69230 Hermes

Infobox Planet | discovery=yes | physical_characteristics = yes | bgcolour=#FFFFC0
name=69230 Hermes
discoverer=Karl Wilhelm Reinmuth
discovered=October 28, 1937
alt_names=1937 UB
mp_category=Apollo, Mars-crosser, Venus-crosser
epoch=November 26, 2005 (JD 2453700.5)
semimajor=247.599 Gm (1.655 AU)
perihelion=93.115 Gm (0.622 AU)
aphelion=402.084 Gm (2.688 AU)
eccentricity=0.624
period=777.739 d (2.13 a)
inclination=6.068°
asc_node=34.511°
arg_peri=92.397°
mean_anomaly=325.865°
avg_speed=20.70 km/s
dimensions=0.4 km
mass=6.7×10¹⁰ kg
density=2.0? g/cm³
surface_grav=0.0001? m/s²
escape_velocity=0.0002? km/s
rotation=0.57883±0.00025 d (13.892±0.006 h) [http://www.johnstonsarchive.net/astro/astmoons/am-69230.html]
spectral_type=S
abs_magnitude=17.5
albedo=0.1?
single_temperature=~216 K

69230 Hermes is an Apollo, Mars- and Venus-crosser asteroid that passed Earth at about twice the distance of the Moon on October 30, 1937. It is named after the Greek god Hermes.

At the time, this was the closest known approach of an asteroid to the Earth. Not until 1989 was a closer approach (by 4581 Asclepius) observed. At closest approach, Hermes was moving 5° per hour across the sky and reached 8th magnitude.

It was discovered by Karl Reinmuth in images taken on October 28, 1937. Only five days of observations could be made before Hermes became too faint to be seen in the telescopes of the day. This was not enough to calculate an orbit, and Hermes was "lost". It thus did not receive a number, but Reinmuth nevertheless named it after the Greek god Hermes. It was the only unnumbered but named asteroid, having only the provisional designation 1937 UB.

On October 15, 2003, Brian A. Skiff of the LONEOS project made an asteroid observation that, when the orbit was calculated backwards in time (by Timothy B. Spahr, Steven Chesley and Paul Chodas), turned out to be a rediscovery of Hermes. The orbit is now well known, and Hermes has been assigned sequential number 69230. In retrospect it turned out that Hermes came even closer to the Earth in 1942 than in 1937, within 1.7 Moon distances, without being observed (perhaps due to global political disagreements occurring at that time).

Hermes is an S-type asteroid, a classification first reported by Andy Rivkin and Richard Binzel. Radar observations led by Jean-Luc Margot at Arecibo Observatory and Goldstone in October and November 2003 showed Hermes to be a binary asteroid. The primary and secondary components have nearly identical radii of about 300 m, and their orbital separation is only 1200 m.

In popular culture

* In the 1978 novel, "The Hermes Fall" by John Baxter, the asteroid endangers the Earth in 1980.

External links

*
* [http://www.news.cornell.edu/releases/Oct03/Arecibo.asteroid.deb.html Arecibo 2003 press release]
* [http://www.astro.cornell.edu/~jlm/NEAs/Hermes/index.html Hermes radar results at Cornell University]