2001 Mars Odyssey

***2001 Mars Odyssey*** is a robotic spacecraft orbiting the planet Mars. The project was developed by NASA, and contracted out to Lockheed Martin, with an expected cost for the entire mission of US$297 million. Its mission is to use spectrometers and a thermal imager to detect evidence of past or present water and ice, as well as study the planet's geology and radiation environment. It is hoped that the data *Odyssey* obtains will help answer the question of whether life existed on Mars and create a risk-assessment of the radiation that future astronauts on Mars might experience. It also acts as a relay for communications between the Mars Science Laboratory, and previously the Mars Exploration Rovers and *Phoenix* lander, to Earth. The mission was named as a tribute to Arthur C. Clarke, evoking the name of *2001: A Space Odyssey*.

*Odyssey* was launched April 7, 2001, on a Delta II rocket from Cape Canaveral Air Force Station, and reached Mars orbit on October 24, 2001, at 02:30 UTC (October 23, 19:30 PDT, 22:30 EDT).

By December 15, 2010, it broke the record for longest serving spacecraft at Mars, with 3,340 days of operation. As of 2019 October it is in a polar orbit around Mars with a semi-major axis of about 3,800 km or 2,400 miles. It has enough propellant to function until 2025.

## Overview[edit]

On May 28, 2002 (sol 210), NASA reported that *Odyssey*'s GRS instrument had detected large amounts of hydrogen, a sign that there must be ice lying within a meter of the planet's surface, and proceeded to map the distribution of water below the shallow surface. The orbiter also discovered vast deposits of bulk water ice near the surface of equatorial regions.

*Odyssey* has also served as the primary means of communications for NASA's Mars surface explorers in the past decade, up to the *Curiosity* rover. By December 15, 2010, it broke the record for longest serving spacecraft at Mars, with 3,340 days of operation, claiming the title from NASA's *Mars Global Surveyor*. It currently holds the record for the longest-surviving continually active spacecraft in orbit around a planet other than Earth, ahead of the Pioneer Venus Orbiter (served 14 years) and the Mars Express (serving over 14 years), at 18 years, 6 months and 3 days.

## Naming[edit]

In August 2000, NASA solicited candidate names for the mission. Out of 200 names submitted, the committee chose Astrobiological Reconnaissance and Elemental Surveyor, abbreviated ARES (a tribute to Ares, the Greek god of war). Faced with criticism that this name was not very compelling, and too aggressive, the naming committee reconvened. The candidate name "2001 Mars Odyssey" had earlier been rejected because of copyright and trademark concerns. However, NASA e-mailed Arthur C. Clarke in Sri Lanka, who responded that he would be delighted to have the mission named after his books, and he had no objections. On September 20, NASA associate administrator Ed Weiler wrote to the associate administrator for public affairs recommending a name change from ARES to *2001 Mars Odyssey*. Peggy Wilhide then approved the name change.

## Scientific instruments[edit]

The three primary instruments *Odyssey* uses are the:

* **Thermal Emission Imaging System** (THEMIS).
* **Gamma Ray Spectrometer** (GRS), includes the **High Energy Neutron Detector** (HEND), provided by Russia. **GRS** is a collaboration between University of Arizona's Lunar and Planetary Lab., the Los Alamos National Laboratory, and Russia's Space Research Institute.
* **Mars Radiation Environment Experiment** (MARIE).

## Mission[edit]

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Summary of *Mars Odyssey* mission start

Animation of 2001 Mars Odyssey's trajectory around Sun
 2001 Mars Odyssey **·**   Earth **·**   Mars

Animation of 2001 Mars Odyssey's trajectory around Mars from 24 October 2001 to 24 October 2002
  2001 Mars Odyssey **·**   Mars

*Mars Odyssey* as imaged by *Mars Global Surveyor*

*Mars Odyssey* launched from Cape Canaveral on April 7, 2001, and arrived at Mars about 200 days later on October 24. The spacecraft's main engine fired in order to decelerate, which allowed it to be captured into orbit around Mars. *Odyssey* then spent about three months aerobraking, using friction from the upper reaches of the Martian atmosphere to gradually slow down and reduce and circularize its orbit. By using the atmosphere of Mars to slow the spacecraft in its orbit rather than firing its engine or thrusters, *Odyssey* was able to save more than 200 kilograms (440 lb) of propellant. This reduction in spacecraft weight allowed the mission to be launched on a Delta II 7925 launch vehicle, rather than a larger, more expensive launcher.

