Camera), derived
requirements from asteroid fly-by
* small-delta-v manoeuvre accuracy (RCS)
Other mission requirements, that relate to the interplanetary cruise
phases rather than to the scientific objectives, drive mainly the
power supply, propulsion, autonomy, reliability and
telecommunication:
For achieving the escape energy (C3=11.8 km^2/s^2) to the
interplanetary injection, an Ariane 5 Launch (delayed ignition) is
required, that constrains the maximum S/C wet mass and defines the
available S/C envelope in Launch configuration.
The total mission delta-v of more than 2100 m/s requires a propulsion
system with over 1700 kg bi-propellant.
The environmental loads (radiation, micro meteoroids impacts) over
the mission duration of nearly 12 years is very demanding w.r.t.
shielding, reliability and life time of the S/C components.
The large S/C to Earth distance throughout most mission phases makes
a communication link via an on-board high gain antenna (HGA)
mandatory. The spacecraft must provide an autonomous HGA Earth-
pointing capability using star sensor attitude information and on-
board stored ephemeris table. TC link via spherical LGA coverage, and
TC/TM links via an MGA shall be possible as backup for a loss of the
HGA link.
The wide range of S/C to Sun distances (0.88 to 5.33 AU) drive the
thermal control and the size of the solar generator.
The long signal propagation time (TWTL up to 100 minutes), and the
extended hibernation phases (2.5 years the longest one), and the many
solar conjunctions/oppositions (the longest in active phases is 7
weeks) require a high degree of on-board autonomy, with corresponding
FDIR concepts.
Platform Definition
=====================================================================
The ROSETTA platform is designed to fulfill the need to accommodate
the payload (including fixed, deployable and ejectable experiment
packages), high gain antenna, solar arrays and propellant mass in a
particular geometrical relationship (mass properties and spacecraft
viewing geometry) and with the specified modularity (Bus Support
Module and Payload Support Module incorporating Lander Interface
Panel). The thermal environment also drives the configuration such
that high dissipation units must be mounted on the side walls with
thermal louvres providing trimming for changing external conditions
during the mission.
The design of the platform's electrical architecture is driven by the
need to meet specific power requirements at aphelion (the solar array
sizing case) and to incorporate maximum power point tracking.
Additional factors such as the uncertainty in the performance of the
Low Intensity Low Temperature solar cell technology have also
influenced the design.
The telecommunications design is driven by the need to be compatible
with ESA's 15m and 32m ground stations and the 34m and 70m DSN
stations. This has produced requirements for dual S/X band and
variable rate capability, together with an articulated High Gain
Antenna to maximise data transfer during the payload operations, and
a fixed Medium Gain Antenna to act as backup for the HGA in case of
failure.
Subsystem Accommodation
=====================================================================
The majority of the subsystem equipments are accommodated together
within the BSM. The electronic units are located mostly on the Y
panels so that their thermal dissipations are closely coupled to the
louvred radiators on the sidewalls. So far as practical, functionally
related groups are located close together for harness, integration
and testability reasons. Where possible, equipments are positioned
towards the +X half of the S/C to counterbalance the mass of the
Lander on the opposite side.
Some subsystem equipments are deliberately located on the PSM. These
include the PDU and RTU for the payload, the NAVCAMS, two of the SAS
units and the +Z LGA. The PDU and RTU are located closer to the
payload instruments to reduce harness complexity and mass, and the
NAVCAMs and SASs and +Z LGA are located on the PSM for field of view
reasons. Other subsystem equipments have been located on the PSM
sidewalls as a result of BSM equipment/harness growth, or thermal
limitations. These comprise the STR electronics and SSMM as well as
the USO.
The RCS subsystem comprises tanks, thrusters and the associated
valves and pipework. The main tanks are accommodated within the
central tube while the helium pressurisation tanks are mounted on the
internal deck. Most of the valves and pipework are located on the +X
BSM, panel which becomes permanently attached to the BSM once RCS
assembly is completed. Sixteen of the twenty-four thrusters are
located at the four lower corners of the BSM. The remaining
thrusters are located in 4 groups near the top corners of the S/C.
They are installed as part of the BSM, but are attached to the PSM
after PSM/BSM mating.
The Star Trackers are mounted on the -X shearwalls. The STR B is
rotated by additional 10 degrees towards the -Z direction compared to
STR A to avoid the VIRTIS radiator rim to be seen in its field of
view. This location of the STRs is both thermally stable and
mechanically close to the -X PSM panel which accommodates the
instruments requiring high pointing accuracy. The reaction wheels are
located on the internal deck which provides them with a thermo-
elastically stable location.
A 2.2m diameter HGA is stowed face-outwards for launch against the
S/C +X face (so it would be partially usable even in the event of a
deployment failure). After deployment, the HGA can be rotated in two
axes around a pivot point on a tripod assembly some distance clear of
the lower corner of the S/C. This provides the HGA with greater than
hemispherical pointing range. The two MGAs are fixed mounted on the
S/C +X face, oriented in the +Xs/c direction, as this is the most
useful direction for a fixed MGA. The LGAs are located at the +Z and
-Z ends of the S/C but angled at 30 degs to the Z axis. This
accommodation provides spherical coverage with minimum need for
switching.
The solar array comprises two 5-panel wings folded against the
Spacecraft Y axis for launch. Because the arrays are sized to operate
at aphelion, the outwards facing outer panel can also generate useful
power before array deployment.
Two Sun Acquisition Sensors are located on the solar arrays and
another two on the S/C body. Their design and location of these also
allow them to serve as fine Sun sensors.
Rosetta Spacecraft Frame
=====================================================================
Rosetta spacecraft frame is defined as follows:
- +Z axis is perpendicular to the launch vehicle interface
plane and points toward the payload side;
- +X axis is perpendicular to the HGA mounting plane and
points toward HGA;
- +Y axis completes the frame is right-handed.
- the origin of this frame is the launch vehicle interface
point.
These diagrams illustrate the ROS_SPACECRAFT frame:
+X s/c side (HGA side) view:
----------------------------
^
| toward comet
|
Science Deck
._____________.
.__ _______________. | | .______________ ___.
| \ \ \ | | / \ \ |
| / / \ | +Zsc | / / / |
| \ \ `. | ^ | .' \ \ |
| / / | o| | |o | / / |
| \ \ .' | | | `. \ \ |
| / / / | | | \ / / |
.__\ \_______________/ | +Xsc| | \_______________\ \__.
-Y Solar Array .______o-------> +Ysc +Y Solar Array
._____.
.' `.
/ \
. `. .' . +Xsc is out of
| `o' | the page
. | .
\ | /
`. .'
HGA ` --- '
+Z s/c side (science deck side) view:
-------------------------------------
_____
/ \ Lander
| |
._____________.
| |
| |
| +Zsc | +Ysc
o==/ /==================o | o------->o==================/ /==o
-Y Solar Array | | | +Y Solar Array
| | |
.______|______.
`. | .'
.--V +Xsc
HGA .' `.
/___________\
`.|.' +Zsc is out
of the page
Structure Design
=====================================================================
The ROSETTA platform structure consists of two modules, the Bus
Support Module and the Payload Support Module (BSM and PSM). Mounted
to the BSM is the Lander Interface Panel (LIP), which can be handled
separately for the Lander integration.
The spacecraft structural design is based on a version with a central
cylinder accommodating the two propellant tanks. The general
dimensions are dictated on one hand by the need to accommodate the
two large tanks, to provide sufficient mounting area for the payload
and subsystems and the Lander, as well as being able to accommodate
two large solar arrays, and on the other hand by the requirement to
fit within the Ariane 5 fairing.
The spine of the structure is the central tube, to which the
honeycomb panels are mounted. The spacecraft box is closed by lateral
panels, which are connected to the central tube by load carrying
vertical shear webs and an internal deck.
The Bus Support Module (BSM) accommodates most of the platform and
avionic equipment.
The Payload Support Module (PSM) is accommodating all science
equipment. The PSM structure consists of the PSM +z-panel, the PSM -x
panel, the PSM +y/-y panels and the Lander Interface Panel (LIP).
Most instrument sensors are located on a single face, the +Z panel,
with the exception of VIRTIS and OSIRIS mounted on the -X panel to
allow for the accommodation of their cold radiators, Alice mounted on
PSM -X and COSIMA mounted on the PSM -Y panel. The P/L electronics
are mounted on the +Y and -Y side of this module for heat radiation
via Louvers.
Special supports are provided by the structure for:
Solar Array
-----------
They provide stiff and accurately positioned points for the solar
array hold down points and for solar arrays drive mechanisms.
Reaction Wheels
---------------
The brackets provide stiff wheel support with alignment capability.
All 4 RW brackets are mounted together between the +X shear wall and
the central deck building one compact bracket unit which provides
high stiffness and stability.
Propellant Tanks
----------------
The two tanks are mounted via a circumferential ring of flanges to a
reinforced adapter ring on the tube with titanium screws.
Helium Tanks
------------
The two helium tanks are mounted on the main deck of the BSM. They
are attached by an equatorial fixation in the middle of the tank
through internal deck holes.
Thrusters
---------
Thrusters on the side of the spacecraft are mounted on lateral panel
extensions with aluminium machined brackets ensuring the angular
position of the thrusters. Thrusters underneath the spacecraft (-Z
pointing thrusters) are mounted on brackets on the corners of the
+/-Y panels.
High Gain Antenna
-----------------
The HGA is stowed against the +X panel, in areas stiffened by the
+/-Y panels and the HGA support tripod. After launch, the HGA is
deployed and is connected to the S/C by the support tripod only. The
axis Antenna Pointing Mechanisms, fixed on the tripod, are located
close to the edge of the HGA.
Gyros
-----
A single bracket provides stiff gyro support and alignment capability
and orientates the 3 IMUs in the requested angular orientation. The
bracket is mounted on the -Y BSM panel for thermal dissipation
reasons.
