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382 Dodona

File:382Dodona_(Lightcurve_Inversion).png · Wikimedia Commons · See Wikimedia Commons

EntityQ152227· pop 42· linked from 8 articles

382 Dodona

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Also known as (382) Dodona, Dodona

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
29 January 1894
Pronunciation
/ d ə ˈ d oʊ n ə /
Named after
Dodona
Alternative designations
1894 AT
Minor planet category
Main belt
Observation arc
122.21 yr (44636 d)
Aphelion
3.6577 AU (547.18 Gm )
Perihelion
2.58301 AU (386.413 Gm)
Semi major axis
3.1204 AU (466.81 Gm)
Orbital period sidereal
5.51 yr (2013.3 d )
Mean anomaly
6.32892 °
Mean motion
0° 10 43.716 / day
Inclination
7.3928°
Longitude of ascending node
313.511°
Argument of perihelion
270.036°
Dimensions
58.37 ± 2.8 km , 58.37 km
Synodic rotation period
4.113 h (0.1714 d )

via Wikipedia infobox

~1 min read

Encyclopedic overview

382 Dodona is a large Main belt asteroid that was discovered by the French astronomer Auguste Charlois on 29 January 1894 in Nice. It is classified as an M-type asteroid.

Measurements of the thermal inertia of 115 Thyra give an estimated range of 15–150 J m K s, compared to 50 for lunar regolith and 400 for coarse sand in an atmosphere.

Excerpted from Wikipedia’s “382 Dodona” article, available under the CC BY-SA 4.0 licence.