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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
- Raymond Smith Dugan
- Discovery site
- Heidelberg
- Discovery date
- 4 November 1902
- Pronunciation
- / ˈ aɪ v ə /
- Alternative designations
- 1902 KJ
- Observation arc
- 113.45 yr (41,438 d) 113.45 yr (41438 d)
- Aphelion
- 3.7065 AU (554.48 Gm )
- Perihelion
- 1.9966 AU (298.69 Gm)
- Semi major axis
- 2.8516 AU (426.59 Gm)
- Orbital period sidereal
- 4.82 yr (1,758.8 d) 4.82 yr (1758.8 d )
- Mean anomaly
- 242.202 °
- Mean motion
- 0° 12 16.848 / day
- Inclination
- 4.8205°
- Longitude of ascending node
- 6.3305°
- Argument of perihelion
- 3.5819°
- Synodic rotation period
- 4.620 h (0.1925 d )
via Wikipedia infobox
~2 min read
Encyclopedic overview
497 Iva is a main-belt asteroid orbiting the Sun, not to be confused with 1627 Ivar. It was discovered by American astronomer R. S. Dugan on 4 November 1902, and was named for Iva Shores, the young daughter of the family where he was staying in Heidelberg. This object is orbiting at a distance of 2.85 AU with a period of 4.82 yr and an eccentricity of 0.3. The orbital plane is inclined at an angle of 4.8° to the plane of the ecliptic.
This asteroid is classified as an M-type asteroid and is considered anhydrous but oxidized. Further analysis of the spectra suggests the "presence of either an olivine or high-Ca pyroxene phase in addition to orthopyroxene ± Type B clinopyroxene". Analysis of light curves based on photometric data show a rotation period of 4.621±0.001 h with a brightness variation of 0.34±0.02 in magnitude.
Excerpted from Wikipedia’s “497 Iva” article, available under the CC BY-SA 4.0 licence.