Data Set Information
|
DATA_SET_NAME |
ODY MARS SPICE KERNELS V1.0
|
DATA_SET_ID |
ODY-M-SPICE-6-V1.0
|
NSSDC_DATA_SET_ID |
|
DATA_SET_TERSE_DESCRIPTION |
Navigation and ancillary data in the form of SPICE System kernel
files for the Odyssey spacecraft.
|
DATA_SET_DESCRIPTION |
Data Set Overview
=================
This data set includes the complete set of SPICE data for the
Mars Odyssey in the form of SPICE kernels, which can be accessed
using SPICE software available to read these files.
The SPICE data contains geometric and other ancillary information
needed to recover the full value of science instrument data. In
particular SPICE kernels provide spacecraft and planetary
ephemerides, instrument mounting alignments, spacecraft
orientation and spacecraft sequences of events. Data needed for
relevant time conversions is also included.
Data Types (SPICE kernel types)
===============================
SPK kernels contain ephemerides for spacecraft, planets,
satellites, comets and asteroids as well as for moving or
fixed spacecraft and instrument structures. They provide
position and velocity, given in a Cartesian reference frame.
SPK files are located under the ``data/spk'' directory of
this data set.
PCK kernels contain certain physical, dynamical and
cartographic constants for target bodies, such as size and shape
specifications, and orientation of the spin axis and prime
meridian. PCK files are located under the ``data/pck'' directory
of this data set.
IK kernels (Instrument description kernels) give descriptive and
operational data peculiar to a particular scientific instrument,
such as internal timing relative to the spacecraft clock and
field-of-view model parameters. IK files are located under the
``data/ik'' directory of this data set.
CK kernels describe pointing, containing a transformation
traditionally called the C-matrix which is used to determine
time-tagged pointing (orientation) angles for a spacecraft
structure upon which science instruments are mounted. CK files
are located under the ``data/ck'' directory of this data set.
EK (Events) kernels are derived from the integrated sequence of
events used to produce actual spacecraft commands. EK files are
located under the ``data/ek'' directory of this data set.
LSK (Leapseconds) kernels contain the leapseconds and the values
of other constants required to perform a transformation between
Universal Time Coordinated (UTC) and Ephemeris time (ET). LSK
files are located under the ``data/lsk'' directory of this data
set.
SCLK (Spacecraft Clock) kernels contain on-board clock calibration
data required to perform a mapping between Ephemeris time (ET)
and spacecraft on-board time (SCLK.) SCLK files are located under
the ``data/sclk'' directory of this data set.
FK (Frame Definitions) kernels contain information required to
define reference frames, sources of frame orientation data and
inter-connections between these frames and other frames supported
within the SPICE system. This includes mounting alignment
information for each instrument. FK files are located under
the ``data/fk'' directory of this data set.
Kernel File Details
===================
A brief overview of the different types of M01 kernels included
in this data set is provided in the CONFIDENCE_LEVEL_NOTE section
of this file while details specific to individual files are found
in the ``*info.txt'' files in the corresponding data directory.
The most detailed description of the data in each file is
provided in metadata included inside the file -- in the
description area of text kernels or in the comment area of binary
kernels.
Software
========
The SPICE Toolkit contains software modules needed to read
SPICE kernel files. SPICELIB software is highly documented
via internal headers. Additional documentation is available
in separate ASCII text files called Required Reading files.
For example, the S- and P- Kernel (SPK) Required Reading File,
named SPK.REQ, describes use of the SPK kernel file readers
and contains sample programs.
The latest SPICE Toolkit for a variety of computer platforms such
as PC, Mac, SUN, HP, SGI, VAX, DEC Alpha, etc. is available at
the NAIF Node of PDS electronically (via anonymous FTP and WWW
servers). Refer to information in ``software/softinfo.txt'' for
additional details. Each version of the Toolkit is also archived
at the NASA National Space Science Data Center.
