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Mars Global Surveyor

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The Mars Global Surveyor (MGS) is a US spacecraft developed by NASA and the Jet Propulsion Laboratory and launched November 1996. It began the United States's return to Mars after a 20-year absence. It completed its primary mission in January 2001 and is now in an extended mission phase through at least September 2008.

On November 2, 2006, the spacecraft was thought to have gone into safe mode after experiencing a problem with its solar panels. Attempts to recontact it and resolve the problem have failed and the current state of the spacecraft is unknown. The newly arrived Mars Reconnaissance Orbiter spacecraft has attempted to take a picture of Mars Global Surveyor in order to check the craft's orientation towards the Sun and Earth to help diagnose the problem.<ref>Orbiter may be last chance to rescue Mars probe (November 13, 2006).</ref> However, preliminary analysis has shown no indication of the Mars Global Surveyor. Mars Exploration Program manager Fuk Li has said, "Realistically, we have run through the most likely possibilities for re-establishing communication, and we are facing the likelihood that the amazing flow of scientific observations from Mars Global Surveyor is over."<ref name="may end">NASA's Mars Global Surveyor May Be at Mission's End. NASA/Jet Propulsion Laboratory news release. Retrieved on November 21, 2006.</ref>

Contents

[edit] Specifications

The Surveyor spacecraft, fabricated at the Lockheed Martin Astronautics plant in Denver, is a rectangular-shaped box with wing-like projections (solar panels, used to convert sunlight into electricity) extending from opposite sides. When fully loaded with propellant at the time of launch, the spacecraft weighed 1,060 kilograms (2,342 pounds). Most of Surveyor's mass lies in the box-shaped module occupying the center portion of the spacecraft. In reality, this center module is made of two smaller rectangular modules stacked on top of each other, one of which is called the equipment module and holds the spacecraft's electronics, science instruments, and the 1750A mission computer. The other module, called the propulsion module, houses Surveyor's rocket engines and propellant tanks.

[edit] Scientific instruments

Five scientific instruments fly onboard Mars Global Surveyor:

[edit] Launch and orbit insertion

The Surveyor spacecraft was launched from the Cape Canaveral Air Station in Florida on November 7, 1996 aboard a Delta-7925 rocket. The spacecraft travelled nearly 750 million kilometers (466 million miles) over the course of a 300-day cruise to reach Mars on September 11, 1997.

Upon reaching Mars, Surveyor fired its main rocket engine for the 22-minute Mars orbit insertion (MOI) burn. This maneuver slowed the spacecraft and allowed the planet's gravity to capture it into orbit. Initially, Surveyor entered a highly elliptical orbit that took 45 hours to complete. The orbit had a periapsis of 262 km above the northern hemisphere, and an apoapsis of 54,026 km above the southern hemisphere.

[edit] Aerobraking

After orbit insertion, Surveyor performed a series of orbit changes to lower the periapsis of its orbit into the upper fringes of the Martian atmosphere at an altitude of about 110 kilometers (68 miles). During every atmospheric pass, the spacecraft slowed down by a slight amount because of atmospheric resistance. The density of the Martian atmosphere at such altitudes is comparatively low, allowing this procedure to be performed without damage to the spacecraft. This slowing caused the spacecraft to lose altitude on its next pass through the orbit's apoapsis. Surveyor used this aerobraking technique over a period of four months to lower the high point of its orbit from 54,000 kilometers to altitudes near 450 kilometers.

On October 11, the flight team performed a maneuver to raise the periapsis out of the atmosphere. This suspension of aerobraking was performed because air pressure from the atmosphere caused one of Surveyor's two solar panels to bend backward by a slight amount. The panel in question was slightly damaged shortly after launch in November 1996. Aerobraking was resumed on November 7 after flight team members concluded that aerobraking was safe, provided that it occurs at a more gentle pace than proposed by the original mission plan.

This image taken by Mars Global Surveyor spans a region about 1500 meters across, showing gullies on the walls of Newton Basin in Sirenum Terra.  Similar channels on Earth are formed by flowing water, but on Mars the temperature is normally too cold and the atmosphere too thin to sustain liquid water. Nevertheless, many scientists hypothesize that liquid groundwater can sometimes surface on Mars, erode gullies and channels, and pool at the bottom before freezing and evaporating.

Under the new mission plan, aerobraking occurred with the low point of the orbit at an average altitude of 120 km, as opposed to the original altitude of 110 km. This slightly higher altitude resulted in a decrease of 66 percent in terms of air resistance pressure experienced by the spacecraft. During these six months, aerobraking reduced the orbit period to between 12 and 6 hours.

