391 Ingeborg

Mars-crossing asteroid From Wikipedia, the free encyclopedia

391 Ingeborg (prov. designation: A894 VB or 1894 BE) is an asteroid and second-largest Mars-crosser on an eccentric orbit from the asteroid belt. It was discovered by German astronomer Max Wolf on 1 November 1894, at the Heidelberg Observatory in southwest Germany. When discovered, it was observed for a couple of weeks, and follow-up observations were made in 1901 and 1904.[3][4]

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391 Ingeborg
Modelled shape of Ingeborg from its lightcurve
Discovery[1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date1 November 1894
Designations
(391) Ingeborg
PronunciationGerman: [ˈɪŋəbɔʁk] [2]
Named after
unknown (Ingeborg)[3]
1894 BE · 1934 AJ
A894 VB
Mars-crosser[1][4][5]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc122.86 yr (44,875 days)
Aphelion3.0285 AU
Perihelion1.6120 AU
2.3203 AU
Eccentricity0.3052
3.53 yr (1,291 days)
292.16°
0° 16m 44.04s / day
Inclination23.202°
212.88°
147.06°
Mars MOID0.2350 AU
Physical characteristics
Dimensions15.75±3.05 km[6]
17.33±1.73 km[7]
18.15±0.19 km[8]
19.63 km (calculated)[5]
16 h[9]
26.39±0.02 h[10]
26.391±0.006 h[11]
26.4145±0.0005 h[12]
26.4146±0.0005 h[13]
26.4149±0.0001 h[14]
0.20 (assumed)[5]
0.282±0.056[7]
0.290±0.110[6]
0.34±0.16[6]
0.495±0.013[8]
Tholen = S[1]
SMASS = S[1][5]
10.10[8] · 10.21±0.81[15] · 10.80[1][6][7] · 10.9[5] · 10.9±0.2[16][9]
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    Among the many thousands of named minor planets, Ingeborg is one of 120 asteroids, for which no official naming citation has been published. All of these low-numbered asteroids have numbers between 164 Eva and 1514 Ricouxa and were discovered between 1876 and the 1930s, predominantly by astronomers Auguste Charlois, Johann Palisa, Max Wolf and Karl Reinmuth.[17]

    Ingeborg orbits the Sun in the inner main-belt at a distance of 1.6–3.0 AU once every 3 years and 6 months (1,291 days). Its orbit has an eccentricity of 0.31 and an inclination of 23° with respect to the ecliptic.[1] The stony S-type asteroid has a rotation period of 26.4 hours[3]

    According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Ingeborg measures between 15.75 and 18.15 kilometers in diameter and its surface has an albedo between 0.282 and 0.495.[6][7][8] The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.20 and calculates a diameter of 19.63 kilometers based on an absolute magnitude of 10.9.[5] Other large Mars crossing minor planets include 132 Aethra (43 km), 323 Brucia (36 km), and 2204 Lyyli (25 km).

    References

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