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Mission lead
NASA
Launch Date
12 August 2005
Destination
Mars
Current status
Extended mission

At a Glance

Why do we need the Mars Reconnaissance Orbiter?

Among rocky planets, is Earth unique? In some ways, yes: Earth hosts a complex ecosystem with intelligent life. But how common are the geologic forces that shaped our planet, and how did they create the conditions hospitable for life? Are they common or rare among similar types of planets, both in our solar system and in planetary systems beyond? Studying Mars—a nearby, rocky, similarly-sized planet—helps us answer these questions.

Of particular interest is water: how much of it there was, how it sculpted the surface of the planet, and where it still exists today. Water is a key requirement for the evolution of life as we know it. Understanding the history of water on Mars informs the understanding of life on Mars—if it ever existed.

NASA's Mars Reconnaissance Orbiter (MRO) is an orbiting spacecraft that studies the geologic history of Mars and its present climate. It allows scientists to compare the forces that shaped Mars to those that shaped the Earth—including water— and provides unique insights into the planet's formation and evolution. It also provides an ongoing record of Mars' climate and weather patterns. These insights help scientists understand how this Earth-like planet changed from a habitable world to a wasteland, and whether Earth could suffer the same fate.

MRO is part of NASA's Mars Exploration Program, an unprecedented, multi-decade campaign to comprehensively understand Mars and its suitability to host past or present life. All spacecraft launched in this effort play a complementary scientific role to each other. But MRO plays a special role in supporting these other missions.

The spacecraft's powerful camera helps engineers select safe landing sites for future robotic and human missions to Mars, free of obstacles like uneven terrain or large rocks and boulders. It also provides high-resolution maps to help Earth-bound rover operators plan driving routes. It has even captured jaw-dropping pictures of spacecraft in the process of landing on Mars.

Phoenix spotted by HiRISE against Heimdall crater as it descends

NASA / JPL / U. Arizona

Phoenix spotted by HiRISE against Heimdall crater as it descends
This amazing image was captured as Phoenix came in for its Mars landing on May 25, 2008.  The HiRISE camera on Mars Reconnaissance Orbiter pointed at Phoenix, which is seen here against the background of a 10-kilometer-diameter crater called Heimdall.

Additionally, MRO is the cornerstone of NASA's satellite communications network at Mars. The robotic spacecraft and rovers that land on the martian surface are limited to small, low-powered antennas that beam data back to Earth at a relative trickle. At that rate, those missions could never send all of their science data back to Earth. MRO solves this problem by relaying this data back to Earth at high speeds on behalf of the surface missions, using its powerful 3-meter antenna. The success of NASA's surface exploration of the Red Planet is dependent upon this relay capability provided by MRO and a few other orbiting spacecraft.

How the Mars Reconnaissance Orbiter Studies the Geology and Climate of Mars

The Mars Reconnaissance Orbiter launched in August of 2005 and reached Mars 7 months later in March of 2006. Using its suite of exquisitely sensitive scientific instruments, it has been observing Mars ever since—far outlasting its original 5-year design lifetime.

The Mars Reconnaissance Orbiter hosts 6 science instruments:

The High Resolution Imaging Science Experiment (HiRISE) Camera

NASA / JPL / Ball Aerospace

The High Resolution Imaging Science Experiment (HiRISE) Camera
HiRISE is the most powerful camera yet sent to Mars and is the marquee instrument on the Mars Reconnaissance Orbiter. In this photograph, a worker at Ball Aerospace and Technology Corp., Boulder, Colo., prepares the instrument before it is attached to the spacecraft.

MRO carries the most powerful camera ever sent to Mars. It can reveal details as small as 1 meter (3 feet) across and create precise 3D maps of the surface. Combined with a complementary camera that provides a wider context of the surface, MRO examines the surface at great detail to identify geologic processes that shaped it, from the subtle to the catastrophic.

Martian Avalanche!

NASA /JPL / University of Arizona

Martian Avalanche!
Caught in the act by the Mars Reconnaissance Orbiter: an avalanche cascades down a steep, icy scarp near the north pole of Mars, kicking up a cloud of reddish dust about 200 meters wide.

Through these efforts, MRO has found that Mars experienced many geologic processes similar to the ones that shaped Earth in its past, including volcanic lava flows, wind erosion forming massive buttes, the depositing of sedimentary layers within lake beds, and meandering rivers cutting through bedrock. These data suggest that similar-sized rocky planets share a similar set of forces that shape their surfaces.

MRO's other instruments look at Mars through specific ranges of the electromagnetic spectrum—basically, ranges of colors, many of which are beyond what the human eye can see. Different physical processes, atmospheric gasses, and surface compounds have distinctive "fingerprints" when viewed in these color ranges. By looking at Mars through these color ranges, MRO's instruments help confirm the presence (or absence) of these processes and materials, providing important clues into the history of Mars and how it formed.

Diverse exposed surface mineralogy around the Jezero delta

NASA / JPL / JHUAPL / MSSS / Brown University

Diverse exposed surface mineralogy around the Jezero delta
A preserved river delta in Jezero crater, Mars as imaged by the Mars Reconnaissance Orbiter. The colors denote the presence of different types of materials formed or altered by water.

In addition to studying the surface, MRO uses its specialized instruments to track the annual changes in Mars' climate as the planet revolves around the sun. Its cameras make frequent global weather maps, a specialized instrument studies the composition and structure of Mars' atmosphere, and it uses radar to seek out buried deposits of water. MRO has provided more than 15 years of climate and weather data, leading to improved models that assist in the safe landing of future robotic and human missions.

MRO added additional, overwhelming evidence that water once flowed on Mars. Its cameras found surface features sculpted by flowing water. It detected abundant minerals formed or chemically altered by water scattered over the planet's surface. And its ground-penetrating radar discovered large amounts of buried ice, including an ice reservoir the size of Lake Superior.

What you can do to support the Mars Reconnaissance Orbiter

The Mars Reconnaissance Orbiter met its prime mission objectives and is now operating well beyond its original design lifetime of 5 years. NASA intends to operate it until its fuel is exhausted, probably in the mid-2020s. Because it plays such a critical role relaying communications for landers and rovers—including NASA's Perseverance mission—MRO is a high-priority mission for NASA, though not because of its own scientific output.

Mars is a big place, and even though MRO has been there for many years, there is still much more science left to do. Appropriate funding for the missions' scientific work will ensure that humanity gets the best possible return out of this unique mission.

Here are 2 specific actions you can take to support MRO:

Three ways you can be a space advocate

More ways to follow the Mars Reconnaissance Orbiter:

This page was written by Planetary Society staff writers. It is regularly updated.

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