Mechanisms Design
=====================================================================
The ROSETTA mechanisms comprise the following major equipments:
* Solar Array Drive Mechanism (SADM)
* Solar Array Deployment Mechanisms
* HGA Antenna Pointing Mechanism (APM)
* HGA Holddown & Release Mechanism (HRM)
* Experiment Booms & HRMs
* Louvres (mechanical elements)
Solar Array Drive Mechanism (SADM)
----------------------------------
The SADM performs the positioning of the Solar Array w.r.t. the Sun
by rotation of the panels around the spacecraft Y-axis. There are two
identical SADMs on both sides of the spacecraft, which can be
individually controlled. The control authority rests with the AOCMS
subsystem, which always 'knows' the actual attitude and Sun direction
and is therefore in the position to determine the required
orientation of the solar panels. The positioning commands are routed
from the AOCMS I/F Unit via the SADE (SADM-Electronics) to the SADM.
The Solar Array rotation is limited to plus and minus 180 degrees to
the reference position. The array zero position is defined in the
section 'Power Design: Solar Array Generator' below.
The Solar Array Drive Mechanism baseline design comprises the
following major components:
* Housing structure from aluminium alloy
* Main bearing, pre-loaded angular contact roller bearing
* Drive unit consisting of a redundantly wound stepper motor, gear-
reduction unit, anti-backlash pinion, and final stage gear ring
* Redundant position transducer and electronics, harness and
connectors.
* Mechanical end-stop for +/-180 deg travel limit with redundant
micro-switches (4 in all)
* Redundant electrical power and signal harnesses, and connectors
* Twist capsule unit, allowing +/-180 deg electrical circuit transfer
* Thermistor for temperature reading, with harness.
The SADM drive unit employs a 'pancake' configuration with one single
X-type ballbearing to provide high moment stiffness and strength
within a compact axial envelope. The central output shaft is of
hollow construction, providing sufficient space to accommodate the
power and signal transfer harness and a twist capsule allowing +/-180
degrees rotation of the harness. The drive unit contains a position
transducer and a drive train.
The Solar Arrays Drive Electronic is intended to manage two Solar
Array Drives that can be rotated so as to get the maximum energy from
the solar cell panels.
Solar Array Deployment Mechanisms
----------------------------------
The baseline are 2 solar arrays, each with a full silicon 5-panel
wing, with panel sizes as used in the ARA MK3 5-panel qualification
wing (about 5.3 m2 per panel).
During launch the wings are stowed against the sidewalls of the
satellite. They are kept in this position by means of 6 hold-down
mechanisms per wing.
Approximately 3 hours after launch, the satellite is pointed towards
the Sun and the wings are deployed to their fully deployed position.
They are released for full deployment by 'cutting' Kevlar restraint
cables by means of thermal knives (actually degrading of the Kevlar
by heat).
The deployment system makes use of spring driven hinges and is
equipped with a damper, that limits the deployment speed of the wing.
Thus, the deployment shocks on SADM hinge and inter-panel hinges are
kept relatively low.
The Rosetta wing is further equipped with:
* ESD protection on front and rear side,
* Solar Array sun acquisition sensor,
* Solar Array performance strings
HGA Antenna Pointing Mechanism (APM)
------------------------------------
The APM is a two-axes mechanism which allows motion of the HGA in
both azimuth and elevation. The control authority rests with the
AOCMS subsystem, which always 'knows' the actual attitude and Earth
direction and is therefore in the position to determine the required
orientation of the antenna. The positioning commands are routed from
the AOCMS I/F Unit via the APM-E (APM-Electronics) to the APMM. HGA
elevation rotation is physically limited to +30deg/ -165deg from the
reference position (after deployment). Before and during deployment
the range is -207deg and +30deg.
HGA azimuth rotation is physically limited to +80deg / -260deg from
the reference position.
The main functions of the APM are:
* Allow accurate and stable pointing of the antenna dish through
controlled rotation about azimuth and elevation axes.
* Minimise stresses on the waveguides by acting as load transfer path
between the HGA and the spacecraft.
It consists of three main components:
* The motor drive units (APM-M) and RF Ancillary Equipment (Rotary
Joint)
* The support structure (APM-SS).
* The electronic control of these units (APM-E).
The APM-M is mounted between the antenna dish and the APM-SS.
For thermal reasons the elements of the APM-M and APM-SS and the
Antenna HDRMs are covered with MLI.
Experiment Boom Mechanisms
---------------------------
Two deployable experiment booms support a number of different
lightweight sensors from the plasma package which need to be deployed
clear of the S/C body. These booms are deployed at beginning of the
mission after Launch.
Each boom consists of a 76 mm dia CFRP tube. The lower boom is
approximately 1.3 m long and the upper boom 2m.
The boom deployment is performed by means of a motor driven unit. The
deployment mechanism consists of:
* Hinge, Motor Gear Unit, Coupling system, Latching system and
Position switches.
The Hold down and release mechanisms, one per boom, has the following
characteristics:
* Three Titanium blades to allow relative displacement in the boom
centreline direction. This reduces the mechanical and thermo-
elastic I/F forces.
* The separation device is the Hi-Shear low shock Separation Nut
SN9422-M8
Louvres
--------
The Rosetta Thermal Control Subsystem contains 14 louvers with 2
different set points which are located on the S/C Y walls in front of
white painted radiators. The louvers are designed, manufactured and
qualified by SENER.
The mechanisms of the 16 blade louver are the 8 temperature dependent
bi-metal springs (actuators), which supply the fundamental function
of the louver. The actuators are driving the louver blades to its end
stops for the defined fully open / fully closed temperature set
points.
Thermal Control Design
=====================================================================
Thermal Control Concept
-----------------------
The thermal control design is driven on one side by the low heater
power availability together with the low solar intensity in the cold
case, and on the other side by the hot cases characterised by high
dissipation of the operational units and high external heat loads.
The thermal control concept mainly utilises conventional passive
components supported by active units like heaters and controlled
radiative areas, using well proven methods and classical elements.
This concept can be characterised as follows :
* Heat flows from and to the external environment are minimised using
high performance Multi-Layer Insulation (MLI).
* Most unit heat is rejected through dedicated white paint radiator,
actively controlled by louvers, located on very low Sun-illuminated
+/-Y panels.
* High internal emissivity compartments reduce structural temperature
gradients.
* Individually controlled instruments and appendages (booms, antennas
,...) are mounted thermally decoupled from the structure.
* High temperature MLI is used in the vicinity of thrusters.
* Optimised heaters, dedicated to operational, and hibernation modes,
are monitored and controlled to judiciously compensate the heat
deficit during cold environment phases.
Thermal control design
-----------------------
The thermal control subsystem (TCS) design is optimised for the
enveloping design cases of the end of life comet operations and the
aphelion hibernation. From the overall mission point of view the deep
space hibernation heater power request is the most critical thermal
design case. This heater power request is dependent on the radiator
sizing which need to be performed for worst case end of mission
conditions. The very strong heater power limitation implies that to
a certain extent constraints in the operation and/or attitude need to
be accepted for hot case.
The TCS uses a combination of selected surface finishes, heaters,
multi-layer insulation (MLI) and louvres to control the units in the
allowable temperature ranges. The units are mostly mounted on the
main +/- Y panels of the spacecraft (and +Z for experiments), with
interface fillers to enhance the conductive link to the panel for the
collectively controlled units. The individually controlled
experiments are thermally decoupled from the structure.
Generated heat by the collectively controlled units is then rejected
via conduction into the panel and subsequent radiation from the
external surface of the panel to space. These surfaces are covered
with louvers over white painted radiators minimising any absorbed
heat inputs and heat losses in cold mission phases. The louvers are
selected as baseline being the best solution (investigated during
phase B) for flexibility, qualification status and reliability.
VIRTIS and OSIRIS cameras are located at the top of the -X (anti-sun
face) so that their radiator may view deep space. The top floor is
extended over the top as a sunshield to prevent any direct solar
illumination of these instruments, while the sun angle on the -Z side
has to be limited to 80 degrees for the same reason.
Any external structural surface not required as a radiator, (or
experiment aperture) is covered with a high performance MLI blanket.
The bottom of the bus module, which is not enclosed with a structural
panel, is covered with a high performance MLI blanket used also as an
EMC screen. In the areas around thrusters, a high temperature version
of the MLI are implemented. All blankets are adequately grounded and
vented.
The bi-propellant propulsion subsystem needs to be maintained between
0 to +45 degrees throughout the mission. This is far warmer than some
units, particularly when the spacecraft is in deep space hibernation
mode. The tanks and RCS are therefore well isolated from the rest of
the spacecraft to allow their specific thermal control.
The antennae and experiment booms are passively thermally controlled
by the use of appropriate thermo-optical surface finishes and MLI.
The mechanism for the HGA has similar appropriate passive control but
also needs heaters to prevent the mechanism from freezing. It is
thermally decoupled from the rest of the spacecraft to allow its
dedicated thermal control.
The chosen solution for thermal control subsystem design uses well
known and proven technologies and concepts.
General Heater Control Concept
-------------------------------
The operation of the TCS shall enable to maintain all spacecraft
units within the required temperature range throughout the entire
mission coping with all possible spacecraft orientations and unit
mode operations.
The thermal heater concept uses the following major control features:
* Thermistor controlled (software) heater circuits, which are used to
maintain platform, avionics and payload units within operating limits
when these units are operating.
* The S/W heater design includes 3 control thermistors sited next to
each other and uses the middle temperature reading to control the
heater switching. This method is used in order to maximise the
reliability of thermistor controlling temperature.
* Thermistors will be also used to monitor the temperature at each
unit's temperature reference point (TRP) and at the System Interface
Temperature Points (STP).
* Thermostat controlled (hardware) heater circuits, which are used to
maintain platform, avionics and payload units within their non-
operating (or switch-on) limits when these units are non-operating.
These operate autonomously during satellite hibernation and Safe
modes to ensure thermal control.
* The hardware heater circuits will be controlled by one thermostat
(cold guard) connected in redundant circuit. The prime circuits
without any thermostat will be powered as long as the relevant LCL is
defined to be enabled. In the prime circuit a thermostat (hot guard)
is included to prevent from overheating. In the event of a failure in
the prime circuit the redundant circuit is automatically switched on
when the temperature falls because it is permanently enabled.
* The lower set points for the thermostats (cold guard) are at the
lower nonoperating limits of units. The hysteresis of the thermostats
is chosen to 35 degrees Celsius to limit the number of switching
cycles for the long Rosetta mission. The higher set points of the
prime thermostats (hot guard) is oriented to the upper operational
temperature limit, but will still have an appropriate margin to that
limit.
