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Messenger: New Views of Mercury

Messenger is the first orbital mission around Mercury. More properly known as the MErcury Surface, Space ENvironment, GEochemistry, and Ranging mission, the more than 1,000-pound spacecraft is checking out the sun's closest planetary neighbor and beaming back pictures as well as information about how craters and the mysterious landscape were formed – and even, how the planet itself might have come together.

A view of the horizon of Mercury, taken by NASA's Messenger spacecraft on March 29, 2011. The picture shows a stretch of land about 750 miles long, from top to bottom.
A view of the horizon of Mercury, taken by NASA's Messenger spacecraft on March 29, 2011. The picture shows a stretch of land about 750 miles long, from top to bottom.
Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

Messenger left Earth on Aug. 3, 2004, to take a complex path toward Mercury. Using a technique dating back to the Pioneer and Voyager missions, Messenger would use the gravity of several worlds to slingshot it from place to place.

This would give the spacecraft enough of a boost to arrive at Mercury and use the least fuel possible. This is important as fuel is heavy to carry, increasing launch costs.

Dress rehearsal

The spacecraft swung by Earth on Aug. 2, 2005, to pick up speed, then aimed for Venus and did two flybys on Oct. 24, 2006, and June 5, 2007.

When Messenger zipped by these worlds, NASA took the opportunity to turn on the cameras and instruments and get some data back, since they were in the neighborhood.

At Venus, for example, Messenger snapped 614 pictures. The imaging team then looked at the snapshots to make sure the colors were rendering properly and that the camera was working. Luckily, everything was looking just fine.

Flying by the clouded planet also provided a dress rehearsal for the crucial Mercury flybys; naturally, NASA wanted to make sure all was well on the spacecraft well ahead of arriving at the innermost planet.

An artist's conception shows the MESSENGER spacecraft in orbit around Mercury.
An artist's conception shows the MESSENGER spacecraft in orbit around Mercury.
Credit: NASA

Messenger then did three flybys of Mercury between 2008 and 2009, which was intended to adjust its trajectory to settle into orbit in March 2011.

Scientists were excited by the prospect of mapping Mercury's unseen side, because only one U.S. spacecraft had flown by Mercury before. Although Mariner 10 was a capable spacecraft, its flybys in 1974 and 1975 had only mapped parts of the planet. There was much more for Mercury to show us.

Seeking scientific answers

Some of Messenger's objectives included finding out why Mercury is so dense compared to other planets, understanding Mercury's geologic history and its core, and how the planet's magnetic field works.

Even in the early months of orbiting Mercury, a wealth of new information flowed back to Earth. For example, Messenger found troves of sulfur on Mercury's surface, suggesting a couple of interesting things. Scientists believe Mercury's building blocks not only had less oxidization than other planets, but that the sulfur could reveal clues about Mercury's possible volcanic history. [Infographic: NASA's Messenger Mission to Mercury]

Additionally, Messenger began measuring the depths of craters around the north pole of Mercury, hunting for evidence that there could be spots in permanent shadow from the sun.

Messenger's primary mission to Mercury ended in March 2012, but the spacecraft's mission was extended until at least March 2013.

Part of scientists' motivation for extending the mission was to watch what happened at Mercury as the sun entered a solar maximum, when sunspots and solar activity would increase.

Cores and a 'curious' landscape

In 2012, Messenger discovered that Mercury's core is probably about 85 percent of its radius, which is an immense fraction compared to Earth's core, which is 50 percent of the planet's radius.

As Mercury does have a magnetic field, scientists believe the core must have some liquid in it (since liquid cores are believed to generate magnetic fields.) Still, the structure of Mercury's core is different from any other one known in the solar system. For one thing, there's a layer of solid iron sulfide lying over the planet's core.

NASA also released findings about Mercury's landscape, which it called a "curiosity." Messenger revealed a fairly smooth planet, with less elevation than observed on volcanic Mars or the moon.

The spacecraft's laser altimeter found a large area of lowlands high on the northern face of the planet, and also mapped out a large crater – Caloris Planitia, some 960 miles (1,550 kilometers) in diameter.

Divining water ice

Messenger is on a hunt for water ice, based on observations of very "radar-bright" deposits at both of Mercury's poles.

The spacecraft does have evidence that areas of the poles are in permanent shadow, which would provide the potential ice protection against the sun.

It's a smoking gun, but not definitive proof. NASA says it aims to get more answers by combining pictures with observations from Messenger's laser altimeter and neutron spectrometer.

Even though Messenger is busy in Mercury's orbit, occasionally the scientists can get some pictures of Earth — the spot where the spacecraft came from, and where it will never return.

In 2010, Messenger grabbed a shot of the Earth and the moon from 114 million miles (183 million km) away, a great deal farther away than the distance from the Earth to the sun (93 million miles, or 150 km.)

— Elizabeth Howell, SPACE.com Contributor

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