Data Set Information
|
DATA_SET_NAME |
MRO MARS SPICE KERNELS V1.0
|
DATA_SET_ID |
MRO-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 Mars Reconnaissance Orbiter.
|
DATA_SET_DESCRIPTION |
Data Set Overview
=================
This data set includes the complete set of Mars Reconnaissance
Orbiter 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, and data needed for relevant
time conversions.
This data set is contained on a single virtual volume,
MROSP_1000, including data from all mission phases and covering
from launch, 2005-08-12T12:40:00, through the end time of the
latest spacecraft trajectory file supplied in the data set. Until
the end of the spacecraft lifespan this data set is accumulating
with new data added approximately every three to six months.
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
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 MRO 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. SPICE 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, etc. is available at the NAIF Node of PDS
electronically (via anonymous FTP and WWW servers). Refer to
information in ``software/softinfo.txt'' for details regarding
obtaining this software. 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 MRO meta-kernel(s), see the file
``extras/mk/mkinfo.txt''.
|
DATA_SET_RELEASE_DATE |
2007-06-08T00:00:00.000Z
|
START_TIME |
2005-08-12T12:40:00.000Z
|
STOP_TIME |
2024-04-01T12:00:00.000Z
|
MISSION_NAME |
MARS RECONNAISSANCE ORBITER
|
MISSION_START_DATE |
2005-08-12T12:00:00.000Z
|
MISSION_STOP_DATE |
N/A (ongoing)
|
TARGET_NAME |
MARS
|
TARGET_TYPE |
PLANET
|
INSTRUMENT_HOST_ID |
MRO
|
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 data set 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.
Where there are questions about data accuracy or ``confidence''
not addressed herein the reader is invited 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 the Solar System planets
and Martian system satellites, and SPK files for the relative
locations of selected spacecraft structures. Each of these kinds
is briefly described below; more information is available in the
file ``data/spk/spkinfo.txt''.
Two sets of the MRO spacecraft orbit SPK files are included in
this data set.
The first set of the spacecraft orbit SPK files contains the
reconstructed spacecraft trajectory determined by the MRO
Navigation (NAV) Team, JPL. Each of these SPK files covering the
whole or a part of a particular mission phase was made by merging
together numerous shorter duration individual files officially
delivered by the NAV team to the project. The component files
used to make a merged product can be discerned by reading the
descriptive information (metadata) found in the comment area of
each file. The accuracy of the spacecraft trajectory provided by
these files for the orbital phases of the mission was informally
reported by the NAV team to be better than than a few meters.
The second set of the spacecraft orbit SPK files contains the
reconstructed spacecraft trajectory determined by the Solar
System Dynamics (SSD) Group, JPL. These SPK files are available
only for the post-aerobraking phases of the mission (PSP, Relay).
They were generated in the process of the MRO gravity experiment
data reduction using the 95th degree and order MRO95A gravity
solution, which included entire MGS mission tracking data set and
Mars Odyssey and MRO tracking data up to the orbit solution date.
The data arcs for the orbits in these files are slightly longer
than 4 days in length. They were extended so that Doppler data
was contained at the beginning and end of the orbit solutions.
The orbit overlap errors using a 2-hr overlap were on average 0.5
meters for along the velocity vector and normal to the orbit
plane, and 5 cm for the radial component. The normal error
increased to about 50 meters during the edge-on geometry phase at
the end of June 2007.
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 the MRO orbit number files, see the
file ``extras/orbnum/orbinfo.txt''.
The DE410 planetary ephemeris SPK file included in this data set
contains ephemeris data for the Solar System planet barycenters,
Sun, Mercury, Venus, Earth, Moon, and Mars. This version of
ephemerides was officially used by the project during mission
operations. The internal comments included this SPK file provide
detailed accuracy information.
The MAR063 Martian satellite ephemeris SPK file provided in this
data set contains 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
The MRO structures SPK file included in this archive provides
relative locations of the High Gain Antenna (HGA) and Solar Array
(SA) components. The data included in the file are based of the
dimensions from the spacecraft engineering drawings.
CK Files
========
Five kinds of C-kernel files are provided in this archive: the
spacecraft bus (SC) orientation CKs (reconstructed and
predicted), the solar arrays (SA) orientation CKs (reconstructed
and predicted), the high gain antenna (HGA) orientation CKs
(reconstructed and predicted), the CRISM instrument orientation
CKs (reconstructed only), and the MCS instrument orientation CKs
(reconstructed only).