* Main and redundant heaters will be in separate foil heaters. It is
necessary to define reserved unpainted areas on all units, which
would nominally be black painted, specifically for the mounting of
heaters.
All software and hardware heaters circuits will comprise a simple
series connection of heaters with no parallel connections. The heater
concept assumes prime and redundant heater elements in different
mats. The heaters will be mounted directly onto units as this
maximises the efficiency of the heating.
The sizing of the autonomous H/W heater circuits are based upon the
following criteria:
* Payload heaters shall be designed to maintain non-operating
temperature limits at 5.33AU or switch-on limits at 3.25AU,
whichever gives the greater heater power requirement,
* Platform and Avionics units OFF in hibernation have heaters
designed to maintain non-operating temperature limits at 5.33AU
or switch-on limits at 4.5AU, whichever is the greater power
requirement,
* Platform and Avionics units ON during hibernation have heaters
designed to maintain operating temperature limits at 5.33 AU.
The suppliers of individually controlled (I/C) units shall
size their S/W and H/W heaters by themselves and may install them
where they wish in order to control their unit temperatures.
Micrometeoroid and Cometary Dust Protection
--------------------------------------------
The micrometeoroid protection used for Rosetta is composed of 2
layers of betacloth and a spacer. This protection is only applied to
the exposed +Z and -Z central tube areas of the propellant tanks as
the spacecraft honeycomb structure will form an effective shield
elsewhere.
The first betacloth layer is underneath the outermost layer of the
S/C MLI acting as a bumper. To reach the agreed probability of no
micrometeroid impacts in 998 out of 1000 strikes, a separation of 50mm
to the second betacloth layer (on top of the tank MLI) is needed. The
micrometeoroid protection is part of the overall MLI design.
The cometary dust will have a velocity similar to that of Rosetta and
so hypervelocity impacts are not an issue. Of more concern is the
coating of the spacecraft surfaces by the cometary dust. Grounding of
the external surfaces prevents differential charging but the whole
spacecraft may be charged to some potential.
Propulsion Design
=====================================================================
The propulsion subsystem is based on a pressure fed bipropellant type
using MMH (MonoMethylHydrazine) and NTO (Nitrogen TetrOxide). It is
capable to operate in both regulated and in blow-down mode and
provides a delta v of more than 2100 m/s plus attitude control. It is
able to operate in three axis and in spin stabilised mode (about the
x-axis) provided that the spin rate does not exceed 1 rpm. The
subsystem provides a high degree of redundancy in order to cope with
the special requirements of the ROSETTA mission.
The materials used in the propulsion subsystem are proven to be
compatible with the propellants and their vapours the wetted area
being mainly made of titanium or suitable stainless steel alloys.
The components and most of the pipework are installed on the
spacecraft -X panel by means of supporting brackets made of material
with low thermal conductance.
The subsystem has 24 10 N thruster for attitude and orbit control.
They are located such that they can provide pure forces and pure
torques to the spacecraft. The 24 thrusters are grouped in pairs on
the brackets, one of each pair being the main and one the redundant
thruster. The subsystem allows the operation of 8 thrusters
simultaneously.
The subsystem will be maintained within the temperature limits of the
components. The mixture ratio may be adjusted by tank temperature
(i.e. pressure) manipulation in order to enhance thruster
performance.
Operation
----------
The propulsion subsystem will be operated in regulated mode as well
as in blow down mode. The pressurisation strategy must take into
account various constraints as the available propellant, the minimum
inlet pressures for the thrusters, the maximum allowable pressures in
the propellant tanks etc. Calculations have been performed to
demonstrate the capability of the subsystem to fulfil the mission
requirements in terms of delta-v provision under the various
constraints and also with respect to the requirement for additional
20% fuel.
Telecommunication Design
=====================================================================
The Tracking, Telemetry and Command (TT & C) communications with the
Earth over the complete Rosetta mission is ensured by three antenna
concepts, operating at various stages throughout the overall
programme, combined with a number of electrical units performing
certain functions. The Telecommunication Subsystem is required to
interface with the ESA ground segment in normal operational mode and
with the NASA Deep Space Network during emergency mode.
The TT & C subsystem comprises a number of equipment's whose
descriptions appear below:
* Two Transponders interfacing with the S-Band RF Distribution Unit
(RFDU), with the High Power Amplifiers - in this case Travelling Wave
Tube Amplifiers (TWTA's) -, and with the Data Management System
(DMS). The Transponders modulate and transmit the Telemetry stream
coming from both parts of the redundant Data Management System either
in S or X-Band or both simultaneously without any interference and
transpond the ranging signal in S and X-Band. The Transponders
provide hot redundancy for the receiving functions and cold
redundancy for transmitting functions. The receivers can receive
telecommands in S-Band or X-Band (selectable per command), but not
simultaneously in both frequency bands. The configuration is such
that both receivers can receive, demodulate and send the telecommand
signal to the DMS simultaneously. The transmitters are also able to
receive the telemetry stream from both parts of the redundant DMS.
Each transponder is capable of operating in a coherent or non-
coherent mode depending on the lock status of the receiver.
* An RF Distribution Unit (RFDU) providing an S-Band transmit/receive
switching function between the antennas and the two Transponder units
via two diplexers.
* Two TWTA's providing >28W of power at X-Band to the MGA or HGA via
the Waveguide Interface Unit (WIU). The input to the TWTA HPA's is
supplied by the Transponder X-Band modulators via a 3dB passive
hybrid.
* A Waveguide Interface Unit (WIU) comprising of diplexers, two
transfer switches and high power isolators so that it is possible to
switch between antennas without turning off the TWTA.
* The transmit frequency (and receiver rest frequency) can also be
derived from an external Ultra Stable Oscillator (USO) on request by
Telecommand which may be used any time during the mission. This USO
has a superior performance compared to the Transponder internal
oscillator such that it is used for one-way ranging as part of the
Radio Science Investigations (RSI).
* Two Low Gain Antennas (LGA) providing a quasi omni directional
coverage for any attitude of the satellite which may be used for:
a)the near earth mission phase at S-Band for uplink telecommand
and downlink telemetry.
b)the telecommand Up Link at S-Band during emergency and
nominal communications over large ranges up to 6.25 AU.
* A 2.2m High Gain Antenna (HGA) providing the primary communication
for Uplink at S/X-band and Downlink at S/X-Band.
* Two Medium Gain Antennas (MGA) providing emergency Up and Downlink
default communication after sun pointing mode of the S/C is reached.
The S-Band MGA is realised as a flat patch antenna whereas the X-
Band MGA is a offset-type 0.31m reflector antenna. The MGAs also
perform some mission communications functions at various phases
throughout their lifetime due to their much larger coverage area.
High Gain Antenna Major Assembly
---------------------------------
The transmission of the high rate scientific data of the ROSETTA
spacecraft to earth is depending reliable operation of the High Gain
Antenna major assembly, which is therefore a critical element for
the mission success. The most important requirements for this
assembly are:
* High reliability
* conform to specified pointing requirements
* minimize mechanical disturbances
* comply to antenna gain requirements
The HGA Major Assembly comprises:
* HRM Hold-down and Release Mechanism for the HGA dish during
launch with three release points
* Two axes APM Antenna Pointing Mechanism (HGAPM) mounted on
a tripoid to offset the antenna from the +X panel
* A Cassegrain (X-Band) quasiparaboloid highgain Antenna (HGA)
with a dichoric subreflector and S-band primary feed
* Antenna Pointing Mechanism Electronics (APME)
* Waveguide (WG) and Rotary Joints (RJ) for the RF transmission
High Gain Antenna Frame
--------------------------------------
The Rosetta High Gain Antenna is attached to the +X side of the s/c
bus by a gimbal providing two degrees of freedom and it articulates
during flight to track Earth. Therefore, the Rosetta HGA frame,
ROS_HGA, is defined with its orientation given relative to the
ROS_SPACECRAFT frame.
The ROS_HGA frame is defined as follows:
- +Z axis is in the antenna boresight direction;
- +X axis points from the gimbal toward the antenna dish
symmetry axis;
- +Y axis completes the right hand frame;
- the origin of the frame is located at the geometric center of
the HGA dish outer rim circle.
The rotation from the spacecraft frame to the HGA frame can be
constructed using gimbal angles from telemetry by first rotating
by elevation angle about +Y axis, then rotating by azimuth about
+Z axis, and then rotating by +90 degrees about +Y axis to finally
align +Z axis with the HGA boresight.
This diagram illustrates the ROS_HGA frame:
+X s/c side (HGA side) view:
----------------------------
^
| toward comet
|
Science Deck
._____________.
.__ _______________. | | .______________ ___.
| \ \ \ | | / \ \ |
| / / \ | +Zsc | / / / |
| \ \ `. | ^ | .' \ \ |
| / / | o| | |o | / / |
| \ \ .' | | | `. \ \ |
| / / / | | | \ / / |
.__\ \_______________/ | +Xsc| | \_______________\ \__.
-Y Solar Array .______o-------> +Ysc +Y Solar Array
.__o__.
.' `.
/ \
. `. .' . +Zhga and HGA
| `o-------> +Yhga boresight are
. | . out of the page
\ | /
`. | .'
HGA ` -|- '
V +Xhga
Medium Gain Antenna (MGA)
-------------------------
The MGA design has been split into two physically separated antennae
parts:
* the MGAS operating in -S-Band frequencies,
* the MGAX operating in -X-Band frequencies,
MGA S-band (MGAS)
- - - - - - - - -
The antenna design for the S-Band subsystem consists of an array of
patch antenna elements providing a circularly symmetrical radiation
pattern. The maximum gain obtainable for this array surface area
(300mm x 300mm) ranges between 14.1 and 14.7 dBi in the receive and
transmit frequency bandwidths.
The MGAS assembly can be sub-divided into two parts, the RF active
part (radiators plus distribution network) and the support structure
(platform plus stand-offs).
The array elements are arranged in a hexagonal lattice to provide the
required symmetry to the antenna pattern. Six elements are used to
meet the required specification.