Aerobraking ended in January 2002, and Odyssey began its science mapping mission on February 19, 2002. *Odyssey*'s original, nominal mission lasted until August 2004, but repeated mission extensions have kept the mission active.

About 85% of images and other data from NASA's twin Mars Exploration Rovers, *Spirit* and *Opportunity*, have reached Earth via communications relay by *Odyssey*. The orbiter helped analyze potential landing sites for the rovers and performed the same task for NASA's Phoenix mission, which landed on Mars in May 2008. *Odyssey* aided NASA's *Mars Reconnaissance Orbiter*, which reached Mars in March 2006, by monitoring atmospheric conditions during months when the newly arrived orbiter used aerobraking to alter its orbit into the desired shape.

*Odyssey* is in a Sun-synchronous orbit, which provides consistent lighting for its photographs. On September 30, 2008 (sol 2465) the spacecraft altered its orbit to gain better sensitivity for its infrared mapping of Martian minerals. The new orbit eliminated the use of the gamma ray detector, due to the potential for overheating the instrument at the new orbit.
MARIE hardware, designed to measure radiation
The payload's MARIE radiation experiment stopped taking measurements after a large solar event bombarded the *Odyssey* spacecraft on October 28, 2003. Engineers believe the most likely cause is that a computer chip was damaged by a solar particle smashing into the MARIE computer board.

The orbiter's orientation is controlled by a set of three reaction wheels and a spare. When one failed in June 2012, the fourth was spun up and successfully brought into service. Since July 2012, *Odyssey* has been back in full, nominal operation mode following three weeks of 'safe' mode on remote maintenance.

On February 11, 2014, mission control accelerated *Odyssey*'s drift toward a morning-daylight orbit to "enable observation of changing ground temperatures after sunrise and after sunset in thousands of places on Mars". The orbital change occurred gradually until November 2015. Those observations could yield insight about the composition of the ground and about temperature-driven processes, such as warm seasonal flows observed on some slopes, and geysers fed by spring thawing of carbon dioxide (CO2) ice near Mars' poles.

On October 19, 2014, NASA reported that the *Mars Odyssey* Orbiter, as well as the *Mars Reconnaissance Orbiter* and *MAVEN*, were healthy after the Comet Siding Spring flyby.

In 2010, a spokesman for NASA's Jet Propulsion Laboratory stated that *Odyssey* could continue operating until at least 2016. This estimate has since been extended until 2025.

### Water on Mars[edit]

Main article: Water on Mars

By 2008, *Mars Odyssey* had mapped the basic distribution of water below the shallow surface. The ground truth for its measurements came on July 31, 2008, when NASA announced that the Phoenix lander confirmed the presence of water on Mars, as predicted in 2002 based on data from the *Odyssey* orbiter. The science team is trying to determine whether the water ice ever thaws enough to be available for microscopic life, and if carbon-containing chemicals and other raw materials for life are present.

The orbiter also discovered vast deposits of bulk water ice near the surface of equatorial regions. Evidence for equatorial hydration is both morphological and compositional and is seen at both the Medusae Fossae formation and the Tharsis Montes.

### *Odyssey* and *Curiosity*[edit]

*Mars Odyssey*'s THEMIS instrument was used to help select a landing site for the Mars Science Laboratory (MSL). Several days before MSL's landing in August 2012, *Odyssey*'s orbit was altered to ensure that it would be able to capture signals from the rover during its first few minutes on the Martian surface. *Odyssey* also acts as a relay for UHF radio signals from the (MSL) rover *Curiosity*. Because *Odyssey* is in a Sun-synchronous orbit, it consistently passes over *Curiosity*'s location at the same two times every day, allowing for convenient scheduling of contact with Earth.