Galileo - Glossary of Selected Terms

AACS
Attitude and Articulation Control Subsystem. Navigates the spacecraft, establishes and maintains its attitude (pointing in space; It tends to be quite good-natured, otherwise), controls movements of booms, the scan platform, the despun section, etc. The AACS has two "strings" for redundancy. Elements of these strings can be swapped for additional robustness.

More information on the AACS.

Alfven wing
Electromagnetic waves that are generated when plasma flow s past an electrically conducting body such as Jupiter's moon Io.

aurora
A glow from a planet's atmosphere produced by the impact and interation of charged particles in a planet's magnetosphere with the atmospheric atoms and molecules.

CDS
Command and Data Subsystem. The "Master Computer" of the spacecraft. The CDS provides the interface between the ground and the spacecraft. All commands are either directed to the CDS, passed by the CDS to other subsystems (eg AACS), or control relays directly. The CDS also collects data from all the subsystems and science instruments and formats them for transmission to the ground.

The CDS has two strings also. In addition, complete copies of the flight software are in the normal and extended (spare) memory on each string, to enable rapid switching in case of a memory failure on one string.

More information on the CDS.

Fields and Particles instruments
Complement of instruments designed to provide data on the structure and dynamical variations of the Jovian magnetosphere. This complement is made up of the Dust Detector, Energetic Particles Detector, Heavy Ion Counter, Magnetometer, Plasma and Plasma Wave Subsystems.

HGA
High-Gain Antenna. Galileo's original design called for a deployable antenna to unfurl, providing approximately 34dB of gain at X-band (10GHz) for a 134kbps downlink of science and priority engineering data. When it did not unfurl following the Earth fly-by in 1992, the spacecraft was reconfigured to utilize the S-band (2.8GHz) omnidirectional antenna for downlink at much lower data rates, from 8-16 bps through Jupiter Orbit Insertion. This 8dB gain low-gain antenna (LGA) was originally supposed to "trickle" down low-rate engineering data, and to be utilized in case a fault resulted in the spacecraft "safing" and shifting to a Sun-pointed attitude, resulting in loss of signal from the HGA. Enhancements to the Deep Space Network and reprogramming the flight computers on Galileo will increase the telemetry bit rate to 8-160 bps which will be used starting in the spring of 1996.

New Telecommunications Strategy

magnetosphere
The volume of space in which a planet's magnetic field dominates that of the solar wind.

magnetotail
The portion of a planetary magnetosphere pulled downstream by the solar wind.

mini-tour
Continuous survey of Fields and Particles data through at least one complete orbit.

occultation
Period of time when the view to one celestial body is blocked by the body of another, e.g. when the spacecraft's view of the Earth or Sun is blocked by Jupiter.

OPNAV
SSI image taken for optical naviation; image typically consists of the limb and terminator of one main body (Jupiter or a satellite) and stars. The image is used to determine the position of the imaged body against a star background which enables the navigators to better estimate the relative position of the spacecraft and the imaged body.

palimpsest
A roughly circular spot on icy satellites, thought to identify a former impact crater.

phase angle
The angle between the Sun, an object, and an observer. 0 degrees phase means the Sun is behind the observer.

plasma
A highly ionized gas, consisting of almost equal numbers of free electrons and positive ions.

plasma sheet
Low energy plasma, largely concentrated within a few planetary radii of the equatorial plane, distributed throughout the magnetosphere throughout which concentrated electric currents flow.

satellites, Galilean
Io, Europa, Ganymede, and Callisto; four largest satellites of Jupiter discovered by Galileo in 1610.

satellite wake
Region created in front of the Galilean satellites as the charged particles that corotate with the Jovian magnetosphere sweep past the satellites.

solar conjunction
Period of time during which the Sun is in or near the spacecraft-Earth communications path, thus corrupting the communications signals.

thruster flush
The term "thruster flush" may sound mysterious, but it's really a simple form of preventive maintenance. Galileo's thrusters operate by the controlled burning of fuel (MonoMethyl Hydrazine) and oxidizer (Nitrogen Tetroxide). The oxidizer is especially reactive. Even though the thruster valves are made from special steels, the liquid still dissolves minute amounts of iron. The erosion is too small to harm the valves, but the dissolved iron compounds eventually condense and cling to the fine mesh filters used to keep debris from the valve seats. Unchecked, these deposits may clog the filters and hold back oxidizer to the thrusters, a process known as "flow decay". Periodic short burns of all the thrusters (about one second) clears out propellant resting in the valves, flushing the iron solution before it settles. A flush every three weeks protects the thrusters from flow decay.

torus, Io
Donut-shaped cloud of neutral and ionized gases (plasma) along Io's orbit believed to be supplied by the volcanic eruptions on Io.

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