Galileo (spacecraft)
Consideration of sending a probe to Jupiter began as early as 1959. NASA's Scientific Advisory Group for Outer Solar System Missions evaluated the requirements for future missions. They noted that technology to build a heat shield did not yet exist at that time. Facilities to test such shields would not be available until 1980. NASA management designated the Jet Propulsion Laboratory as the lead center for the project. The mission was named Galileo after the Italian astronomer who first viewed Jupiter through a telescope in 1610. His discovery of four moons orbiting Jupiter provided evidence for the Copernican model of the solar system. The name was officially adopted in February 1978. John R. Casani became the first project manager and solicited suggestions for an inspirational name. The most votes went to Galileo, though it was also the name of a spacecraft in Star Trek television shows.
The launch date faced significant hurdles following the Space Shuttle Challenger disaster. The original May launch could not be met due to safety concerns. Anti-nuclear groups sought court injunctions prohibiting the launch because of plutonium in the radioisotope thermoelectric generators. These RTGs were necessary for deep space probes flying distances from the Sun where solar energy is impractical. The launch was delayed twice more by a faulty main engine controller and inclement weather. Atlantis finally lifted off at 16:53:40 UTC on the 18th of October 1989. It entered a 285-kilometer orbit before deploying Galileo at 00:15 UTC on October 19. The spacecraft separated from the Inertial Upper Stage booster at 01:06:53 UTC that same day. Atlantis returned to Earth safely on October 23 after completing its mission.
One section of the spacecraft rotated at 3 revolutions per minute to keep Galileo stable. This spinning section held six instruments including fields and particles detectors. Back on the ground, the mission operations team used software containing 650,000 lines of code for orbit sequence design. Another 1,615,000 lines handled telemetry interpretation while 550,000 lines managed navigation. All components received a minimum of 2,000 hours of testing before flight. The spacecraft was designed to last for at least five years. Six RCA 1802 COSMAC microprocessor CPUs controlled the system, each clocked at about 1.6 MHz. These chips were fabricated on sapphire material which is radiation-hardened. Each CPU operated as an 8-bit low-power CMOS processor similar to those in Apple II computers. Memory capacity provided by bulk memory units totaled 176K of RAM across the subsystems. The propulsion module included a main engine and twelve thrusters developed by Messerschmitt-Bölkow-Blohm from West Germany.
Galileo arrived at Jupiter on the 7th of December 1995 after gravitational assist flybys of Venus and Earth. The spacecraft departed JPL in Pasadena, California on the 19th of December 1985. It traveled toward Venus first using gravity assists to gain speed. This trajectory allowed the probe to reach Jupiter despite limited fuel reserves. The journey covered vast distances through the solar system over several years. Galileo became the first spacecraft to orbit an outer planet upon arrival. The mission path required precise calculations and multiple course corrections during transit. The spacecraft maintained its orientation relative to the Sun and Canopus star for navigation purposes. This approach enabled high-resolution imaging capabilities that would later define scientific discoveries.
The spacecraft had a large high-gain antenna which failed to deploy during the mission. Engineers used the low-gain antenna instead to maintain communication with Earth. This limitation reduced data transfer rates significantly compared to original design specifications. Despite the failure, teams developed engineering workarounds to recover critical information. Software updates were sent to reconfigure systems for optimal performance under constraints. The mission continued successfully despite this major hardware malfunction affecting transmission speeds. Teams managed to transmit valuable data back to ground stations throughout the extended mission duration. The recovery effort demonstrated remarkable adaptability in space operations when facing unexpected technical challenges.
Scientific instruments measured fields and particles mounted on the spinning section of the spacecraft. The camera system obtained images of Jupiter's satellites at resolutions 20 to 1,000 times better than Voyager best results. Galileo flew closer to the planet and its inner moons enabling detailed observations. The solid-state imager weighed specific amounts and consumed average power levels during operation. Instruments detected heavy ions with energies ranging from carbon to nickel elements. Magnetic field measurements covered ranges from ±32 to ±512 nanoteslas using outboard sensors. Plasma subsystems collected charged particles covering most angles from zero to 180 degrees. These findings revealed complex dynamics within Jupiter's magnetosphere and atmosphere. Data helped determine how particles gained energy and moved through the Jovian environment over time.