From May to November 1998, aerobraking was temporarily suspended to allow the orbit to drift into the proper position with respect to the Sun. Without this hiatus, Surveyor would complete aerobraking with its orbit in the wrong solar orientation. In order to maximize the efficiency of the mission, these six months were devoted to collecting as much science data as possible. Data was collected between two to four times per day, at the low point of each orbit.

Finally, from November 1998 to March 1999, aerobraking continued and shrank the high point of the orbit down to 450 km. At this altitude, Surveyor circled Mars once every two hours. Aerobraking was scheduled to terminate at the same time the orbit drifted into its proper position with respect to the Sun. In the desired orientation for mapping operations, the spacecraft always crossed the day-side equator at 14:00 (local Mars time) moving from south to north. This geometry was selected to enhance the total quality of the science return.

[edit] Mapping

The spacecraft circles Mars once every 117.65 minutes at an average altitude of 378 kilometers (235 miles). It is in a near polar orbit (inclination = 93°) which is almost perfectly circular, moving from being over the south pole to being over the north pole in just under an hour. The altitude is chosen to make the orbit sun-synchronous, so that all images taken by the spacecraft of the same surface features on different dates are taken under identical lighting conditions. After each orbit, the spacecraft views the planet 28.62° to the west because Mars has rotated underneath it. In effect, it is always 14:00. for Mars Global Surveyor as it moves from one time zone to the next exactly as fast as the Sun. After seven sols and 88 orbits, the spacecraft approximately retraces its previous path, with an offset of 59 km to the east. This ensures eventual full coverage of the entire surface.

And now, in its extended mission, MGS is doing much more than studying the planet directly beneath it. It commonly performs rolls and pitches to acquire images off of its nadir track. The roll maneuvers, called ROTOs (Roll Only Targeting Opportunities), roll the spacecraft left or right of its ground track to shoot images as much as 30° from nadir. A Pitch maneuver can be added to compensate for the relative motion between the spacecraft and the planet. This is called a CPROTO (Compensation Pitch Roll Targeting Opportunity), and allows for some very high resolution imaging by the on board MOC (Mars Orbiting Camera).

In addition to this, MGS can shoot pictures of other orbiting bodies, such as other spacecraft and the moons of Mars.

MOC images

[edit] MER Communications Subsystem

Mars Global Surveyor now also functions as a communications satellite to relay data back to Earth from the MER surface landers. Portions of MGS are scheduled to remain active until at least September 2008 to support MER.<ref>NASA Mars Spacecraft Gear Up for Extra Work (September 25, 2006).</ref>

[edit] Loss of Contact

On November 2, 2006, NASA lost contact with the spacecraft after commanding it to adjust its solar panels.

Several days later a faint signal was received indicating that the spacecraft had entered safe mode, and was awaiting further instructions from Earth.

On November 20, NASA attempted to image MGS with the recently arrived Mars Reconnaissance Orbiter. The attempt was unsuccessful, leaving NASA with very few options for recovering MGS. This pushed NASA engineers to declare MGS operations "likely" complete.<ref name="may end"/>

On November 21-22 MGS failed to relay communications to the Opportunity rover on the surface of Mars, adding to the belief that the spacecraft is lost.

[edit] Mission timeline

[edit] Other pictures

[edit] See also

[edit] References

[edit] Notes

<references/>

[edit] External links

cs:Mars Global Surveyor de:Mars Global Surveyor es:Mars Global Surveyor fa:نقشه‌بردار سراسر مریخ fr:Mars Global Surveyor it:Mars Global Surveyor lv:Mars Global Surveyor hu:Mars Global Surveyor nl:Mars Global Surveyor ja:マーズ・グローバル・サーベイヤー pl:Mars Global Surveyor pt:Mars Global Surveyor ru:Марс Глобал Сервейор sk:Mars Global Surveyor sv:Mars Global Surveyor

 

v  d  e</span> 

Mars Spacecraft Missions
Flybys: Mariner 4 | Mariner 6 | Mariner 7 | Mars 4
Orbiters: Mariner 9 | Mars 2 | Mars 3 | Mars 5 | Mars 6 | Viking 1 | Viking 2 | Phobos 2 | Mars Global Surveyor | Mars Odyssey | Mars Express Orbiter | Mars Reconnaissance Orbiter
Landers and Rovers: Mars 3 | Viking 1 | Viking 2 | Mars Pathfinder | Spirit rover | Opportunity rover
Future: Phoenix Scout (2007) | Mars Science Laboratory (2009) | Phobos-Grunt (2009) | Mars 2011 | ExoMars (2013) | Astrobiology Field Laboratory (2016?)
See also: Mars | Exploration of Mars | Colonization of Mars
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