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117 Lomia

File:000117-asteroid_shape_model_(117)_Lomia.png · Wikimedia Commons · See Wikimedia Commons

EntityQ136712· pop 47· linked from 8 articles

Also known as (117) Lomia, Lomia

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
Alphonse Borrelly
Discovery date
12 September 1871
Pronunciation
/ ˈ l oʊ m i ə /
Alternative designations
A871 RB;1900 DA;, 1900 MC
Minor planet category
Main belt
Adjectives
Lomian
Observation arc
123.03 yr (44938 d)
Aphelion
3.0759 AU (460.15 Gm )
Perihelion
2.90810 AU (435.046 Gm)
Semi major axis
2.99201 AU (447.598 Gm)
Orbital period sidereal
5.18 yr (1890.4 d )
Average orbital speed
17.22 km/s
Mean anomaly
317.47 °
Mean motion
0° 11 25.584 / day
Inclination
14.902°
Longitude of ascending node
348.790°
Argument of perihelion
52.461°
Earth moid
1.92459 AU (287.915 Gm)

via Wikipedia infobox

Wikidata facts

Instance of
asteroid
Named after
Lamia
Followed by
118 Peitho
Follows
116 Sirona
Parent body
Sun
Minor-planet group
asteroid belt
Diameter
208.974
Orbital period
1890.234463890318
Show 19 more facts
discoverer or inventor
Alphonse Borrelly
site of astronomical discovery
Marseille Observatory
provisional designation
A871 RB
time of discovery or invention
1871-09-12
asteroid spectral type
X-type asteroid
orbital inclination
14.92192499871803
albedo
0.027
argument of periapsis
53.24201092795472
Commons category
117 Lomia
rotation period
9.127
absolute magnitude
8.15
orbital eccentricity
0.02292109180801113
semi-major axis of an orbit
2.991884567109772
periapsis
2.923307306268077
apoapsis
3.060461827951467
longitude of ascending node
348.6167919181505
mean anomaly
244.3981700028092
time of periapsis
2461607.4848976373
Sources (2)

via Wikidata · CC0

~2 min read

Encyclopedic overview

117 Lomia is a large main-belt asteroid that has a nearly circular orbit; the orbital eccentricity is 0.029. It was discovered by French astronomer Alphonse Borrelly on September 12, 1871, from the Marseilles Observatory. The preliminary orbital elements were published in the following year by German astronomer Friedrich Tietjen. The reason for the name is uncertain, but Lutz D. Schmadel believes it is most likely a misspelling of Lamia, the female demon of Greek mythology (the asteroid 248 Lameia is also named after this figure).

Photometric observations of this asteroid in 1985 gave a light curve with a period of 9.127±0.009 hours and a brightness variation of 0.29±0.03 in magnitude. The curve is symmetrical with a single maxima and minima. This object has a spectrum that matches an XC classification; occupying the transition range between an X-type and a C-type asteroid. It has an estimated cross-section diameter of ~148 km.

Excerpted from Wikipedia’s “117 Lomia” article, available under the CC BY-SA 4.0 licence.

Gallery (3)