MGA X-band (MGAX)
- - - - - - - - -
The configuration of the X-band MGA (MGAX) is a single offset
parabolic reflector illuminated by a circular polarised conical horn.
Reflector dimensions are selected to reach a desired minimum gain and
to lead to a simple feeder design. This leads to an aperture diameter
of about 310mm and a focal length of 186mm (F/D = 0.6). With these
values a large reflector subtended angle is obtained which ensures
small feeder dimensions and a compact antenna design.
The MGAX antenna assembly is composed of two sub-assemblies, a
reflector and a feeder, and of a platform which supports both these
sub-assemblies and provides the interface to the Rosetta spacecraft.
The total envelope of the antenna is length=600mm, width=320mm,
height=320mm.
The thermal protection for the antenna consists of:
* White paint on the radiant face (PYROLAC 120 FD + P128)
* Thermal blankets on the rear face of reflector, feeder, supports
and platform.
Low Gain Antenna (LGA)
----------------------
Two classical S-band Low Gain Antennae (LGA) of a conical quadrifilar
helix antenna type are implemented on the satellite in opposite
direction to achieve an omnidirectional coverage. One is located at
the +Z-panel in the near of the edge to the +X panel and thus is
orientated towards the comet during the comet mission phase. The
other one is mounted on the opposite face.
Ultra Stable Oscillator
------------------------
An Ultra Stable Oscillator is implemented within the TTC subsystem
providing the required frequency stability (Allan Variance, 3s,
2.0e-13 at 38.2808642 MHz) for the RSI instrument. This USO will be
used by the TTC subsystem whenever needed and is available for RSI
measurements as well. Should the USO fail, each transponder will use
it's own oscillator (TCX0), but with less stability and not harming
the performance.
Power Design
=====================================================================
The Power Subsystem (PSS) conditions, regulates and distributes all
the electrical power required by the spacecraft throughout all phases
of the mission. Distribution involves the switching and protection of
power lines to all users, including the Avionics units and the
Payload instruments, and includes equipment power, thermal power and
keep-alive-lines. The PSS also switches, protects and distributes
power for the pyrotechnics and the thermal knives of the various
release mechanisms of the spacecraft.
Main power source for Rosetta is provided by the Solar Array
Subsystem from silicon solar cells mounted on 2 identical solar array
wings, which are deployed from the +Y and -Y faces of the spacecraft
and can be rotated to track the sun. The solar cells on the outer
panel of each wing are outward facing when in the launch (stowed)
configuration in order to provide power input to the PSS for loads
and battery recharge following separation from the launcher and prior
to array deployment.
Batteries provide power for launch and post-separation support until
the solar arrays are fully deployed and sun aligned, and thereafter
will support the main power bus as necessary to supply peak loads and
special situations during Safe Mode where the sun might not be fully
oriented towards the sun. One special feature of the power supply is
the Maximum Power Point Tracker (MPPT), which will operate the solar
array in its maximum power point in case of power shortage. During
almost all time of the mission, except for short periods of peak
power demands, the PCU will operate in nominal mode, i.e. the PCU
takes only the power required by the satellite from the solar array.
The delta power will remain in the solar array. Because of this
feature the actual performance of the array can only be assessed by
utilising 'performance strings' which operate some cells in short
circuit current mode and others in open circuit voltage mode. From
the data obtained from these cells the performance of the solar
generator can be determined.
Batteries are also the main power source for the pyrotechnics,
although pyrotechnic power is also available from the main bus as a
back-up in case there is no battery power.
The subsystem is designed in accordance to the ESA Power Standard
PSS-02-10.
Power Conditioning Unit (PCU)
-----------------------------
* Produces a fully regulated 28V single power bus from solar array
and battery inputs.
* Main bus voltage control including triple redundant error
amplifiers
* Separate hot redundant array power regulators for each array wing.
* Separate hot redundant Maximum Power Point Trackers (MPPT) for
each array wing
* Separate Battery Discharge Regulator (BDR) for each battery.
* Separate Battery Charge Regulator (BCR) for each battery.
* Array performance monitor.
* TM/TC interface.
* Some automatic functions to support power bus management.
Payload Power Distribution Unit (PL-PDU)
----------------------------------------
* Dedicated to payload power distribution.
* Fully redundant unit.
* Main bus power outlets are all switched and protected by Latching
Current Limiters (LCL).
* LCLs have current measurement and input under-voltage protection.
* 7 LCL power rating classes covering 5.5W to 135W (nominal load
capability).
* Provision of Keep Alive Lines (KALs) for experiments.
* Pyrotechnic power protection and distribution, including firing
current measurement and storage.
* Distributes power to the Thermal Control Subsystem hardware and
software controlled heaters.
* Individual on/off switching for each software controlled heater
circuit.
* TM/TC interface.
Subsystems Power Distribution Unit (SS-PDU)
-------------------------------------------
* Dedicated to Platform and Avionics power distribution.
* Fully redundant unit.
* Fold-back Current Limiters (FCL) for non-switchable loads
(Receivers and CDMUs).
* All other main bus power outlets are switched and protected by
Latching Current Limiters (LCL).
* FCLs and LCLs have current measurement and FCLs have input under-
voltage protection.
* LCL classes and power ratings as for PL-PDU.
* Pyrotechnic power protection and distribution, including firing
current measurement and storage.
* Thermal Knives (TKs) power distribution (for Solar Array panels
release).
* Distributes power to the Thermal Control Subsystem combined
hardware - software controlled heaters.
* Individual on/off switching for each software controlled heater
circuit.
* TM/TC interface.
Batteries
----------
* 3 batteries each comprising 6 series and 11 parallel connected Li-
Ion 1.5 Ah cells (corresponds to 16.5 Ah per battery).
* Power and monitoring connections to PCU.
* Power connections also to the PDUs for the pyrotechnics.
* Cells arrangement and wiring to minimise magnetic moment.
* 1 thermistors per battery for battery charge/discharge control.
* A combination of relay/heater mat in order to discharge the
batteries for capacitance verification.
Solar Array Generator
----------------------
The orbit of the S/C has an extremely wide variation of Spacecraft-
Earth-Sun angles and distances, hence it is mandatory to include an
electrical design based on LILT (Low Intensity Low Temperature) solar
cell technology.
The structural parts/units (deployment system, substrates, hold-down
& release system) are identical to the qualified ARA MK3 design of
Fokker Space.
The geometry and mechanical interface definition of the Rosetta
baseline Solar Array design is identical to the 5-panel qualification
wing.
The electrical architecture (cells, strings, sections & harness lay-
out) is uniquely designed for Rosetta. Electro static discharge (ESD)
protection design is qualified for the ARA MK3 type solar array.
The baseline are 2 solar arrays, each with a full silicon 5-panel
wing, with panel sizes as used in the ARA MK3 5-panel qualification
wing (about 5.3 m2 per panel).
x-------x
x---.---.---.---.---x | | x---.---.---.---.---x
| | | | | |--| x |--| | | | | |
x---'---'---'---'---x | | x---'---'---'---'---x
x-------x
Mechanical Design of the Solar Panels
--------------------------------------
The basic skin design of the panels of the solar arrays consists of
two layers [0/90degres] M55J/950-1 CFRP prepreg (thickness per layer
0.06 mm) in closed lay-up. The panel substrate dimensions are 2.25 x
2.736 m2. The front side skin will use a 50^m Kapton foil to isolate
the solar cell network from the conductive CFRP layers. The Kapton
foil is co-cured with the CFRP layers.
The panel core consists of Aluminium honeycomb with a core height of
22 mm. Local circular reinforcement plugs ('subassembly panels') are
used to provide the holddown areas with extra strength, stiffness and
fatigue resistance.
The hold-down and release system uses a tie-down element (Kevlar
cable) under high preload which will be degraded by heat of the
thermal knife for release. The hold-down, SADM and yoke snubber
locations for Rosetta are fully identical to the ARA MK3
qualification hardware definition.
The stowed wing has a height of <239 mm at the wing tips (the gap
between inner panel and sidewall is increased from nominal 70 mm by
about 30mm by means of a dedicated bracket, the inter panel gap is 12
mm, and the panel substrate thickness is 22 mm).
The deployment mechanism concept relies on spring-driven hinges. The
spring characteristics are chosen such that the energy supply is
enough for the full range up to 5 maximum sized panels, while
maintaining the required deployment safety factors. In order to
reduce the shock loads on the SADM and inter-panel hinges, a damper
is introduced in the deployment system.
A stiff synchronisation system is applied to prevent a very non-
synchronous deployment, resulting in unpredictable high deployment
latch-up shocks at the interpanel hinges.
The V-yoke length is 1103 mm when measured from SADM hinge-line to
yoke/inner panel hinge-line. The yoke length used within the ARAFOM
5-panel QM wing programme is identical.
The arms of the V-shaped yoke consist of M46J CFRP filament wound
with a circular cross section (inner diameter 43 mm; nominal wall
thickness 0.9 mm) with reinforcements at the ends of the yoke tubes.
Rosetta Solar Array Frames
--------------------------------------
The Rosetta solar arrays can be articulated (each having one degree
of freedom), the solar Array frames, ROS_SA+Y and ROS_SA-Y, are
defined with their orientation given relative to the ROS_SPACECRAFT
frame.
Both array frames are defined as follows :
- +Y axis is parallel to the longest side of the array,
positively oriented from the end of the wing toward the
gimbal;
- +Z axis is normal to the solar array plane, the solar cells
on the +Z side;
- +X axis is defined such that (X,Y,Z) is right handed;
- the origin of the frame is located at the geometric center
of the gimbal.
The axis of rotation is parallel to the Y axis of the spacecraft and
solar array frames.
At zero (reference) position the array wing is aligned such that the
array surface is in the spacecraft Y-Z plane, with the face (cells)
aligned such that the array normal is parallel to the +X axis of the
spacecraft. This means that in stowed configuration (i.e. launch
configuration) the array position of the array on the +Y panel is -90
degrees and on the -Y panel +90 degrees.