Loading Kernel Files into a SPICE-based Application
===================================================
The easiest way to make data from a collection of SPICE kernels
available to a SPICE-based application is to list these kernels
in a meta-kernel and load it into the program using the high
level SPICE data loader routine FURNSH. This data set provides
such meta-kernel(s) under the ``extras/mk'' directory. For more
information about the MGS meta-kernel(s), see the file
``extras/mk/mkinfo.txt''.
|
DATA_SET_RELEASE_DATE |
2002-09-30T00:00:00.000Z
|
START_TIME |
2001-04-07T12:00:00.000Z
|
STOP_TIME |
2024-01-01T12:00:00.000Z
|
MISSION_NAME |
2001 MARS ODYSSEY
|
MISSION_START_DATE |
2001-01-04T12:00:00.000Z
|
MISSION_STOP_DATE |
N/A (ongoing)
|
TARGET_NAME |
MARS
|
TARGET_TYPE |
PLANET
|
INSTRUMENT_HOST_ID |
ODY
|
INSTRUMENT_NAME |
SPICE KERNELS
|
INSTRUMENT_ID |
SPICE
|
INSTRUMENT_TYPE |
N/A
|
NODE_NAME |
Navigation and Ancillary Information Facility
|
ARCHIVE_STATUS |
LOCALLY ARCHIVED
|
CONFIDENCE_LEVEL_NOTE |
This volume contains SPICE kernel files created during mission
operations and after mission data reconstruction and analysis.
Some general information about this collection follows here,
but the prospective user is also referred to extensive
descriptions about each file that are stored inside each kernel
file. These metadata provide detailed information regarding
the information source from which the data were derived, the
type of processing applied to the source data, applicability
of the data, etc. Metadata are located in the ``comment area''
for binary kernel types (SPK, CK, ESQ), accessible using either
the COMMNT or SPACIT utility program found in the NAIF Toolkit.
Metadata are located after ``\begintext'' markers within the
text kernel types (PCK, IK, FK, LSK, SCLK, MK), accessible by
using any available text file display tool such as a word
processor, text editor, or the unix ``more'' or ``cat''
commands.
In some cases data accuracy information does not exist, or
may be estimated after mission completion.
Where there are questions about data accuracy or ``confidence''
not addressed herein the reader is invited to examine subsequent
SPICE archive releases associated with this data set (if such
exist), or to contact the NAIF node of the Planetary Data System
for possible further information.
SPK Files
=========
Three kinds of SPK files are provided in this archive: SPK
files for the spacecraft orbit, SPK files for Phobos, Deimos,
Mars, Earth and Sun, and SPK files for the solar array and
high gain antenna structures.
Spacecraft Orbit SPK Files
--------------------------
Most of the included SPK files provide the orbit of the ODY
spacecraft. These files came from three different producers --
Mars Odyssey Navigation Team (NAV) and Alex Konopliv and Eugene
Fahnestock of the Solar System Dynamics group of JPL. The NAV SPK
files provide the reconstructed trajectory solution generated for
use by various project teams during mission operations. The
Konopliv's and Fahnestock's solutions were done at a later time
using more recent and complex models and, in general, is more
accurate. Refer to the detailed comments provided in the comment
area of these files for more information about accuracy of the
trajectory stored in the these files, models used in process,
etc.
This data set also includes the orbit number files generated
during the mission using the NAIF's ORBNUM utility program for
each of the NAV spacecraft trajectory SPK files for the orbital
phases of the mission. These files are not SPICE kernels; for
this reason they are provided in the ``extras/orbnum'' directory.
For more information about Mars Odyssey orbit number files, see
the file ``extras/orbnum/orbinfo.txt''.
Solar System Body SPK Files
---------------------------
The MAR033 Martian satellite ephemeris SPK files provided in this
data set were used by the project up to the fall of 2006. They
contain ephemeris data for Phobos, Deimos, Earth and the sun.
Formal one-sigma accuracy information for Phobos and Deimos are
reported as follows:
Body Downtrack Crosstrack Radial
Uncertainty Uncertainty Uncertainty
------ ----------- ----------- -----------
Phobos 15 km 7 km 3 km
Deimos 30 km 16 km 3 km
The MAR063 Martian satellite ephemeris SPK files provided in this
data set superseded the MAR033 files and were used by the project
starting in the fall of 2006. As the MAR033 files the MAR063 SPKs
contain ephemeris data for Phobos, Deimos, Earth and the sun.
