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
- A. Schwassmann, Bergedorf
- Discovery date
- 27 April 1919
- Pronunciation
- / m ə ˈ r ɪ t ɪ m ə /
- Minor planet category
- Main belt
- Observation arc
- 85.59 yr (31263 days)
- Aphelion
- 3.6842 AU (551.15 Gm ) (Q)
- Perihelion
- 2.5842 AU (386.59 Gm) (q)
- Semi major axis
- 3.1342 AU (468.87 Gm) (a)
- Eccentricity
- 0.17548 (e)
- Orbital period sidereal
- 5.55 yr (2026.7 d )
- Mean anomaly
- 282.25 ° (M)
- Mean motion
- 0° 10 39.468 / day (n)
- Inclination
- 18.344° (i)
- Longitude of ascending node
- 34.032° (Ω)
- Argument of perihelion
- 88.889° (ω)
- Mean radius
- 41.585 ± 1 km ( IRAS )
- Synodic rotation period
- 1,332 h (55.5 d )
- Geometric albedo
- 0.1115 ± 0.006
via Wikipedia infobox
~1 min read
Encyclopedic overview
912 Maritima is an asteroid in the asteroid belt. Based on lightcurve studies observing Maritima over a three-month period, Maritima has a rotation period of 1332 hours. Analysis reveals a possible synodic period of 1332±5 h. Superslow rotators, those with periods longer than a few days, are generally small asteroids. The current paradigm is that slowing of an asteroid's spin rate is the result of YORP radiation pressure, which acts on the target as the inverse square of its size and the inverse of its semi-major axis. The rotation period is less than conclusive.
References
Excerpted from Wikipedia’s “Q157855” article, available under the CC BY-SA 4.0 licence.