Lacking fuel to escape Jupiter's gravity well, the main spacecraft was deliberately crashed into Jupiter on the 21st of September 2003. This decision prevented forward contamination of possible life on Europa moon. The probe entered the atmosphere at high speed reaching temperatures around certain values. An ablative heat shield made of carbon phenolic protected scientific instruments during descent. The atmospheric probe included seven instruments measuring temperature pressure deceleration and gas composition. Batteries manufactured by Honeywell provided nominal power output throughout the entry phase. The mission concluded after completing all planned objectives for studying Jupiter and its moons. Next orbiter Juno arrived on the 5th of July 2016 continuing exploration efforts beyond Galileo's legacy.
Common questions
When was the Galileo spacecraft launched?
The Galileo spacecraft lifted off at 16:53:40 UTC on the 18th of October 1989. It entered a 285-kilometer orbit before deploying Galileo at 00:15 UTC on October 19.
Who named the Galileo mission after an Italian astronomer?
John R. Casani became the first project manager and solicited suggestions for an inspirational name. The most votes went to Galileo, though it was also the name of a spacecraft in Star Trek television shows.
What happened to the high-gain antenna on the Galileo spacecraft?
The large high-gain antenna failed to deploy during the mission. Engineers used the low-gain antenna instead to maintain communication with Earth.
Why did NASA crash the Galileo probe into Jupiter?
Lacking fuel to escape Jupiter's gravity well, the main spacecraft was deliberately crashed into Jupiter on the 21st of September 2003. This decision prevented forward contamination of possible life on Europa moon.
When did the Galileo spacecraft arrive at Jupiter?
Galileo arrived at Jupiter on the 7th of December 1995 after gravitational assist flybys of Venus and Earth. It departed JPL in Pasadena, California on the 19th of December 1985.
All sources
48 references cited across the entry
- 1press releaseThe Final Day on GalileoJet Propulsion Laboratory — 21 September 2003
- 2webGalileo Jupiter ArrivalNASAJet Propulsion Laboratory — December 1995
- 4newsGalileo ends in blaze of glory2003-09-21
- 5magazineWhat Galileo SawMichael Benson — September 1, 2003
- 6webGalileo In DepthNASA
- 7press releaseFour New Shuttle Crews Named (STS-32, STS-33, STS-34, STS-35)Jeffrey Carr — NASA — November 10, 1988
- 8newsGroups Protest Use of Plutonium on GalileoWilliam J. Broad — October 10, 1989
- 9journalRadiation Risk and Planetary Exploration - The RTG ControversyDavid Salisbury — May–June 1987
- 10webGalileo: To Launch or not to Launch?Carl Sagan — October 9, 1989
- 11newsGalileo Launch NearsKathy Sawyer — October 17, 1989
- 12webMission Archives: STS-34NASA — February 18, 2010
- 13webPDS: Mission InformationNASA
- 15webGalileo EngineeringRESA
- 16webWhat's in an RTG?NASA
- 17webSolid-State Imaging (SSI)NASA
- 18webSSI – Solid State ImagingNASA
- 19webSSI Imaging TeamNASA
- 21webNIMS TeamUCLA
- 23webEUV TeamUniversity of Colorado at Boulder
- 24webPPR – Photopolarimeter-RadiometerNASA
- 25webPPR TeamLowell Observatory
- 26webDDS – Dust Detector SubsystemNASA
- 27webCosmic Dust: Messengers from Distant WorldsHigh Energy Stereoscopic System
- 28webEPD – Energetic Particles DetectorNASA
- 29webGalileo EPDJohns Hopkins University Applied Physics Laboratory
- 30webHIC – Heavy Ion CounterNASA
- 31webHIC TeamCaltech
- 32webMAG – MagnetometerNASA
- 33webMAG TeamUCLA
- 34webPLS – Plasma SubsystemNASA
- 35webPLS TeamUniversity of Iowa
- 36webPWS – Plasma Wave SubsystemNASA
- 37webGalileo PWSUniversity of Iowa
- 39webGalileo Probe Science ResultsD. Isbell et al. — NASA / JPL — 22 January 1996
- 40webDevelopment of New Ablative Thermal Protection Systems (TPS)Bernard Laub — NASA / Ames — 19 October 2004
- 41webGalileo Jupiter Atmospheric ProbeNASA — December 2017
- 42webGalileo FAQ – Galileo AntennasNASA / JPL
- 43webJupiter: Facts – NASA ScienceNASA — October 5, 2017
- 44webNASA's 50 Year Men and WomenNASA
- 45press releaseGalileo Arrives at Kennedy Space CenterNASA / JPL — 17 May 1989
- 46webExperiments on Galileo ProbeNASA
- 47webSpace Launch 1989-084Knihovna Akademie věd ČR
- 48webGalileo Plunges Into JupiterFraser Cain — 22 September 2003