437 Rhodia

Rhodia (minor planet designation: 437 Rhodia) is a Main belt asteroid that was discovered by French astronomer Auguste Charlois on 16 July 1898 in Nice. It was named after one of the Oceanid nymphs of Greek mythology.[4] This asteroid is orbiting the Sun at a distance of 2.39 AU with a period of 3.69 years and an eccentricity (ovalness) of 0.25. The orbital plane is tilted at an angle of 7.3° to the plane of the ecliptic.[2] 437 Rhodia was originally a proposed fly-by target of interest for the Rosetta mission.[5]

437 Rhodia
Discovery
Discovered byAuguste Charlois
Discovery date16 July 1898
Designations
(437) Rhodia
Pronunciation/rˈdə/[1]
Named after
Ῥόδεια Rhodeia
1898 DP
Main belt
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc117.73 yr (43,001 d)
Aphelion2.9793 AU (445.70 Gm)
Perihelion1.79242 AU (268.142 Gm)
2.38586 AU (356.920 Gm)
Eccentricity0.24873
3.69 yr (1,346.1 d)
355.267°
0° 16m 2.82s / day
Inclination7.3442°
263.22°
62.058°
Physical characteristics
Dimensions13.12±0.7 km[2]
56 h (2.3 d)
0.7035±0.084[2][3]
10.41[2]

    Analysis of the bimodal light curve generated using photometric data show a lengthy rotation period of 433.2 ± 0.5 hours (18.05 ± 0.02 days) with a brightness variation of 0.35±0.05 in magnitude. It also appears to be tumbling.[6] 437 Rhodia is classified as an E-type asteroid with a diameter of approximately 13 km. This object has the highest albedo in the IRAS dataset, with a value of 0.70±0.08.[7]

    References

    1. Noah Webster (1884) A Practical Dictionary of the English Language
    2. "JPL Small-Body Database Browser: 437 Rhodia (1898 DP)" (2008-05-13 last obs). Retrieved 10 May 2016.
    3. Johnston, Wm. Robert (28 June 2003). "Asteroid albedos: graphs of data". Johnston's Archive. Archived from the original on 17 May 2008. Retrieved 16 June 2008.
    4. Schmadel, Lutz D. (2012), Dictionary of Minor Planet Names, Springer Berlin Heidelberg, p. 48, ISBN 9783642297182.
    5. Barucci, M. A.; et al. (January 2005), "Asteroid target selection for the new Rosetta mission baseline. 21 Lutetia and 2867 Steins", Astronomy and Astrophysics, 430: 313–317, Bibcode:2005A&A...430..313B, doi:10.1051/0004-6361:20041505.
    6. Pilcher, Frederick; Polakis, Tom (July 2018), "A Photometric Study of 437 Rhodia", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers, 45 (3): 287–289, Bibcode:2018MPBu...45..287P.
    7. Fornasier, S.; et al. (July 2008), "Visible and near infrared spectroscopic investigation of E-type asteroids, including 2867 Steins, a target of the Rosetta mission" (PDF), Icarus, 196 (1): 119–134, Bibcode:2008Icar..196..119F, doi:10.1016/j.icarus.2008.02.015, S2CID 122794657.


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