National Aeronautics and Space Administration Logo
Follow this link to skip to the main content NASA Banner
Solar System Exploration
News & Events
More on Hermes
More on Hermes
23 Oct 2003
(Source: Cornell University)

http://www.news.cornell.edu/releases/Oct03/Arecibo.asteroid.deb.html

Asteroid Hermes, lost for 66 years, is found to be two objects orbiting each other, astronomers using Arecibo telescope report

FOR RELEASE: Oct. 23, 2003

Contact: David Brand
Office: 607-255-3651
E-mail: deb27@cornell.edu

ARECIBO, P.R. -- , a planetary scientist using the National Science Foundation's (NSF) Arecibo Observatory radio telescope and his colleagues report.

The asteroid Hermes was re-discovered last week after being lost for 66 years. Now Jean-Luc Margot, a researcher in the Department of Earth and Space Sciences at the University of California, Los Angeles, has determined that the asteroid is in fact two objects orbiting each other. The two objects together would cover an area approximately the size of Disneyland.

Margot and colleagues are analyzing new radar measurements from the Arecibo Observatory, Puerto Rico, the world's largest single-dish radio telescope, operated by the National Astronomy and Ionosphere Center (NAIC) at Cornell University, Ithaca, N.Y., for the NSF. The astronomers are scheduled to obtain additional measurements using the Arecibo telescope this weekend (Oct. 25-26).

Hermes makes frequent close approaches to Earth, Venus, Mars, as well as Vesta, the third largest asteroid in the main asteroid belt between Mars and Jupiter.

While several other asteroids have satellites, the other known binaries with trajectories that cross the orbit of the Earth consist of a large primary asteroid orbited by a much smaller one.

"Hermes is the first asteroid ever discovered in the near-Earth population where the two components are essentially equal in size," Margot said. "It's a very unusual binary, a puzzle. It may have formed when it swung so close to a planet that it was ripped apart by gravitational forces, but we don't know for sure. One of our goals is to learn more about the two components and how they rotate about each other in the hopes that we may be able to deduce how Hermes became a double asteroid.

"Because the components are close to each other, they raise appreciable tides in each other and each has slowed down the other's spin significantly. They are now likely in a doubly synchronous state, where their spin period is equal to their orbital period. This means they constantly present the same face to each other, just like Pluto and its satellite, Charon."

Hermes, was first observed in 1937 as a fast-moving bright object and then went undetected until last week, although it had circled the sun almost exactly 31 times since then, said Brian Marsden, of the Minor Planet Center in Cambridge, Mass.

On Oct. 15, Brian Skiff of the Lowell Observatory Near-Earth-Object Search sighted a mysterious object; Timothy Spahr at the Minor Planet Center in Cambridge identified similarities with the 1937 observations, and Steven Chesley and Paul Chodas at NASA's Jet Propulsion Laboratory (JPL) linked the observations to Hermes.

The same day, Margot and his team proposed to observe the asteroid with the Arecibo Observatory's high-powered radar system -- a proposal that was accepted within hours.

The goals of the proposal were to measure precisely the distance and velocity of this object, to improve the knowledge of its trajectory and help trace back its history, to characterize Hermes' physical properties, and to search for satellites.

Margot and collaborators have been given five sessions at Arecibo and five sessions at the Goldstone radar telescope in California to observe Hermes. Due to the urgent nature of the proposal, Margot observed from his home computer while his associates, Mike Nolan, Victor Negron, Alice Hine, and Don Campbell, associate director of NAIC, were at the Arecibo telescope.

Hermes gets as close as 378 000 miles from Earth -- which, in astronomical terms, is quite close, about 1.6 times the distance between Earth and the moon. Orbits can change appreciably over time due to gravitational influences of the planets, noted Nolan, an Arecibo Observatory scientist.

Hermes travels on an elliptical orbit and reaches deep into the inner solar system, crossing Venus' orbit. The new research has made it possible to extend the time interval over which the trajectory can be computed reliably, said Jon Giorgini, a senior engineer at JPL and member of the team.

"As far as impact risk, there is no cause for worry in our lifetimes," Giorgini said. "Over hundreds of thousands or millions of years, Hermes could impact the Earth, but only if it doesn't hit Venus first."

Margot and colleagues described their observations and data in an International Astronomical Union Circular this week. Margot's research is funded by NASA. His co-authors are Nolan, Negron, Hine, Campbell, and Ellen Howell at NAIC; Lance Benner, Steven Ostro, and Giorgini at JPL; and Marsden at the Minor Planet Center.

News Archive Search  Go!
Show  results per page
 
 
Awards and Recognition   Solar System Exploration Roadmap   Contact Us   Site Map   Print This Page
NASA Official: Kristen Erickson
Advisory: Dr. James Green, Director of Planetary Science
Outreach Manager: Alice Wessen
Curator/Editor: Phil Davis
Science Writer: Autumn Burdick
Producer: Greg Baerg
Webmaster: David Martin
> NASA Science Mission Directorate
> Budgets, Strategic Plans and Accountability Reports
> Equal Employment Opportunity Data
   Posted Pursuant to the No Fear Act
> Information-Dissemination Policies and Inventories
> Freedom of Information Act
> Privacy Policy & Important Notices
> Inspector General Hotline
> Office of the Inspector General
> NASA Communications Policy
> USA.gov
> ExpectMore.gov
> NASA Advisory Council
> Open Government at NASA
Last Updated: 28 Oct 2003