The SC, SA, and HGA reconstructed CK files were produced from
engineering telemetry downlinked from the spacecraft while the
SC, SA, and HGA predicted CK files were produced from spacecraft
orientation and articulation data modeled by the AtArPS program
ran by the MRO Spacecraft Team, LMA. While the coverage provided
by the reconstructed CK is fairly complete, they have occasional
small gaps. The predicted CKs included in this data set are
intended to be used to fill these gaps with nominal orientation
by loading these predicted files simultaneously with (but with
lower priority than) the reconstructed files. All of these CKs
contain data tagged with encoded SCLKs computed using the clock
with ID -74.
The CRISM CK files providing orientation for the CRISM instrument
were produced by the CRISM team using the gimbal angle data from
the instrument housekeeping telemetry. These files were used by
the CRISM team to process CRISM science data. The CRISM CKs
contain data tagged with encoded SCLKs computed using the clock
with ID -74999.
The MCS CK files providing orientation for the MCS instrument
were produced by the MCS team using the gimbal angle data from
the instrument housekeeping telemetry. These files were used by
the MCS team to process MCS science data. These CKs contain data
tagged with encoded SCLKs computed using the clock with ID -74.
Currently no formal accuracy estimates are available for any of
these CKs.
More information about MRO CK files is available in 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 only PCK file included in this data set is based on the
IAU/IAG/COSPAR values accepted in 2000. This PCK has been used by
the MRO project during operations.
More information about the PCK files included in this data set is
available in 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 MRO FK provided
in this data set contains the 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.
More information about the MRO FK files is available in the file
``data/fk/fkinfo.txt''.
IK Files
========
Instrument kernel files provide specifications for geometric
parameters and--where applicable--field-of-view size, shape and
orientation for the named instruments. Metadata describing these
estimates are provided in each IK file included in this archive.
Parameter values were determined from pre-launch measurements,
instrument parameters specification documents, and in some cases
from analysis of in-flight calibration data. The accuracy
estimates for these data vary from instrument to instrument and,
where available, are included in the IK internal comments.
This data set includes IK files for six MRO instruments -- CRISM,
CTX, HIRISE, MCS, MARCI, and ONC. Because the sets of geometric
parameters included in the IKs vary from instrument to instrument
users are encouraged to carefully examine the IKs before using
them.
The IK for SHARAD will be added to the data set in a later
release.
More information about MRO IK files is available in 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). The MRO SPICE SCLK files were made
from similar files--SCLK/SCET files, or SCLKvSCET file--produced
by another mission entity. Each newly made SCLK file fully
replaces the previous SCLK file.
For MRO the time correlation accuracy provided in SCLK/SCET files
is informally reported by the Lockheed Martin spacecraft team to
be better than 10 milliseconds. (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.
Each of the MRO SCLK files incorporates two time correlation data
sets -- one for the MRO on-board clock tags presented in the
``standard'' format and the other for the tags in the ``high
precision'' format.
``Standard'' MRO on-board clock tags are derived from 5-byte tags
present in majority of the spacecraft and instrument telemetry
and utilizing only the last of five bytes for fractional seconds.
This results in one SCLK tick being equal to 1/256 of a second.
The ID of this clock is -74, the same as of the MRO spacecraft.
``High precision'' MRO on-board clock tags are derived from
6-byte tags present in some of the spacecraft and instrument
telemetry and utilizing the last two of six bytes for fractional
seconds. This results in one SCLK tick being equal to 1/65536 of
a seconds. The ID of this clock is -74999.
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.
More information about the MRO SCLK files is available in 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.
More information about the LSK files is available in the file
``data/lsk/lskinfo.txt''.
EK Files
========
The MRO project did not produce any EK files; therefore, no EKs
are included in this data set.
|
CITATION_DESCRIPTION |
Semenov, B.V., C.H. Acton, M. Costa Sitja, and A.M. Bailey,
MARS RECONNAISSANCE ORBITER SPICE KERNELS V1.0,
MRO-M-SPICE-6-V1.0, NASA Planetary Data System, 2007.
https://doi.org/10.17189/1520100
|
ABSTRACT_TEXT |
This data set includes the complete set of Mars Reconnaissance
Orbiter 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, 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
|
|