File:191_Kolga.png · Wikimedia Commons · See Wikimedia Commons
Picture of the Day · NASA

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
- C. H. F. Peters
- Discovery date
- 30 September 1878
- Pronunciation
- / ˈ k ɒ l ɡ ə /
- Named after
- Kólga
- Minor planet category
- Main belt
- Observation arc
- 131.26 yr (47942 d)
- Aphelion
- 3.1588 AU (472.55 Gm )
- Perihelion
- 2.6313 AU (393.64 Gm)
- Semi major axis
- 2.8951 AU (433.10 Gm)
- Orbital period sidereal
- 4.93 yr (1799.2 d )
- Mean anomaly
- 326.28 °
- Mean motion
- 0° 12 0.288 / day
- Inclination
- 11.508°
- Longitude of ascending node
- 159.31°
- Argument of perihelion
- 227.00°
- Earth moid
- 1.64648 AU (246.310 Gm)
- Jupiter moid
- 2.29413 AU (343.197 Gm)
- Dimensions
- ( 134.3 ± 12.8 ) × ( 78.2 ± 1.7 ) km
via Wikipedia infobox
~1 min read
Encyclopedic overview
191 Kolga is a large, dark main-belt asteroid that was discovered by German-American astronomer C. H. F. Peters on September 30, 1878, in Clinton, New York. It is named after Kólga, the daughter of Ægir in Norse mythology.
In 2009, Photometric observations of this asteroid were made at the Palmer Divide Observatory in Colorado Springs, Colorado. The resulting light curve shows a synodic rotation period of 17.625 ± 0.004 hours with a brightness variation of 0.30 ± 0.03 in magnitude. Previous independent studies produced inconsistent results that differ from this finding.
Excerpted from Wikipedia’s “191 Kolga” article, available under the CC BY-SA 4.0 licence.