Raw Radio Science Data from Galileo

Review facilitated by the Ring-Moon Systems Node of NASA PDS: Mia Mace, Matt Tiscareno
May, 2025

The data providers are Dustin R. Buccino, Elias Barbinis, and Daniel S. Kahan.

Background

This bundle is a data restoration. The original PDS3 archives were submitted by the Galileo Radio Science Support Team (RSST) at the Jet Propulsion Laboratory (JPL) to the Planetary Data System (PDS). These archives were rejected due to issues with the data; however, there was no funding remaining to resolve these items so the data were never formally archived. This PDS4 migration and archival, performed by the Radio Science Sub Node (RSSN) of the PDS, contains all known RSS data at the time of archival (May 2025).

Of particular interest are files from the NASA Deep Space Network including closed-loop tracking data and open-loop tracking data. The formats of these files changed throughout the Galileo era, resulting in multiple data formats.

Media calibration data are provided on a best-efforts basis though media calibration data are not complete for this archive. Only ionosphere calibrations are provided; and those have gaps between 1999-10-01 to 2003-01-01.

Galileo mission

The Galileo mission launched on October 18, 1989 on the space shuttle Atlantis. The interplanetary cruise lasted about 6 years and the spacecraft followed a Venus-Earth-Earth gravity assist (VEEGA) trajectory to Jupiter. Several targets of opportunity along the way allowed for cruise science. The spacecraft arrived at Jupiter on December 7, 1995, and released a proble into Jupiter before executing the Jupiter Orbit Insertion maneuver. The Prime Mission orbital operations consisted of 10 targeted satellite encounters over 24 months. Orbital periods varied from as long as 200 days to as little as 35-40 days between encounters. The Galileo Europa Mission (GEM) was a low-cost follow-on to the Galileo Prime Mission that uses the Galileo spacecraft to continue focused studies of the Jovian system. The mission is divided into three main phases or campaigns: Europa Campaign, Perijove Campaign and Io Campaign. The Galileo Millennium Mission (GMM) was a follow on to the GEM mission, with a greatly reduced budget. The mission was designed to continue the exploration of Io and the inner Jovian magnetosphere, and to dispose of the spacecraft with a Jupiter impact on September 21, 2003.

Galileo RSS System

The Galileo Radio Science Subsystem (RSS) was a powerful radio science instrument designed to explore Jupiter. It contained capabilities for both S-band and X-band radio links to Earth and an onboard Ultra Stable Oscillator (USO). It was integrated with the telecommunications subsystem (see Section 2.6.2 of the archive Software Interface Specification (SIS) in the document collection).

Unfortunately, the High Gain Antenna (HGA) failed to deploy and severely limited the capabilities of the investigation. The USO was used throughout the mission as an onboard stable frequency reference, but the radio link to Earth was limited to be used on the Low Gain Antenna (LGA) and at S-band uplink/downlink only.

Science Objectives

Radio Science investigations were carried out by two teams. The Celestial Mechanics Team, under Team Leader John Anderson, conducted experimental tests of general relativity (including searching for gravitational waves), made measurements to improve solar system ephemerides, and sought to improve gravitational models for Jupiter and its satellites. The Radio Propagation Team, under Team Leader Tay Howard, investigated the solar corona and carried out various studies in the Jovian system primarily concerning atmospheres and ionospheres.

Two different types of radio science measurements were conducted with the Galileo Orbiter: radio tracking in which the magnitude and direction of gravitational forces could be derived from 'closed-loop' Doppler (and, sometimes, ranging) measurements, and radio propagation experiments in which modulation on the signal received at Earth stations could be attributed to properties of the intervening medium. The radio science measurements were analyzed by two investigation teams; the Celestial Mechanics Team was primarily interested in characterizing variations in gravitational forces, and the Radio Propagation Team was primarily interested in the atmospheres of the Sun, Jupiter, and Jupiter's satellites.

Note: This information is provided in the bundle's archive SIS, refer to that document for further details.

Data Bundle

The complete peer review bundle (gll.rss.raw.tar.gz) is online here. Also provided are the checksum manifest and validation report; these latter two files are primarily for reviewers concerned with PDS4-compliance (see instructions below).

Reviewers should begin by reading the Software Interface Specification (SIS), which is included in the document collection and provides detailed descriptions of the archive bundle.

The directory structure of the PDS4 bundle is illustrated below:

Instructions for Reviewers

Here are guidelines and some information to help you produce an effective review with a reasonable level of effort.

All reviewers must address two general areas: Furthermore, if you are one of the panel members with a direct affiliation with the PDS, please also address a third general area: If you are not one of the panel members with a direct affiliation with the PDS, then you do not need to address compliance with PDS4 standards. Rather, you should focus on the data (including ancillary data) and documentation.

While it is not realistic for you to analyze every data file, please check enough to convince yourself of the quality and consistency of the data and of any errors that you encounter.

Please also evaluate the documentation provided in individual table labels, and referenced journal articles. Much of the information contained in the referenced articles is not duplicated in the data sets.

Questions for reviewers to address are:

The review panel submits written reviews by email and then, if the RMS Node thinks it is necessary, participates in a teleconference (date TBD) to discuss the reviews, including strengths and weaknesses of the data set. Specific shortcomings and errors will be identified as "liens" – questions about or requests for change – which will need to be corrected. The review panel is responsible for making a recommendation on whether:

In addition to an overall recommendation, the RMS Node will compile a list of liens in the archive design or sample products/bundle. The liens must be resolved before the associated data set can be archived.

Known Issues

Known issues will be resolved during lien resolution, along with any other issues raised by the reviewers and deemed reasonable/necessary.

Reviewers' Submitted Comments and Responses

Review Outcome


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