Probe spots Mercury's curious tail

Boston University - CSP

This image of Mercury's tail was obtained by combining a full day's worth of data from a camera aboard the STEREO-A spacecraft. The reflected sunlight off the planet's surface results in a type of overexposure that causes Mercury to appear much larger than actual size.

Comets aren't the only solar system objects that can grow a tail: NASA's STEREO mission has spotted a tail of faintly glowing gas stretching out from the planet Mercury. Now scientists are trying to figure out exactly what's in that thing.

Astronomers have known for some time that Mercury has some characteristics in common with comets, even though the composition of the closest-in planet is dramatically different from that of the dirty snowballs that ramble through our solar system's icy outer reaches. Mercury is surrounded by an exceedingly thin "coma" of gas, and radiation from the sun pushes a tail of atoms from that coma outward for more than a million miles.

The two satellites involved in the STEREO mission are designed to observe the sun's escaping atmosphere from positions in Earth's orbit that track ahead and behind our planet. Ian Musgrave, an Australian medical researcher who's also interested in astronomy, happened to be sifting through the online database of STEREO's imagery — and noticed that those images also recorded emissions from the Mercurial tail.

When Musgrave pointed that out to scientists at Boston University's Center for Space Physics, the professionals were intrigued. "Now we have found several cases, with detections by both STEREO satellites," Jeffrey Baumgardner, senior research associate at the center, said today in a news release that was timed to coincide with a presentation at the European Planetary Science Congress in Rome.

The tale isn't exactly new: A couple of years ago, Boston University astronomers used ground observations to map the tail's extent to a distance of 1.5 million miles. For that project, they were guided by the bright light emitted from sodium atoms. But even then, they knew that sodium was not the major component of the tail material. STEREO's readings confirm that other elements are involved.

"What makes the STEREO detections so interesting is that the brightness levels seem to be too strong to be from sodium," said BU graduate student Carl Schmidt, lead author of the paper presented at the meeting in Rome.

Now astronomers are trying to sort out all the possibilities for the chemical composition of the tail — a job that will require further refinement of the STEREO observations. And something tells me that Schmidt right in there with the best of them.

"The combination of our ground-based data with the new STEREO data is an exciting way to learn as much as possible about the sources and fates of gases escaping from Mercury," said Michael Mendillo, director of Boston University's Imaging Science Lab. "This is precisely the type of research that makes for a terrific Ph.D. dissertation."

More tales about tails:


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Discuss this post

Tails (or directional outgassings) are exoteric in stellar system bodies. There's absolutely nothing unusual about them. Every type of body within the influence of a star (planetary, cometary, asteroidal, etc.) all outgas, experience shear effects, or re-radiate energy received, and all of that tails away from the star along the lines of the stellar "wind". I'm not exactly sure why it becomes a news event every time someone manages to get a different shot of a tail. I am not impressed.

    Reply#1 - Wed Sep 22, 2010 9:24 PM EDT

    My impression is that these observations are notable because they could lead to a better understanding of what's in the tail material, other than sodium. Maybe it could shed light on Mercury's ice reserves. My bet is that NASA's Messenger probe will find out much more about what's going on once it goes into orbit.

      #1.1 - Wed Sep 22, 2010 10:58 PM EDT

      Granted. With the science focus being composition, then certainly some new and useful details could arise. Not sure what further reduction of these completely serendipitous observations from STEREO -- a pair of instruments designed to "trace the flow of energy and matter from the Sun to Earth" -- could possibly reveal in the way of chemical composition of the tail. There's nothing spectroscopic on-board these craft, and no instrument pairings within a suitable wavelength regime to get at the composition. Maybe these observations can assist in pinpointing just where and how to conduct new ground-based measurements to find out more? And, yes...all roads lead to Messenger.

        #1.2 - Thu Sep 23, 2010 2:46 AM EDT
        Reply

        interesting. Composition was my first question too. I suspect it is iron, never thought of iron as a gas before though. I guess no one thought of pointing a spectroscope at it? Perhaps the suns emmisions make for a difficult reading, like trying to read a single sheet of paper while holding it up in front of a 1000 watt light bulb. I posted though to at least posist the possibility that the suns gravity is constantly pulling in debris, perhaps it is not from mercury per se, rather debris ionized in mercs magnetic tail...just a hypothesis, nothing serious. Either way, I trust we can count on a cosmic log article once we have a consensus or at least data from the next probe..

          Reply#2 - Thu Sep 23, 2010 12:30 AM EDT

          Wow. Mercury has a TAIL! Sorry, somehow I seem to have missed that one. Thanks! It's good to learn new things.

            Reply#3 - Thu Sep 23, 2010 9:49 AM EDT
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