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Q151951

File:365_Corduba.png · Wikimedia Commons · See Wikimedia Commons

EntityQ151951· pop 39· linked from 8 articles

Also known as (365) Corduba, Corduba

main-belt asteroid

Picture of the Day · NASA

Pathfinder on Mars

Pathfinder on Mars

2026-07-04

On July 4th, 1997, using its own array of fireworks, a parachute, and a cocoon of airbags, the Mars Pathfinder spacecraft bounced like a giant beach ball at least 15 times before it came to rest on the surface of Mars at 10:07 AM Pacific Daylight Time. After its then novel airbag-assisted landing sequence was completed, Pathfinder transmitted this color mosaic to mission operators on Earth. In the scene from another world, the Mars Sojourner robot rover is visible in the foreground, crouched on top of the unfolded Pathfinder. About the size of a large house cat, the six-wheeled, solar-powered Sojourner became the first successful Martian rover. Surrounding Pathfinder are deflated airbags and the rock-strewn terrain of the Ares Vallis floodplain. In the distance Martian hills appear against a dusty brownish sky. The Pathfinder lander was subsequently renamed the Carl Sagan Memorial Station.

via NASA APOD

Key facts

Discovered by
Auguste Charlois
Discovery date
21 March 1893
Pronunciation
/ ˈ k ɔːr dj ʊ b ə /
Named after
Possibly Córdoba, Spain
Alternative designations
1893 V
Minor planet category
Main belt
Observation arc
117.96 yr (43084 d)
Aphelion
3.2417 AU (484.95 Gm )
Perihelion
2.36078 AU (353.168 Gm)
Semi major axis
2.80122 AU (419.057 Gm)
Orbital period sidereal
4.69 yr (1712.5 d )
Mean anomaly
233.78 °
Mean motion
0° 12 36.792 / day
Inclination
12.792°
Longitude of ascending node
185.196°
Argument of perihelion
216.45°
Dimensions
105.92 ± 3.0 km , 104.51 ± 2.42 km
Mass
(5.84 ± 0.95) × 10 kg

via Wikipedia infobox

~1 min read

Encyclopedic overview

365 Corduba is a very large main-belt asteroid that was discovered by the French astronomer Auguste Charlois on 21 March 1893 from Nice. It is classified as a C-type asteroid and is probably composed of carbonaceous material.

Photometric observations of this asteroid at the Palmer Divide Observatory in Colorado Springs, Colorado, during 2007 gave a light curve with a period of 6.551 ± 0.002 hours and a brightness variation of 0.05 in magnitude. This differs somewhat from a 2004 study that gave a period of 6.354 hours, but this difference may be explained by the small magnitude variation which tends to increase the randomizing effect of noise in the data.

Excerpted from Wikipedia’s “Q151951” article, available under the CC BY-SA 4.0 licence.