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EntityQ154719· pop 39· linked from 11 articles

Also known as (482) Petrina, Petrina

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
Max Wolf
Discovery site
Heidelberg
Discovery date
3 March 1902
Pronunciation
/ p ɛ ˈ t r aɪ n ə /
Alternative designations
1902 HT
Observation arc
111.53 yr (40737 d)
Aphelion
3.2971 AU (493.24 Gm )
Perihelion
2.7064 AU (404.87 Gm)
Semi major axis
3.0017 AU (449.05 Gm)
Orbital period sidereal
5.20 yr (1899.6 d )
Mean anomaly
287.189 °
Mean motion
0° 11 22.272 / day
Inclination
14.474°
Longitude of ascending node
179.408°
Argument of perihelion
86.737°
Mean radius
23.285 ± 1.4 km
Synodic rotation period
11.7922 h (0.49134 d )
Geometric albedo
0.2372 ± 0.032

via Wikipedia infobox

~1 min read

Encyclopedic overview

482 Petrina is a minor planet orbiting the Sun.

Attempts to produce a light curve for this object have yielded differing synodic rotation periods, perhaps in part because the period is close to half an Earth day. Observations suggest that the pole of rotation is near the orbital plane, yielding only small light variations during certain parts of each orbit. Attempts to observe the asteroid photometrically during an optimal viewing period of the object's orbit gave a rotation period of 11.7922 ± 0.0001 h with an amplitude variation of 0.53 ± 0.05 in magnitude.

Excerpted from Wikipedia’s “Q154719” article, available under the CC BY-SA 4.0 licence.