Formal one-sigma accuracy information for Phobos and Deimos are
reported as follows:
Body Downtrack Crosstrack Radial
Uncertainty Uncertainty Uncertainty
------ ----------- ----------- -----------
Phobos 5 km 2 km 2 km
Deimos 10 km 3 km 3 km
Accuracies for Mars-Sun and Mars-Earth directions (positions
obtained from SPK files) are at the level of 0.001 arc-sec (1
sigma).
Spacecraft Solar Array and HGA Structures SPK File
--------------------------------------------------------------
Included in the SPK archive is a file containing location
information (fixed offsets) for spacecraft structures--the
high gain antenna and solar array. See the metadata in this
file--found in the comment area--for detailed descriptions
of how the file was produced.
For more information about Mars Odyssey SPK files, see the file
``data/spk/spkinfo.txt''.
CK Files
========
C-kernel files provide orientation of a structure:
the spacecraft bus, the solar array, or the high gain
antenna. There is only one reconstructed CK file provided
for each structure for a given mission phase or a portion of
a mission phase. All three kinds of reconstructed CK files
are produced from engineering telemetry downlinked from the
spacecraft. As is often the case with spacecraft engineering
telemetry-based measurements, considerable uncertainty exists
as to the accuracy of such measurements, and, data quality
(accuracy and completeness) can vary significantly.
For the spacecraft bus, in addition to the reconstructed CKs,
this data set also includes predicted nominal nadir-pointed
orientation CK files and CK files providing nominal orientation
during ROTO periods. The ``nadir'' CKs contain orientation
computed assuming that the spacecraft was pointing nadir at all
times or was pointing off nadir by a constant yaw or roll angle
(for HGA mitigation periods in 2005 and 2009). The ``ROTO'' CKs
contain orientation computed assuming that the spacecraft was
pointing according to the commanded off-nadir roll angle; they
cover only the periods when the spacecraft was at ROTO
orientations. Both types of the nominal orientation CKs should be
used only when the reconstructed CKs don't provide coverage and
the spacecraft is known to be in the pointing mode matching the
mode represented by the nominal CK files. For such periods the
nominal orientation usually matches the actual orientation to
about or better than 0.2 degrees.
Reconstructed Solar Array CK Files
--------------------
CK files providing orientation of the solar array relative
to the spacecraft bus are provided to support any spacecraft
dynamics and/or instrument view obstruction analysis that
would require knowledge of the solar orientation and position.
Reconstructed High Gain Antenna CK Files
--------------------------
CK files providing orientation of the high gain antenna (HGA)
relative to the spacecraft bus are provided to support the
radio science analysis, spacecraft dynamics analysis, and
instrument view obstruction analysis.
Reconstructed Spacecraft Bus CK Files
-----------------------
CK files providing the orientation of the spacecraft bus (``the
spacecraft'') are provided to support interpretation of data
obtained by all science experiments. At the time of this archive
release there are no known reports assessing accuracy of the
orientation provided in these files.
Caution on Using CK Files
-------------------------
While not a data accuracy issue, the CK user is nevertheless
cautioned to understand and properly use the data found and
tolerance arguments that are inputs to the CK reader provided
in the SPICE Toolkit. Descriptions about how to read CK files
are found in the CK reader routine headers (top of the source
code files) and in the ``CK Required Reading'' document; these
are contained in each SPICE Toolkit package.
For more information about Mars Odyssey CK files, see the file
``data/ck/ckinfo.txt''.
PCK Files
=========
PCK files provide size, shape and orientation data for ``target''
bodies such as Mars, Phobos and Deimos. A description of these
data items and reference to their source is provided inside
the PCK file, which is a simple text file that can be viewed
using any word processor, text editor or text display utility.
The data for the PCK provided in this archive are official
IAU/IAG/COSPAR values accepted in 2000.
For more information about Mars Odyssey PCK files, see the file
``data/pck/pckinfo.txt''.
FK Files
========
Frames kernel files provide specifications for how one reference
frame is defined relative to another frame. The ODY FK provided
in this data set contains a complete set of frame definitions for
the spacecraft, its structures such as solar array and antennas,
and all of its science instruments. Meta information provided in
the comments included in this file consists of the frame
definitions, description of the frame relationships, source of
and accuracy of the mounting alignment information, etc.
