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Q152422

File:Орбита_астероида_398.png · Wikimedia Commons · See Wikimedia Commons

EntityQ152422· pop 39· linked from 10 articles

Also known as (398) Admete, Admete

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
A. Charlois
Discovery site
Nice Observatory
Discovery date
28 December 1894
Pronunciation
/ æ d ˈ m iː t iː /
Named after
Admete (Greek mythology)
Alternative designations
1894 BN · 1951 LP, 1952 QC 1 · A907 RE
Minor planet category
main-belt · (outer)
Observation arc
120.95 yr (44176 d)
Aphelion
3.3515 AU (501.38 Gm )
Perihelion
2.1269 AU (318.18 Gm)
Semi major axis
2.7392 AU (409.78 Gm)
Orbital period sidereal
4.53 yr (1655.9 d )
Mean anomaly
314.19 °
Mean motion
0° 13 2.64 / day
Inclination
9.5259°
Longitude of ascending node
279.98°
Argument of perihelion
159.02°
Earth moid
1.144 AU (171.1 Gm)

via Wikipedia infobox

~2 min read

Encyclopedic overview

398 Admete, provisional designation 1894 BN, is a dark, carbonaceous asteroid from the outer region of the asteroid belt, about 47 kilometers in diameter. It was discovered on 28 December 1894, by French astronomer Auguste Charlois at Nice Observatory in south-eastern France.

The dark C-type asteroid orbits the Sun at a distance of 2.1–3.4 AU once every four years and six months (1,656 days). Its orbit shows an eccentricity of 0.22, and it is tilted by ten degrees to the plane of the ecliptic. The body's surface has a low albedo of 0.06, a typical value for carbonaceous asteroids.

Excerpted from Wikipedia’s “Q152422” article, available under the CC BY-SA 4.0 licence.