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EntityQ151925· pop 42· linked from 14 articles

Also known as (363) Padua, Padua

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
Auguste Charlois
Discovery date
17 March 1893
Pronunciation
/ ˈ p æ d j u ə /
Named after
Padua
Alternative designations
1893 S
Minor planet category
Main belt ( Lydia )
Observation arc
121.80 yr (44489 d)
Aphelion
2.94211 AU (440.133 Gm )
Perihelion
2.55710 AU (382.537 Gm)
Semi major axis
2.74960 AU (411.334 Gm)
Orbital period sidereal
4.56 yr (1665.3 d )
Mean anomaly
193.817 °
Mean motion
0° 12 58.219 / day
Inclination
5.94381°
Longitude of ascending node
64.7678°
Argument of perihelion
295.490°
Dimensions
97 km
Synodic rotation period
8.401 h (0.3500 d )

via Wikipedia infobox

~1 min read

Encyclopedic overview

363 Padua is a main belt asteroid that was discovered by Auguste Charlois on 17 March 1893 in Nice. It was named after the city of Padua (Padova), Italy.

Richard P. Binzel and Schelte Bus further added to the knowledge about this asteroid in a lightwave survey published in 2003. This project was known as Small Main-belt Asteroid Spectroscopic Survey, Phase II or SMASSII, which built on a previous survey of the main-belt asteroids. The visible-wavelength (0.435-0.925 micrometre) spectra data was gathered between August 1993 and March 1999.

Excerpted from Wikipedia’s “Q151925” article, available under the CC BY-SA 4.0 licence.