This diagram illustrates the ROS_SA+Y and ROS_SA-Y frames:
+X s/c side (HGA side) view:
----------------------------
^
| toward comet
|
Science Deck +Xsa+y0
._____________.^+Xsa+y
.__ _______________. | || .______________ ___.
| \ \ \ | || / \ \ |
| / / \ | +Zsc || / / / |
| \ \ `. | ^ ||.+Zsa+y0 \ \ |
| / / +Zsa-y0 o-----> | <-----o Zsa+y / / |
| \ \ +Zsa-y.'|+Ysa-y0|+Ysa+y0 `. \ \ |
| / / / ||+Ysa-y|+Ysa+y| \ / / |
.__\ \_______________/ || | | \_______________\ \__.
-Y Solar Array |.______o-------> +Ysc +Y Solar Array
v +Xsc o__.
+Xsa-y0 .' `.
+Xsa-y / \
. `. .' . +Zsa+y0, +Zsa+y, +Zsa-y0,
| `o' | and +Zsa-y are out of
. | . the page
\ | /
`. .' Active solar cell is
HGA ` --- ' facing the viewer
Power Constraints in Deep Space
=====================================================================
In the phases with Sun distances above approximately 4.0 AU the
decreasing solar array power forces the use of economical strategies
for certain operations. Thereby the situation after the deep space
hibernation phase is much more severe. From radiation degradation
analysis it has been derived that after DSHM at 4.5 AU about 65 W
less solar array power will be available compared to 4.5 AU before
DSHM. This corresponds to about 13% of the power needed at that
distance.
In the deep space phases the general operational concept is the
following:
* minimise the overall power consumption by switching off all
equipment not directly needed during the current operation
* additionally, for certain operations with high extra power
demand, perform a power sharing strategy by switching off some TCS
heaters; as a consequence this puts a time limit on such operations
* operate equipment like RWs and SSMM in reduced power mode
* for autonomous operations, which are not directly under ground
control, like in Safe Mode, the ground can set a Low Power Flag as
invocation parameter in the call of the Safe Mode OBCP (which is
loaded in the System Init Table) at the appropriate time in the
mission, according to the current Sun distance. This flag will be
checked by the OBCP; if the flag is set, the Safe Mode downlink
will be performed in power sharing strategy and the SSMM is set
into stand-by mode (memory modules remain powered, but memory
controllers are switched off).
As a safety precaution the battery discharge alarm shall remain
enabled all the time. This will allow for nominal short (< 4 min)
peak power demands to be satisfied by the batteries, e.g. for RW
offloading, but will trigger a system alarm and transition to Safe
Mode in case of a creeping battery discharge due to a wrong power
configuration e.g. because of a missed command. If for such a case a
processor reconfiguration is not desired, it is possible to use the
monitoring of the MEA Voltage to trigger transition into Safe Mode
before the battery discharge alarm triggers (see Handling of On-board
Monitoring, [RO-DSS-TN-1155]).
Harness Design
=====================================================================
The harness performs the electrical connection between all
electrical and electronic equipment in the ROSETTA spacecraft. It
provides distribution and separation of power supplies, signals,
scientific data lines, pyrotechnic firing pulses, and all connections
to the umbilical, safe/arm brackets/connectors and test connectors.
The harness consists of the following subassemblies:
* Payload Support Module Harness
* Bus Support Module Harness
* Harness to the Lander I/F
Furthermore the harness / cables are divided into three harness EMC
classes: power, signal and data, and the pyro harness. Their routing
is physically separated. In addition to the appropriate twisting and
shielding techniques this minimises the probability of electrical
cross talking of critical lines.
The harness design follows a distributed single point grounding
scheme. Redundant functions have their own connectors and are routed
in separate bundles and in a different way as far as practical.
All connectors supplying power have female contacts.
To achieve a complete Faraday cage around the harness each of the
harnesses has its own overall shield made of aluminium tape with an
overlap of at least 50 % for harnesses within the spacecraft and a
double shield for harnesses outside the spacecraft. As fixation
points for the harness aluminium bases (Ty-bases) are bonded to the
structure with a two component conductive glue. The distance of the
Ty-bases is selected such that the harness withstands all specified
environmental conditions.
To avoid interruptions of the shield between the connector and the
overall shield, redundant connection wires are used between connector
case and harness overall shield. In case of pyro-lines and sensible
interfaces conductive connector boots are implemented.
To prevent contamination the harness was baked-out in a thermal
vacuum chamber prior to integration.
Avionics Design
=====================================================================
The ROSETTA Avionics consists of the Data Management Subsystem (DMS)
and the Attitude and Orbit Control and Measurement Subsystem (AOCMS)
functions.
Data Management Subsystem (DMS)
-----------------------------------------------
The data management subsystem is in charge of telecommand
distribution to other spacecraft subsystems and payload, of
telemetry data collection from spacecraft subsystems and payload and
formatting, and of overall supervision of spacecraft and payload
functions and health.
The DMS is based on a standard OBDH bus architecture enhanced by high
rate IEEE 1355 serial data link between the different Avionics
processors and the SSMM, STR and CAM. The OBDH bus is the data route
for data acquisition and commands distribution via the RTUs. Payload
Instruments are accessed via a dedicated Payload RTU. Subsystems are
accessed via a dedicated Subsystem RTU.
DMS includes 4 identical Processor Modules (PM) located in 2 CDMUs.
Any of the processor modules can perform either the DMS or the AOCMS
processing. The PM selected for the DMS function acts as the bus
master. It is also in charge of Platform subsystem management (TTC,
Power, Thermal). The one selected as the AOCMS computer is in charge
of all sensors, actuators, HGA & SA drive electronics. TCdecoder and
Transfer Frame Generator (TFG) are included in each CDMU.
Telemetry can be downlinked via the TFG using the real time channel
(VC0) or in form of retrievals from the SSMM (VC1).
Solid State Mass Memory (SSMM)
- - - - - - - - - - - - - - - -
The Solid State Mass Memory (SSMM) is used like a 'Hard Disk Storage'
including 25 Gbit of memory. It contains a data compression module
which allows lossy (for CAM image) and loss-less (for HK and science
data) compression of data to be stored. It is able of file management
capability. It stores CAM images, science and telemetry packets as
well as software data for the AOCMS and DMS computer.
It is coupled to:
* the 4 processors via an IEEE 1355 link,
* the TFGs of the 2 CDMUs via a serial link,
* VIRTIS, OSIRIS and the Navigation Camera via a high data rate
serial link (IEEE 1355)
* the High Power Command Module (HPCM) selecting the valid PM
The lossy compression method (WAVELET) will be used for image data
compression of the NAVCAM or STR. The degree of compression can be
set by filter parameters from ground. The compression of OSIRIS and
VIRTIS image data could also be performed inside the SSMM. Present
baseline however is that these two instruments do not request data
compression from the system.
The SSMM SW runs on a Digital Signal Processor. The SSMM SW is made
of:
* The Init Mode Software
The Init mode software ensures the boot up of the SSMM and the
establishment of the communication with the DMS SW. It allows the
loading of the operational SW from EEPROM to RAM, and its starting.
* The Operational Software
The operational SW manages the files located in the Memory Modules of
SSMM, and the Data Compression Function that performs Rice lossless
and Wavelet lossy data compression.
The functionality of the SSMM can be summarised with the three points
below.
* Store on-board data in files. The on-board data can be both
scientific data and software images in files.
* Transmit the data stored in SSMM files to either an on-board User
or to the ground.
* Compress the stored files using both lossy and lossless compression
algorithms.
The Rosetta Solid State Mass Memory (SSMM) functionally consists of
the following modules:
* 2 Memory Controllers (MC)
* 3 Memory Modules (MM)
* 2 Power Converters, which supplies power to the memory controller
and memory module boards.
The Memory Controllers are responsible for all data transfer to and
from the Mass Memory, compression of data in the mass memory and
basic housekeeping functions (collection of telemetry packets,
configuration of the SSMM etc.). The Memory Controllers work in cold
redundancy.
The three Memory Modules are where the files are stored. The modules
can be turned on and off independently, giving the possibility to
increase and decrease the storage capacity of the SSMM. The Memory
Controllers access the Memory Modules via a memory module bus. Both
the Memory Controllers can access all three Memory Modules.
Attitude and Orbit Control Measurement System (AOCMS)
-----------------------------------------------------
The AOCMS is in charge of attitude and orbit measurement and control
and is in charge with sensors and actuators for autonomous attitude
determination and control as well as pre-programmed manoeuvring.
The AOCMS uses a decentralised architecture built around the AOCMS
Interface Unit (AIU) linked to all sensors / actuators and to the
Processor Modules included in the CDMUs:
* the AOCMS sensors: 2 Navigation Cameras (CAM) and 2 Star Trackers
(STR) having a common electronics unit, 4 Sun Acquisition Sensors
(SAS) and 3 Inertial Measurement Packages (3 IMP, each including 3
gyros + 3 acceleros),
* the AOCMS actuators: the Reaction Wheel Assembly (RWA), and
belonging to the Platform the Reaction Control System (RCS), the High
Gain Antenna Pointing Mechanism (HGAPM), and the 2 Solar Array Drive
Mechanisms (SADM).
AOCMS PM communication with AOCMS sensors (IMP, SAS, STR, CAM) and
actuators (RWA, RCS), and with pointing mechanism electronics
(SADE and HGAPE) is performed through the AIU. Functional AOCMS data
which need to be put in the Telemetry and sent to the ground are
given packetised by the AOCMS processor and sent to the DMS processor
for futher downlink to ground and storage in the SSMM.
The DMS PM permanently checks the AOCMS health by monitoring that the
AOCMS PM does not stop to communicate with DMS PM. This is done by
checking the correct reception of the so-called 'essential' AOCMS HK
packet every one second.
The AIU is the central data acquisition and distribution unit which
allows access to the sensors and actuators with different type of
interfaces. It includes RS 422, IEEE 1355 and MACS Bus interfaces as
well as analog and discrete digital interfaces for commanding and
data acquisition.
The AIU includes furthermore a 12 bit A/D converter in order to
convert analog signals from the pressure transducers (temperature and
pressure) precise enough for the fuel level prediction on-board of
Rosetta late in the mission, when the fuel level is critical.
The major AOCMS components are the following:
* AOCMS Interface Unit (AIU): it interfaces to all AOCMS sensors and
actuators
* The Sun Acquisition Sensors (SAS): they are internally redundant
and are used for Sun Acquisition and pointing. They provide full sky
coverage and ensure a permanent sensing of the Sun direction vector.
