Saturday, July 17, 2010

Final Mercury Flyby Reveals Huge Magnetic "Power Surges"

MESSENGER in Orbit (with Sun)Artist's impression of the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft in orbit at Mercury. MESSENGER launched from Cape Canaveral Air Force Station, Fla., on Aug. 3, 2004, and will begin a yearlong orbital study of Mercury in March 2011. Though the Sun is up to 11 times brighter at Mercury than we see on Earth and surface temperatures can reach 450 degrees Celsius (about 840 degrees Fahrenheit), MESSENGER's instruments will operate at room temperature behind a sunshade of heat-resistant ceramic fabric. The spacecraft will also pass only briefly over the hottest parts of the surface, limiting exposure to heat reradiated from the planet.Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of WashingtonThe space weather report for Mercury: stormy, with a chance of power surges.

New data from the third and final flyby of the MESSENGER (MErcury Surface, Space ENvironment, GEochemistry, and Ranging) spacecraft have revealed surprisingly intense electromagnetic storms in Mercury's magnetic "tail," part of the planet's magnetic field. ...

Such tails form when the solar wind—charged particles streaming from the sun—pushes on a planet's magnetic field. The deformed field flows around the planet in a windsock shape, like river water flowing around a rock.

All eight planets in the solar system except Mars and Venus have magnetic fields and tails, although Mercury's field is the smallest and weakest.

But during a September 29, 2009, flyby of the tiny planet, MESSENGER watched as Mercury's magnetic tail collected enormous amounts of energy from the solar wind.

In just 90 seconds, the tail increased magnetic field power by 200 percent during an event known as a magnetic substorm. The tail then snapped back to normal, dissipating the energy over the next minute and a half.

On Earth, a similar process—called tail loading—takes an hour and increases the magnetic field's energy by only about 10 percent.

"This is all very curious," said Jim Slavin, a solar physicist at NASA Goddard Spaceflight Center and lead author of a new paper describing the finding.

"We have very weak solar wind conditions, yet we're seeing more tail loading than what we see on Earth. What's going to happen when the [solar] wind conditions pick up?" ...

via Final Mercury Flyby Reveals Huge Magnetic "Power Surges".

No comments: