Rosetta SPICE Repository
Rosetta SPICE kernels set
ESA, in collaboration with NAIF and the Rosetta Instrument Teams, produce a whole set of SPICE kernels for Rosetta (event kernels are not produced for ESA missions).
Browse our repository for information about naming conventions and time coverage for each of
The Rosetta SPICE dataset consists of several SPICE kernels, organised as follows:
- CK kernels: These kernels contain information about orientation of the space vehicle or any articulating
structure on it.
- FK kernels: Reference frame specifications. Definitions of, and specifications of, relationships between
reference frames (coordinate systems). Among the frames kernels included, there are kernels that specify reference frames
related to the earth and the spacecraft.
- IK kernels: Kernels that hold intrument information, such as field of view or internal timing.
- LSK kernel: These kernels hold a table with the leapseconds used to convert between ET and UTC.
- PCK kernels: These kernels provide information about Solar System bodies orientation and shape, and possibly
parameters for gravitational, atmospheric or rings models.
- SCLK kernel: This kernel (spacecraft clock coefficients) allows for conversion between ET and spacecraft
clock. If there are multiple LSK kernels in this dataset, the latest kernel supersedes he previous ones. More
information on the SCLK kernel(s) in this dataset is provided in SCLKINFO.TXT.
- SPK kernels: Kernels with information about ephemeris (position and velocity) of the spacecraft and solar
system bodies. The dataset provides such information for the planets, the Sun, the Moon, the New Norcia tracking station,
several DSN tracking stations, and the spacecraft. More information on the SPK kernels in this dataset is provided in
Origin of the kernels
Generic kernels provided by NAIF
NAIF generates kernels that are mission independent. Some of them are used by ESA missions:
- Binary and text PCK and LSK kernels.
- Some SPK kernels with ephemeris of the solar system bodies.
- SPK kernels for ground stations.
- Frames kernels for ground stations.
Other kernels provided by NAIF
NAIF collaborates with the ESA SPICE Team and the Intrument Teams to create instrument and frames kernels for
the different ESA Missions:
- The instrument kernels (IK) have been developed NAIF, the intrument teams and RSSD/ESA.
- The Rosetta frames kernel has been created by NAIF, in collaboration with RSSD/ESA.
Kernels generated with ESOC Ancillary Data
Orbit, clock and attitude kernels are created from ESOC data:
- ESOC ancillary data are the main source of information required to create SPICE kernels
for attitude (CK), orbit (SPK) and time (SCLK) information for the Spacecraft.
- Also, ESOC ephemeris data are used in the creation of SPK kernels for martian satellites.
See below for a more detailed explanation on how these kernels are generated.
Kernels created by the Rosetta SGS (Science Ground Segment), alone or in collaboration with the intruments teams
- CK kernels with orientation of the Rosetta Solar Arrays.
- CK kernels with orientation of the Rosetta High Gain Antenna.
- RSSD frames kernel.
- PCK kernels for Steins and Lutetia.
Creation of SPK, CK and SCLK kernels from ESOC Ancillary Data
In terms of orbital data, the mission can be divided in three different phases: cruise phase, nominal
phase and extended phase. The ftp repository provides the most up to date orbit kernels for Rosetta.
Several different types of data products are provided by ESOC: ORHR, ORHO, ORHS, ORER, ORMR, ORFR, ORGR and ORWR.
Attitude data for the spacecraft are provided for all mission phases except for safe modes, for the past and
the near future. The attitude is provided in several records, called segments, each covering a specific time
span. These segments have no overlap, but there may be gaps between the segments, and even gaps in the segments.
The available attitude data is usually predicted, although kernels with reconstructed data are present (for
time intervals for which the predicted attitude is known to be not accurate enough).
Time Correlation Data.
Time Correlation is one of the most critical pieces of information needed for the use of the SPICE system
within the Rosetta mission. This information allows the conversion between the Rosetta S/C Clock
time and UTC time. ESOC delivers time correlation data which are the source for the SCLK kernel.
ESOC always provide predicted and reconstituted orbit data, but only predicted attitude data. Only SPK kernels
with reconstructed data are archived.
An automated system, called ADCS (Automatic Data Conversion System) is responsible for the generation of CK,
SPK and SCLK kernels from the ESOC flight dynamics data. ADCS detects when a new product was generated or a new
time correlation packet is available, and run a series of processes in order to create the corresponding kernels.
ADCS uses the SPICE toolkit in order to fulfill its task. It runs in a server physically located at ESAC.