* The Inertial Measurement Packages (IMP): The IMP function provides
roll rate and velocity measurements along 3 orthogonal axes.
* 4 Reaction Wheels: they are arranged in the Reaction Wheel Assembly
(RWA) and the Reaction Control System (RCS), in a tetrahedral
configuration about the S/C Y-axis in order to enhance the torque and
momentum capacity about that axis for the asteroid fly-by.
* 2 Autonomous Star Trackers: they contain an Autonomous Star Pattern
Recognition function and provide autonomously to the AOCMS an
estimated attitude quaternion and stellar measurements data.
* 2 Navigation Cameras (A&B) are used in the AOCMS control loop
during the Asteroid Near Fly-by Phase. The navigation cameras can
also directly send image data to the SSMM through a high data rate
link.
* Pointing mechanisms (through target pointing angles) and propulsion
thruster valves are commanded by the AOCMS through the AIU links.
Avionics external interface
----------------------------------------------
The Avionics system has the following external interface to other
subsystems of the Rosetta spacecraft:
* Interface with the Ground through TTC Subsystem:
Ground Telecommands (TC) are checked, decoded and executed
internally or sent to other subsystems, Telemetry (TM) data
generated on-board are collected, formatted (if needed) and sent to
Ground through TTC S/S, either in real time or in play-back after
storage in SSMM, on ground request.
* Interface with Platform and Payload:
The Avionics provides the experiments and Platform equipment with a
hardware command capability (power On/Off commands, heater On/Off
commands...),
The Avionics provides experiments with a time synchronisation
capability, so that the Ground can later on correlate results
coming from different experiments,
The Avionics uses for attitude and communication control purpose as
well as for power generation Platform equipment: Reaction Control
System (RCS), High Gain Antenna and Solar Array Pointing Mechanisms
(HGAPM, SADM)
Housekeeping data and experiment science data are collected
on-board to be sent to Ground in real time TM, or to be stored for
play-back downlink,
The Avionics S/W provides experiments and Platform with a
processing capability, in form of application programs (AP) or
On-board Control Procedures (OBCP), coded and implemented by the
Avionics/OBCP contractor, but specified by the users to allow
montoring/surveillance, thermal control, experiment or mechanism
management.
Avionics modes
=====================================================================
The Avionics modes derived from the AOCMS modes are the following:
Stand-By Mode
--------------
The SBM is used in Pre-launch and Launch Modes for general check
supervision. Only DMS functions are activated. It is possible to
command thrusters through AIU for RCS Priming.
Sun Acquisition Mode
---------------------
This mode is used during Separation Sequence to perform rate
reduction (if necessary), Sun acquisition and Sun pointing. SAM is
also used as second level back-up mode to recover Sun pointing
attitude in case of an unsuccessful back-up to Sun Keeping Mode.
Safe/Hold Mode
---------------
The SHM follows the Sun Acquisition Mode / Sun Keeping Mode to
achieve a 3-axis attitude based on star trackers, gyros and reaction
wheels, with solar arrays pointing towards the Sun and Medium and
High Gain Antennae (i.e. S/C Xaxis) pointing towards the Earth and
the Y-axis normally pointing to the noth of the ecliptic plane.
In some mission phases (i.e. defined by the minimum earth distance),
S/C X-axis pointing towards the Earth is forbidden because of thermal
constraints. Then, +X axis is pointed towards the Sun, and the High
Gain Antenna is pointed towards the Earth.
Normal Mode
------------
The NM is used in Active Cruise and Near Comet phases for nominal
longterm operations, for comet observation and SSP delivery. Reaction
wheel off-loading is a function of the Normal Mode.
Thruster Transition Mode
-------------------------
The TTM is used for transition from Normal Mode to operational
thruster Modes, and vice-versa, for control tranquillisation.
Orbit Control Mode
------------------
The OCM is used in Active Cruise Mode for trajectory and orbit
corrections.
Asteroid Fly-By Mode
--------------------
The AFB mode is dedicated to asteroid observation.
Near Sun Hibernation Mode
-------------------------
The NSHM is a 3-axis controlled mode (with the attitude estimation
based on the use of STR only, and no gyro), with a dedicated thruster
control (i.e. single sided) to minimise the fuel consumption.
Spin-up Mode
------------
The SpM is necessary to spin up the spacecraft at hibernation entry
(spin down at hibernation exit is achieved by Sun Keeping Mode). The
attitude control concept is a completely passive inertial spin during
the deep space hibernation phase.
There is no AOCMS Deep Space Hibernation Mode.
Sun Keeping Mode
----------------
The Sun Keeping Mode is used nominally at wake-up after Deep Space
hibernation, and as first level back-up mode to recover Sun pointing
attitude in case of a failure involving the Avionics and for which a
local reconfiguration on redundant units is not efficient. In case
the autonomous entry to Safe / Hold Mode is disabled or not
successful Earth Strobing Mode is established leading to a slow spin
motion around the Sun direction. Then the + X-axis is pointed towards
the expected earth direction (i.e. using the actual Sun/spacecraft/
Earth angle). The rotation along the Sun line is maintained therefore
the Earth crosses once per revolution the + X-axis which will allow
communication with the MGA.
System Level Modes
=====================================================================
A basic conficuration of the system level modes is given below:
Pre-launch only DMS on, AOCMS PM on, external power supply
Mode
Launch Mode Initially: DMS on, SSMM in standby with 1 MM,
AOCMS PM on, separation sequence program running,
power supply from batteries Finally: DMS on, AOCMS
in Sun Acquisition Mode, TTC S-band downlink on,
power supply from solar arrays, X-axis and solar
arrays Sun pointing.
Activation DMS on, AOCMS in Normal Mode, TTC S- or X-band
Mode downlink via HGA (initially in S-band via LGA),
3-axis stabilised, SA Sun pointing attitude
Active Cruise DMS on, AOCMS in Normal Mode or Orbit Control
Mode Mode, TTC S- or X-band downlink via HGA, 3-axis
stabilised, SA Sun pointing attitude
Deep Space CDMU on, AOCMS in SBM mode, inertial spin
Hibernation stabilisation mode, wake-up timers on, thermostat
Mode control of heaters
Near Sun DMS on, AOCMS in NSHM, 3-axis active control mode
Hibernation with 2 PMs, star tracker, thrusters, X-axis Sun or
Mode Earth pointing
Asteroid DMS on, TTC X-band downlink via HGA, SA Sun
Fly-by Mode pointing, payload on, AOCMS in AFM mode: closed loop
asteroid tracking with navigation camera, during Near
Fly-by: HGA tracking stopped
Near Comet DMS on, TTC X-band downlink via HGA, navigation
Mode camera and payload on, AOCMS in Normal Mode: 3-axis
stabilised, SA Sun pointing, instruments comet
pointing;
Safe Mode DMS on, AOCMS in Safe/Hold Mode; SA Sun pointing, X-
axis Sun or Earth pointing, 3-axis stabilised using
gyros, star tracker, RWs(if enabled by ground); TTC
S-Band downlink via HGA; RXs on HGA/LGA; payload off
Survival Mode DMS on, AOCMS in SKM submode 'MGA Strobing' (or in
SKM if this submode is disabled), SA Sun pointing
with offset from +X-axis = SSCE angle, fixed small
residual rate around Sun vector; control by
thrusters, Sun sensors, gyros; S-Band carrier
downlink via MGA, RXs on MGA/LGA, load off
Ground Segment
=====================================================================
Ground Station and Communications Network performing telemetry,
telecommand and tracking operations within the S/X-band frequencies.
Telecommand will always be in the S-band, whilst telemetry will be
switchable between S- and X-band, with the possibility to transmit
simultaneously in both frequency bands, only one of which will be
modulated (S-band down-link is primarily used during the near Earth
mission phases). The ground station used throughout all mission
phases will be the ESA Perth 32m deep-space terminal (complemented by
the ESA Kourou 15m station during near-Earth mission phases). In
addition, the NASA Deep Space Network (DSN) 34m and/or 70m network is
envisaged for back-up and emergency cases.
New Norcia Dur. Start-Date End-Date
--------------------------------------------------
NNO Daily 129d 26/02/04 03/07/04
NNO Weekly 64d 04/07/04 05/09/04
NNO Daily 56d 06/09/04 31/10/04
NNO Weekly 61d 01/11/04 31/12/04
NNO Weekly 30d 01/01/05 30/01/05
NNO Daily 116d 31/01/05 26/05/05
NNO Daily 52d 27/05/05 17/07/05
NNO Weekly 63d 18/07/05 18/09/05
NNO Daily 7d 19/09/05 25/09/05
NNO Weekly 21d 26/09/05 16/10/05
NNO Daily 7d 17/10/05 23/10/05
NNO Weekly 28d 24/10/05 20/11/05
NNO Monthly 41d 21/11/05 31/12/05
NNO Monthly 50d 01/01/06 19/02/06
NNO Daily 16d 20/02/06 07/03/06
NNO Weekly 13d 08/03/06 20/03/06
NNO Daily 48d 21/03/06 07/05/06
NNO Weekly 14d 08/05/06 21/05/06
NNO Daily 3d 22/05/06 24/05/06
NNO Weekly 28d 25/05/06 21/06/06
NNO Monthly 32d 22/06/06 23/07/06
NNO Weekly 35d 24/07/06 27/08/06
NNO Daily 63d 28/08/06 29/10/06
NNO Weekly 28d 30/10/06 26/11/06
NNO Daily 28d 27/11/06 24/12/06
NNO Weekly 7d 25/12/06 31/12/06
NNO Weekly 31d 01/01/07 31/01/07
NNO Daily 122d 01/02/07 02/06/07
NNO Weekly 28d 03/06/07 30/06/07
NNO Monthly 71d 01/07/07 09/09/07
NNO Weekly 21d 10/09/07 30/09/07
NNO Daily 74d 01/10/07 13/12/07
NNO Weekly 18d 14/12/07 31/12/07
NNO Weekly 10d 01/01/08 10/01/08
NNO Daily 7d 11/01/08 17/01/08
NNO Weekly 28d 18/01/08 14/02/08
NNO Monthly 136d 15/02/08 29/06/08
NNO Daily 129d 30/06/08 05/11/08
NNO Weekly 56d 06/11/08 31/12/08
NNO Weekly 21d 01/01/09 21/01/09
NNO Weekly 28d 22/01/09 18/02/09
NNO Daily 65d 19/02/09 24/04/09
NNO Weekly 28d 25/04/09 22/05/09
NNO Monthly 105d 23/05/09 04/09/09
NNO Weekly 28d 05/09/09 02/10/09
NNO Daily 79d 01/10/09 18/12/09
NNO Weekly 13d 19/12/09 31/12/09
NNO Daily 63d 01/01/10 04/03/10
NNO Monthly 62d 05/03/10 05/05/10
NNO Daily 144d 06/05/10 26/09/10
NNO Weekly 42d 27/09/10 07/11/10
NNO Daily 54d 08/11/10 31/12/10
NNO Daily 102d 01/01/11 12/04/11
NNO Weekly 37d 13/04/11 19/05/11
NNO Daily 55d 20/05/11 13/07/11
NNO Daily 343d 23/01/14 31/12/14
NNO Daily 365d 01/01/15 31/12/15
Cebreros
---------------------
Support of the ESA Cebreros ground station is scheduled for 90 days
between the 18-Aug-2014 and the 15-Nov-2014 to support comet
characterization and Lander delivery.
Kourou Dur. Start-Date End-Date
---------------------------------------------------
Kourou 1 14d 26/02/2004 11/03/2004
Kourou 2 30d 04/02/2005 05/03/2005
Kourou 3 30d 22/10/2007 20/11/2007
Kourou 4 30d 22/10/2009 20/11/2009
The support around the Earth swing-by is limited to a few passes
close to the swing-by and a few weekly passes prior to the swing-by
to verify the compatibility between the ground station and the
spacecraft.
NASA DSN Dur. Start-Date End-Date
--------------------------------------------------
DSN1 14d 26/02/04 10/03/04
DSN2 93d 26/02/04 29/05/04
DSN3 7d 03/06/04 09/06/04
DSN4 42d 06/09/04 17/10/04
DSN5 30d 17/02/05 18/03/05
DDOR Check 14d 07/08/06 20/08/06
DSN6 38d 01/09/06 08/10/06
DDOR1 14d 09/10/06 22/10/06
DSN7 155d 23/10/06 26/03/07
DSN8 30d 31/10/07 29/11/07
DSN9 40d 08/08/08 16/09/08
DSN10 30d 28/10/09 26/11/09
DSN11 40d 12/06/10 21/07/10
DSN12 115d 10/11/10 04/03/11
DSN13 30d 05/03/11 03/04/11
DSN14 153d 23/01/14 24/06/14
DSN15 34d 23/07/14 25/08/14
DSN16 28d 25/10/14 21/11/14
Acronyms
------------------------------
For more acronyms refer to Rosetta Project Glossary [RO-EST-LI-5012]
AFB Asteroid Fly-By
AFM Asteroid Fly-by Mode
AIU AOCMS Interface Unit
AOCMS Attitude and Orbit Control Measurement System
AOCS Attitude and Orbit Control System
AP Application Programs
APM Antenna Pointing Mechanism
APME APM Electronics
APM-M APM Motor
APM-SS APM Support Structure
ARA Attitude Reference Assembly
AU Astronomical Unit
BCR Battery Charge Regulator
BDR Battery Discharge Regulator
BSM Bus Support Module
CAM Navigation Camera
CAP Comet Acquisition Point
CAT Close Approach Trajectory
CDMU Control and Data Management Unit
CFRP Carbon Fibre Reinforced Plastic
CNES Centre National d'Etudes Spatiales
COP Close Observation Phase
DDOR Delta Differential One-way Range
DLR German Aerospace Center
DMS Data Management Subsystem
DSHM Deep Space Hibernation Mode
DSM Deep Space Manouver
DSN Deep Space Network
EEPROM Electronically Erasable Programmable Read-Only Memory
EMC Electromagnetic Compatibility
ESA European Space Agency
ESD Electro Static Discharge
ESOC European Space Operations Center
ESTEC European Space Research and Technology Center
EUV Extreme UltraViolet
FAT Far approach trajectory
FCL Fold-back Current Limiters
FDIR Failure Detection Isolation and Recovery
F/D Focal Diameter
FOV Field Of View
FUV Far UltraViolet
GCMS Gas Chromatography / Mass Spectrometry
GMP Global Mapping Phase
HDRM Hold-Down and Release Mechanism
HGA High Gain Antenna
HGAPE High Gain Antenna Pointing Electronics
HGAPM High Gain Antenna Pointing Mechanism
HgCdTe Mercury Cadmium Telluride
HIGH High Activity Phase (Escort Phase)
HPA High Power Amplifier
HPCM High Power Command Module
HK HouseKeeping
I/C Individually Controlled
I/F InterFace
IMP Inertial Measurement Packages
IMU INERTIAL MEASUREMENT UNITS
IRAS InfraRed Astronomical Satellite
IRFPA InfraRed Focal Plane Array
IS Infrared Spectrometer
HRM HGA Holddown & Release Mechanism
H/W Hard/Ware
KAL Keep Alive Lines
LCC Lander Control Center
LCL Latching Current Limiters
LEOP Launch and Early Orbit Phase
LGA Low Gain Antenna
LILT Low Intensity Low Temperature
LIP Lander Interface Panel
LOW Low Activity Phase (Escort Phase)
MACS Modular Attitude Control System
MEA Main Electronics Assembly
MC Memory Controlller
MGA Medium Gain Antenna
MGAS MGA S-band
MGAX MGA X-band
MINC Moderate Increase Phase (Escort Phase)
MLI Multi Layer Insulation
MM Memory Module
MMH MonoMethylHydrazine
MPPT Maximum Power Point Trackers
MS Microscope
NM Normal Mode
NNO New Norcia ground station
NSHM Near Sun Hibernation Mode
NTO Nitrogen TetrOxide
OBCP On-Board Control Procedures
OBDH On-Board Data Handling
OCM Orbit Control Mode
OIP Orbit Insertion Point
PCU Power Conditioning Unit
PDU Power Distribution Unit
PI Principal Investigator
P/L PayLoad
PL-PDU Payload Power Distribution Unit
PM Processor Module
PSM Payload Support Module
PSS Power SubSystem
RAM Random Access Memory
RCS Reaction Control System
RF Radio Frequency
RFDU RF Distribution Unit
RJ Rotary Joints
RMOC Rosetta Mission Operations Center
RL Rosetta Lander
RLGS Rosetta Lander Ground Segment
RO Rosetta Orbiter
RSI Radio Science Investigations
RSOC Rosetta Science Operations CenterRTU
RVM Rendez-vous Manouver
RW Reaction Wheel
RWA Reaction Wheel Assembly
SA Solar Array
SADE Solar Array Drive Electronics
SADM Solar Array Drive Mechanism
SAM Sun Acquisition Mode
SAS Sun Acquisition Sensors
SBM Stand-By Mode
SHM Safe/Hold Mode
SAS Sun Acquisition Sensor
S/C SpaceCraft
SI Silicon
SINC Sharp Increase Phase (Escort Phase)
STP System Interface Temperature Points
SKM Sun Keeping Mode
SONC Science Operations and Navigation Center
SpM Spin-up Mode
S/S SubSystem
SSMM Solid State Mass Memory
SSP Surface Science Package
SS-PDU Subsystems Power Distribution Unit
STR Star TRacker
S/W SoftWare
SWT Sience Working Team
TC Telecommand
TC Telecommunications
TCS Thermal Control Subsystem
TFG Transfer Frame Generator
TGM Transition to global mapping
TK Thermal Knives
TM Telemetry
TRP Temperature Reference Point
TTC Tracking, Telemetry and Command
TTM Thruster Transition Mode
TWTL Two Way Travelling Lighttime
TWTA Travelling Wave Tube Amplifiers
USO Ultra Stable Oscillator
VC Virtual Channel
WG WaveGuide
WIU Waveguide Interface Unit
"
END_OBJECT = INSTRUMENT_HOST_INFORMATION
/********** REFERENCES **************/
OBJECT = INSTRUMENT_HOST_REFERENCE_INFO
REFERENCE_KEY_ID = "RO-DSS-TN-1155"
END_OBJECT = INSTRUMENT_HOST_REFERENCE_INFO
OBJECT = INSTRUMENT_HOST_REFERENCE_INFO
REFERENCE_KEY_ID = "PSS-02-10"
END_OBJECT = INSTRUMENT_HOST_REFERENCE_INFO
OBJECT = INSTRUMENT_HOST_REFERENCE_INFO
REFERENCE_KEY_ID = "RO-EST-LI-5012"
END_OBJECT = INSTRUMENT_HOST_REFERENCE_INFO
END_OBJECT = INSTRUMENT_HOST
/****************** LANDER PHILAE ************************/
OBJECT = INSTRUMENT_HOST
INSTRUMENT_HOST_ID = RL
OBJECT = INSTRUMENT_HOST_INFORMATION
INSTRUMENT_HOST_NAME = "ROSETTA-LANDER"
INSTRUMENT_HOST_TYPE = SPACECRAFT
INSTRUMENT_HOST_DESC = "
Lander overview
=============================================
The Philae Lander is a box-type unit with the dimensions
of 850 x 850 x 640 mm3. On the comet, it will rest on a tripod
called Landing Gear, with a diameter of 2.6 m and will be fixed to
the comet's surface by harpoons.
Philae is composed of three different parts, corresponding to its
structural design:
1) Internal compartment:
This compartment hosts almost all subsystems and most of the
experiment units. It provides a temperature controlled environment
for all electronics and is built by the structural elements of an
Instrument platform and so called Pi-plates. It is surrounded by
Multilayer Insulation built of 2 tents to achieve the required
insulation at a low power environment on the comet at 3 AU distance
from Sun.
2) Solar Hood:
The solar hood is built around the internal compartment and its MLI
tents, the shape follows the overall Lander shape. It hosts the solar
arrays of the Lander composed by 6 different panels. In addition two
absorber foils are mounted on the solar hood lid. These foils are
built by thin copper foils with an external TINOX surface, high
absorptivity and low emissivity, used to collect solar irradiation
and transform it into heat radiated into the internal compartment.
