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10,000 Orbit Odyssey
10,000 Orbit Odyssey
21 May 2004
(Source: Jet Propulsion Laboratory)

http://marsprogram.jpl.nasa.gov/spotlight/odyssey-10000-orbits.html

The Odyssey of Odyssey's 10,000 Orbits
Jet Propulsion Laboratory
May 21, 2004

Like a sweet, older sibling standing quietly to the side as the baby of the family gets all the "ooh's" and "aah's," the 2001 Mars Odyssey orbiter has blended into the background noise of cheers for the Mars Exploration Rover discoveries. But Odyssey deserves her own praise and applause this Saturday as she reaches a major milestone. At 5:29 p.m. PDT on May 22, 2004, Odyssey is scheduled to complete her 10,000th science mapping orbit around the red planet.

"You know, we often take big numbers for granted in the business of exploring space: light years of distance, terabytes of data, millions of pounds of thrust," said Gaylon McSmith, Mars Odyssey Science Office Manager. "Believe me, to the scientists of this project, 10,000 orbits and everything it took to achieve this milestone is truly a BIG number. Odyssey's science return has been outstanding and 10,000 orbits has provided an absolute treasure trove of information that will benefit researchers for many years to come."

Big Orbit Numbers = Big Science

Odyssey was designed to make three major contributions to the understanding of Mars:

  • map chemical elements and minerals on the surface of Mars to find out what "Mars is made of" >/li>
  • look for water in the shallow subsurface
  • analyze the radiation environment to determine its potential effects on human health.

A Long Road to Success

Odyssey was launched from Cape Canaveral in Florida on April 7, 2001, and began its science mapping mission on February 19, 2002.

"It has been a long road getting to this point," explained Bob Mase, Mars Odyssey Mission Manager and former Navigation Lead. "We followed two spacecraft losses: the 1998 Mars Climate Orbiter and the Mars Polar Lander. After those failures, the pressure was on. We had to plan and re-plan."

The original Mars 2001 concept consisted of two spacecraft: an orbiter launching from Vandenburg Air Force Base in California and a precision lander carrying a Spirit- and Opportunity-sized rover. But, following the Mars Climate Orbiter and Mars Polar Lander failures, the entire Mars Program as well as the Mars 2001 project were restructured to incorporate lessons learned. The project was re-planned several times and eventually ended up with just a single orbiter spacecraft. The spacecraft design was still changing in the final 12 months prior to launch. "It was an accomplishment just to get Odyssey to its new launch pad on the opposite side of the country in Florida!" said Mase.

Relief on meeting that deadline was short-lived.While the six-month, 286-million-mile (460-million-kilometer) cruise from Earth to Mars was largely uneventful, getting the spacecraft into orbit around Mars (Mars orbit insertion) was arduous from a personal perspective. One month prior to Mars orbit insertion, the 9/11 national tragedy shocked the nation and the team. The flight team at Jet Propulsion Laboratory in Pasadena, Calif., and their dedicated partners who operate the spacecraft from Lockheed Martin in Denver, Colo., put their heads down and forged ahead to achieve their goal of continuing America's legacy of peaceful exploration. Overcoming personal losses and concerns stemming from the 9/11 experience, the Odyssey team steadfastly prepared for arrival at Mars and the grueling aerobraking process, which would drag the spacecraft through the martian atmosphere to slow the spacecraft and bring Odyssey into its desired mapping orbit.

"Every one of our 332 dives into the volatile martian atmosphere carried the potential to burn us up," Mase explained. "Looking back on it, the current success makes it easy to forget the pressure we were under.The eyes of the world were upon us as a symbol of the American spirit, and the future of the Mars Program was on our shoulders as we were the first mission to return to Mars following two failures. The notion that 'you cannot fail' still echoes in my mind," said Mase.

Fail they did not, and are still making enormous contributions to current and future missions.

"The Mars Exploration Rover project wants to congratulate Odyssey on doing a tremendous job on both accomplishing their own science investigations and at the same time enabling Spirit and Opportunity to make significant scientific discoveries from the surface of Mars," said Richard Cook, Mars Exploration Rover former project manager. "Almost all of our data - over 75% -- is coming down through the Odyssey relay, which is a testament to both the flexibility of the people on the project and to the capability of the design of the spacecraft."

"Odyssey's science return has been outstanding, and the entire team is eager to repeat this feat of 10,000 orbits numerous times in the years to come," said McSmith.

ODYSSEY SCIENCE INSTRUMENT HIGHLIGHTS

The Thermal Emission Imaging System (THEMIS) consists of two cameras: one that images visible wavelengths in full color and an infrared camera that is capable of detecting thermal and mineral variations. To date, THEMIS has mapped 99.7% of the planet in the infrared wavelengths and 15% in visible wavelengths. THEMIS images have been used to identify possible recent snowpacks on martian hillsides, to find exposed water ice near the south pole, to provide the first complete high resolution map of the south polar layered deposits, to map the remarkable region of Meridiani where the Opportunitiy rover drives, and to detect ancient unweathered volcanic rocks and map unusual mineral deposits.

The Gamma Ray Spectrometer (GRS) is a suite of three instruments: a gamma subsystem located on the end of a six-meter boom and two neutron subsystems, a neutron spectrometer and a high energy neutron detector. This collection of instruments collects gamma rays and neutrons emitted from the planet to determine the elemental composition of the upper meter of the martian surface. The GRS has obtained full planet maps of the abundances of several elements including silicon, iron, chlorine, potassium, and thorium. GRS maps show very high contents of water ice buried just beneath the surface over large areas in the polar regions. GRS has also measured the thickness of the annual carbon dioxide frost as the martian seasons change.

The Martian Radiation Environment Experiment (MARIE) is a radiation monitor similar to those flown on the space shuttle and the International Space Station. MARIE has measured the background radiation levels in orbit at Mars, and shown them to be 2 to 3 times that around the Earth. It has also served as an outpost for monitoring solar particle events.

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Last Updated: 25 May 2004