Scientists measure how deep 'Deep Impact' was, with X-rays

July 8, 2005

Here come the X-rays, on cue. Scientists studying the Deep Impact collision using NASA's Swift satellite report that comet Tempel 1 is getting brighter and brighter in X-ray light with each passing day.

The X-rays provide a direct measurement of how much material was kicked up in the impact. This is because the X-rays are created by the newly liberated material lifted into the comet's thin atmosphere and illuminated by the high-energy solar wind from the sun. The more material liberated, the more X-rays are produced.

Swift data of the water evaporation on comet Tempel 1 also may provide new insights into how solar wind can strip water from planets such as Mars.

"Prior to its rendezvous with the Deep Impact probe, the comet was a rather dim X-ray source," said Paul O'Brien of the Swift team at the University of Leicester. "How things change when you ram a comet with a copper probe traveling over 20,000 miles per hour. Most of the X-ray light we detect now is generated by debris created by the collision. We can get a solid measurement of the amount of material released."

"It takes several days after an impact for surface and sub-surface material to reach the comet's upper atmosphere, or coma," said Dick Willingale, also of the University of Leicester. "We expect the X-ray production to peak this weekend. Then we will be able to assess how much comet material was released from the impact."

Based on preliminary X-ray analysis, O'Brien estimates that several tens of thousands of tons of material were released, enough to bury Penn State's football field under 30 feet of comet dust. Observations and analysis are ongoing at the Swift Mission Operations Center at Penn State as well as in Italy and the United Kingdom.

Swift is providing the only simultaneous multi-wavelength observation of this rare event, with a suite of instruments capable of detecting visible light, ultraviolet light, X-rays and gamma rays. Different wavelengths reveal different secrets about the comet.

The Swift team hopes to compare the satellite's ultraviolet data, collected hours after the collision, with the X-ray data. The ultraviolet light was created by material entering into the lower region of the comet's atmosphere; the X-rays come from the upper regions. Swift is a nearly ideal observatory for making these comet studies, as it combines both a rapidly responsive scheduling system with both X-ray and optical/UV instruments in the same satellite.

"For the first time, we can see how material liberated from a comet's surface migrates to the upper reaches of its atmosphere," said John Nousek, director of Mission Operations at Penn State. "This will provide fascinating information about a comet's atmosphere and how it interacts with the solar wind. This is all virgin territory."

Nousek said Deep Impact's collision with comet Tempel 1 is like a controlled laboratory experiment of the type of slow evaporation process from solar wind that took place on Mars. The Earth has a magnetic field that shields us from solar wind, a particle wind composed mostly of protons and electrons moving at nearly light speed. Mars lost its magnetic field billions of years ago, and the solar wind stripped the planet of water.

Comets, like Mars and Venus, have no magnetic fields. Comets become visible largely because ice is evaporated from their surface with each close passage around the Sun. Water is dissociated into its component atoms by the bright sunlight and swept away by the fast-moving and energetic solar wind. Scientists hope to learn about this evaporation process on Tempel 1 now occurring quickly -- over the course of a few weeks instead of a billion years -- as the result of a planned, human intervention.

Swift's "day job" is detecting distant, natural explosions called gamma-ray bursts and creating a map of X-ray sources in the universe. Swift's extraordinary speed and agility enable scientists to follow Tempel 1 day by day to see the full effect from the Deep Impact collision.

For the latest news on Swift analysis of comet Tempel 1, refer to:
-- http://www.science.psu.edu/alert/Swift-Deep-Impact.htm
-- http://swift.gsfc.nasa.gov and
-- http://swift.sonoma.edu/

Source: Penn State


print this article email this article download pdf blog this article bookmark this article     Stumble it Digg this share on Facebook retweet share on Reddit add to delicious
Rate this story - not rated yet


July 8, 2005 all stories

Comments: 0

not rated yet
  • Stumble this up

  • Digg this

  • share this

  • hide
  • Related Stories

  • Hidden Territory on Mercury Revealed
    created Nov 04, 2009 | popularity not rated yet | comments 0
  • 'Ultra-primitive' particles found in comet dust
    created Nov 02, 2009 | popularity not rated yet | comments 0
  • Icebreaker: Scientist brings out big gun to explore behavior of ice in planetary collisions
    created Oct 29, 2009 | popularity not rated yet | comments 0
  • Moon crash: Public yawns, scientists celebrate
    created Oct 10, 2009 | popularity not rated yet | comments 0
  • Israelis bring green power to West Bank village
    created Oct 09, 2009 | popularity not rated yet | comments 0


Other News

Exoplanets Clue to Sun's Curious Chemistry

Exoplanets Clue to Sun's Curious Chemistry

Space & Earth / Astronomy

created 10 hours ago | popularity 4.9 / 5 (14) | comments 11

(PhysOrg.com) -- A ground-breaking census of 500 stars, 70 of which are known to host planets, has successfully linked the long-standing "lithium mystery" observed in the Sun to the presence of planetary systems. ...


Earth's early ocean cooled more than a billion years earlier than thought: Stanford study

Earth's early ocean cooled more than a billion years earlier than thought (w/ Video)

Space & Earth / Earth Sciences

created 10 hours ago | popularity 4.8 / 5 (6) | comments 0

(PhysOrg.com) -- The scalding-hot sea that supposedly covered the early Earth may in fact never have existed, according to a new study by Stanford University researchers who analyzed isotope ratios in 3.4 ...


A bubbling ball of gas

A bubbling ball of gas (w/ Video)

Space & Earth / Space Exploration

created 11 hours ago | popularity 5 / 5 (12) | comments 4

The Sun is a bubbling mass. Packages of gas rise and sink, lending the sun its grainy surface structure, its granulation. Dark spots appear and disappear, clouds of matter dart up - and behind the whole thing ...


A Tale of Planetary Woe

A Tale of Planetary Woe (w/ Video)

Space & Earth / Space Exploration

created 7 hours ago | popularity 5 / 5 (4) | comments 1

Once upon a time — roughly four billion years ago — Mars was warm and wet, much like Earth. Liquid water flowed on the Martian surface in long rivers that emptied into shallow seas. A thick atmosphere blanketed ...


Researchers Discover Use for Carbon Dioxide in Conversion of Biomass Into Biofuel

Researchers Discover Use for Carbon Dioxide in Conversion of Biomass Into Biofuel

Space & Earth / Environment

created 7 hours ago | popularity 3.7 / 5 (7) | comments 1

(PhysOrg.com) -- Researchers at Columbia University have successfully discovered a beneficial use for carbon dioxide in the conversion of organic materials, such as grass and bark, into fuel. Their findings ...