The solar hood also carries the camera system of the Lander, with one
camera head on each panel, thus providing a 360 degrees panoramic
view.
3) Baseplate / Balcony:
The baseplate is the central structural plate carrying the solar hood
with the internal compartment underneath and providing at one end a
special area called balcony. This area hosts all experiments or parts
of them, especially the sensors, which require direct access to the
comet environment and the comet surface.
The baseplate is also the interface panel to the Landing Gear.
In addition the baseplate hosts the Push plate, which is the
interface to the Orbiter during the 10 years cruise from Launch to
the Comet.
The Lander mass is around 100 kg.
In addition three units of the Lander system are mounted on the
Orbiter, and will remain there after Lander separation for the comet.
These units provide the interfaces to the Orbiter: electrical and
data (ESS) and mechanical (MSS). The third system is a TxRx system
used to keep contact to the Lander during its operational phase on
the comet.
Lander Mission Requirements and Constraints
=============================================
The Lander is designed to fullfill the mission requirements given as:
- survive the 10 years cruise phase with long hibernation phases under
autonomous thermal control powered by the Orbiter,
- land safely on the comet,
- provide a scientific phase after landing at 3 AU distance from Sun
with online data transmission,
- provide a long term mission capability observing the comet on its
way from 3 AU to the Sun
Lander Platform Definition
=============================================
The Lander platform is built by three major subsystems, required to
operate the Lander throughout the mission:
- a Power subsystem (PSS) composed of a Battery system with a
Primary Battery and a Secondary Battery, the later refilled
by a Solar array generator, and the required electronics to
distribute and control the power flow inside the Lander,
- a Central Data Management System (CDMS), composed by two hot
redundant computers, controlling all activities on the
Lander, especially on the comet in an autonomous manner,
- a Thermal Control System, composed by a 2-tent
MultiLayerInsulation supported by two absorber foils and an
electrical heater system. Additional independant heater
systems are used during the cruise phase, especially when the
Lander is in hibernation, and on the comet, when the Lander
runs out of power and changes into a so called Wake-up mode,
to provide a thermal environment in the Internal compartment
as required to switch-on the Lander electronics.
Subsystem Definiton
=============================================
In addition to the already described platform units PSS, CDMS and TCS
and the On-Orbiter units ESS, MSS and ESS-TxRx, a set of subsystems
is installed on the Lander.
The Active Descent System ADS provides a 1-axis thruster system used
at touch-down to support the landing and prevent a rebounding until
the harpoons are shot.
An Anchoring system, built by two redundant harpoons, is used to fix
the Lander to the comet's surface after landing and provide the
required counter-force during drilling.
A Flywheel providing a 1-axis momentum wheel used to stabilize the
Lander's descent to the comet.
The Landing gear provides the necessary interface between the Lander
and the comet and supports Lander science operations by a rotation
and tiliting capability.
The structure subsystem provides the required structural elements to
built up the Lander.
A TxRx system is installed to provide access to the Lander and enable
data retrievel during its mission phase on the comet.
Lander Reference Frame
=============================================
The Lander reference frame is defined as follows:
+Z-axis is perdendicular to the baseplate, generally pointing away
from the comet towards space, during cruise parallel to the Orbiter
+Z-axis, +X-axis is generally parallel to the comet surface, pointing
opposite of the Lander's balcony, into the direction of Lander
separation from the Orbiter, during cruise into Orbiter -X direction,
+Y-axis completes the right-handed frame.
The frame origin is located on the upper surface of the balcony
(Z = 0), in the middle of the balcony (Y = 0), at the outer end
(X = 0).
Lander Operating Modes
=============================================
The Lander is operated in the following modes:
Hibernation Mode:
This mode is defined as: Lander attached to the Orbiter, Orbiter LCL
5A or 5B ON, Lander Hibernation heater ON (dissipation > 12W at 28V),
no power on the Lander Primary Bus
In this mode the Lander is non-operational but under thermal control
with a hibernation temperature inside the internal compartment above
minus 55 degC at the reference point.
Wake-up Mode:
This mode is applied on the comet, substituting the Hibernation Mode.
The PSS wake-up thermostats are closed, because the temperature
inside the internal compartment is below minus 53 degC. In this mode
the Lander is non-operational, the Lander operational electronics are
disconnected from the Primary Bus and the wake-up heaters are
connected to the Primary Bus. In this mode NO thermal control is
possible, since the wake-up heaters will only dissipate, if the
Primary Bus is powered, which requires Sun irradiation on the comet to
operate the solar arrays. Without dissipation the compartment
temperature will drop until the comet environmental temperature. When
the Lander is still attached to the Orbiter and powered from the
Orbiter-LCL 15A/B, an additional heater set will also dissipate.
Power Enough Mode:
This mode follows the Wake-up mode, the Lander Primary Bus is
powered, but the voltage is still below 18.5V, which correspond to a
non-sufficient power situation. The available power is not lost,
since special Power Enough loads are used to dissipate and heat the
internal compartment.
Stand-by Mode:
The Lander is operational, since the Lander basic operational
electronics (PCU, CDMS and one TCU) are connected to the Primary Bus
and powered.
In this mode thermal control will be performed from the dissipation
of the activated units. If the temperature of the internal
compartment drops below the TCU set-points, the respcetive TCU
heaters will also dissipate.
Operational Modes:
These modes define Lander operation of Experiments.
APXS:
No activity during SDL and FSS.
CIVA:
CIVA-P mode Orbiter imaging : Imaging of the Orbiter after delivery
with camera 1 & 6.
CIVA-P mode Agilkia Landing site : Imaging of the Landing site Agilkia
just after touch-down Panorama with all 7 camera but only half of image
received.
CIVA-P mode Abydos location : Imaging of the Abydos after touch-down
and move on the comet Panorama with all 7 cameras.
CONSERT:
CONSERT Tuning mode: Instrument Switch ON and tuning of CONSERT
Lander & Orbiter clocks.
CONSERT Sounding during descent (SDL) mode: CONSERT Lander emission and
reception by CONSERT Orbiter. Active during the whole descent and stop during
the touch down window (CONSERT remaining active during this window but not
sounding (RF emission) for no interference with other instruments at time of
Landing. Lander and Orbiter in visibility during all this period as CONSERT
main objective was to monitor the Lander descent trajectory.
CONSERT Sounding after Landing mode: CONSERT Lander emission and reception by
CONSERT Orbiter. Lander and Orbiter in occultation permitting the sounding of
the comet structure.
COSAC:
COSAC Taping station test and sniff mode at Agilkia: Evaluation of the COSAC
taping station position and disengage of the possible taping station of an SD2
Carousel Oven (previous to any SD2 Carousel movement).
COSAC Abydos sniff mode: Analysis of the molecules present at the external
entry of the COSAS Mass Spectrometer done in Agilkia just after landing and
later on Abydos site.
MUPUS:
MUPUS Anchor mode:
Measurement of the acceleration sensors ANC-M inside the harpoons during
anchoring. Measurements of the temperature sensors ANC-T inside the harpoons.
MUPUS MAPPER mode:
Calibration of the Thermal Mapper during descent.
Two sub-mode to MAPPER mode
TM blackbody sub-mode:
Calibration of the Thermal Mapper with blackbody in the TM field of view
(during descent).
Infinite TEM sub-mode:
Calibration of the Thermal Mapper with deep space in TM FOV (during descent)
MUPUS TEM mode:
Passive Thermal Measurement Mode.
MUPUS LONGTERM (-> MAPPER) mode:
Thermal Mapper longterm measurement after landing and during one comet
rotation.
MUPUS PENEL deployment mode:
Penetrator deployment.
MUPUS HAMMER mode:
Penetrator insertion to ground by hammering.
PTOLEMY:
PTOLEMY Sniff and CASE mode: Analyse of the molecules present at the external
entry of PTOLEMY Mass Spectrometer.
PTOLEMY Agilkia sniff mode and tapping station test: Analyse of the molecules
present at the external entry of PTOLEMY Mass Spectrometer done in Agilkia
just after landing. Evaluation of the PTOLEMY taping station position and
disengage of the possible taping station of an SD2 Carousel Oven (previous to
any SD2 Carousel movement).
PTOLEMY Abydos sniff mode: Analyse of the molecules present at the
external entry of PTOLEMY Mass Spectrometer done in Abydos site.
PTOLEMY Oven mass spectrum analysis:
Analyse of the molecules present in the Oven by PTOLEMY Mass
Spectrometer done in Abydos site.
ROLIS:
ROLIS DIT mode: ROLIS imaging during descent Agilkia touch down
location in the field of view.
ROLIS DIS mode: ROLIS imaging during descent once landed.
ROLIS CUC mode: ROLIS imaging once on COMET in Abydos site during night period
with illumination by LED sources (blue, green dark, red, IR) Images of Abydos
site.
ROMAP:
ROMAP Slow Mode: Magnetometer in Slow mode
(1Hz sampling 512 octet / mn).
ROMAP Fast Mode: Magnetometer in Fast mode (916 octet / mn).
ROMAP Surface Mode SPM: Magnetometer and channeltron after Touch
Down from Noon to Day/Night transition.
SD2:
SD2 Drill downward and upward for COSAC: Carousel movements to zero
position Drill roto-translations downward and Sampling at 560 mm,
translation upward to 0mm, sample in Oven#17(SD2 count, HTO) delivered
to COSAC.
SD2 Carousel movements: Carousel movement for PTOLEMY with rotation to
0 arcmin.
SESAME:
SESAME CASSE mode: Measurements executed to register the vibration
environment generated by the Philae flywheel, intra-foot Soundings and
inter-foot Soundings, touchdown impact, the cometary vibration background and
any particles possibly dropping on the sole covers.
SESAME PP Passive Mode : Measurements conducted in order to determine
the electromagnetic environment close to the orbiter.
SESAME PP Active Mode : PP calibrations, determine the permittivity
of the comet surface material, monitor variations in the local
plasma environment.
SESAME DIM mode: DIM conducted to measure the particle environment.
"
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