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762 Pulcova

File:762Pulcova-SwRI.gif · Wikimedia Commons · See Wikimedia Commons

EntityQ156985· pop 41· linked from 125 articles

762 Pulcova

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Also known as (762) Pulcova, Pulcova

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
G. N. Neujmin
Discovery date
3 September 1913
Pronunciation
/ ˈ p ʊ l k ə v ə /
Named after
Pulkovo Heights
Alternative designations
1913 SQ
Minor planet category
Main belt
Adjectives
Pulcovian / p ʊ l ˈ k oʊ v i ə n /
Observation arc
100.08 yr (36553 d)
Aphelion
3.4801 AU (520.62 Gm ) (Q)
Perihelion
2.8291 AU (423.23 Gm) (q)
Semi major axis
3.1546 AU (471.92 Gm) (a)
Eccentricity
0.10319 (e)
Orbital period sidereal
5.60 yr (2046.5 d )
Mean anomaly
348.62 ° (M)
Mean motion
0° 10 33.276 / day (n)
Inclination
13.089° (i)
Longitude of ascending node
305.76° (Ω)
Argument of perihelion
189.54° (ω)

via Wikipedia infobox

~2 min read

Encyclopedic overview

762 Pulcova is a main-belt asteroid. It was discovered by Grigoriy N. Neujmin in 1913, and is named after Pulkovo Observatory, near Saint Petersburg. Pulcova is 137 km in diameter, and is a C-type asteroid, which means that it is dark in colouring with a carbonate composition.

Photometric observations of this asteroid from Leura, Australia during 2006 gave a light curve with a period of 5.8403 ± 0.0005 hours and a brightness variation of 0.20 ± 0.02 in magnitude. This result is in agreement with previous studies.

Excerpted from Wikipedia’s “762 Pulcova” article, available under the CC BY-SA 4.0 licence.

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