For more information about Mars Odyssey FK files, see the file
``data/fk/fkinfo.txt''.
IK Files
========
Instrument kernel files provide specifications for the optical
and physical instrument parameters and -- where applicable --
field-of-view size, shape and orientation for the named
instrument. Metadata describing these estimates are provided in
each IK file included in this archive.
For more information about Mars Odyssey IK files, see the file
``data/ik/ikinfo.txt''.
SCLK Files
==========
Spacecraft Clock kernel files provide a tabulation of data
needed for converting time measurements between ephemeris time
(ET) and spacecraft clock time (SCLK). A SPICE SCLK file is
made from a similar file--SCLK/SCET file, or SCLKvSCET
file--produced by another mission entity. Each newly made SCLK
file fully replaces the previous SCLK file.
For ODY the time correlation accuracy provided in SCLK/SCET
files is informally reported by the Lockheed Martin spacecraft
team to be better than 100 milliseconds during cruise and
better than 10 milliseconds during orbital phases. (NAIF has
not attempted to obtain or produce an independent corroboration
of these LMA estimates.) The SPICE SCLK file has essentially
the same accuracy as the SCLK/SCET file.
SPICE software does not prohibit an SCLK file from being used
for time conversions occurring for ``future times'' (or more
accurately, for epochs that occur later than the epoch of the
last telemetry data used in producing the last correlation
coefficients found in the SCLK file). Such ``predict'' time
conversions are likely to be inaccurate (changed somewhat)
once the epoch of interest has been passed.
For more information about Mars Odyssey SCLK files, see the file
``data/sclk/sclkinfo.txt''.
LSK Files
=========
Leapseconds kernel files provide a tabulation of ``leapseconds''
and some other terms used in converting time measurements
between ephemeris time (ET) and Universal Time (UTC). ``Spacecraft
Event Time'' (SCET) is the commonly used name for UTC events
measured at the spacecraft.
Metadata describing how the LSK data are obtained or computed
is contained inside the LSK text file. The time conversion
provided by SPICE LSK files is accurate to approximately
0.000030 seconds.
For more information about Mars Odyssey LSK files, see the file
``data/lsk/lskinfo.txt''.
EK Files
========
Two kinds of Events kernel (EK) files are included in this
archive: Experimenter's Notebook EKs and Sequence EKs. Each of
these kinds is briefly described below.
Experimenter's Notebook EKs kernels are a digital analog to the
traditional paper laboratory notebook. Hence Experimenter's
Notebook entries represent truth only as seen by the author of
the notes--there is no attempt made to independently validate any
aspect of Experimenter's Notebook information.
Sequence EKs comprise a summary of all commands sent to the
spacecraft as well as some ground system events and instrument
state (status) summaries. All Sequence EK entries are time
tagged. In this archive includes Sequence EKs created the
automated process for providing ``as run'' inputs reflecting what
was actually sent to the spacecraft, and what execution times
were used.
For more information about Mars Odyssey EK files, see the file
``data/ek/ekinfo.txt''.
|
CITATION_DESCRIPTION |
Semenov, B.V., L.S. Elson, C.H. Acton, M. Costa Sitja, and A.M. Bailey,
ODYSSEY SPICE KERNELS V1.0, ODY-M-SPICE-6-V1.0,
NASA Planetary Data System, 2004. https://doi.org/10.17189/1520115
|
ABSTRACT_TEXT |
This data set includes the complete set of Odyssey SPICE data
files (``kernel files''), which can be accessed using SPICE
software. The SPICE data contains geometric and other ancillary
information needed to recover the full value of science
instrument data. In particular SPICE kernels provide spacecraft
and planetary ephemerides, instrument mounting alignments,
spacecraft orientation, spacecraft sequences of events, and data
needed for relevant time conversions.
|
PRODUCER_FULL_NAME |
ALYSSA M. BAILEY
|
SEARCH/ACCESS DATA |
NAIF Online Archives
NAIF Data Set Subsetter
NAIF WebGeocalc
|
|