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85 Io
Main-belt asteroid
Main-belt asteroid
| Field | Value |
|---|---|
| minorplanet | yes |
| background | #D6D6D6 |
| name | 85 Io |
| image | 85 Io.png |
| caption | Lightcurve-based 3D-model of Io on the top and the image of the asteroid on the bottom. |
| discoverer | C. H. F. Peters |
| discovered | 19 September 1865 |
| mpc_name | (85) Io |
| alt_names | A899 LAA899 UA |
| pronounced | |
| adjective | Ionian |
| named_after | Io |
| mp_category | main-belt(middle) |
| Eunomian interloper | |
| orbit_ref | |
| epoch | 4 September 2017 (JD 2458000.5) |
| uncertainty | 0 |
| observation_arc | 151.35 yr (55,280 days) |
| aphelion | 3.1679 AU |
| perihelion | 2.1379 AU |
| semimajor | 2.6529 AU |
| eccentricity | 0.1941 |
| period | 4.32 yr (1,578 days) |
| mean_anomaly | 83.678° |
| mean_motion | / day |
| inclination | 11.961° |
| asc_node | 203.12° |
| arg_peri | 123.11° |
| dimensions | 180 × 160 × 160 km |
| mass | (5.034 ± 0.999/1.406) kg |
| density | 2.14 ± 0.425/0.598 g/cm3 |
| rotation | 0.2864 d (6.875 h) |
| albedo | 0.0666 ± 0.003 |
| spectral_type | FC (Tholen) |
| B (SMASSII) | |
| abs_magnitude | 7.96 |
the asteroid
Eunomian interloper B (SMASSII)
85 Io is a carbonaceous asteroid in the central region of the asteroid belt, approximately 170 kilometers in diameter. It is an identified Eunomian interloper.
Discovery and naming
It was discovered by C. H. F. Peters on 19 September 1865, and named after Io, a lover of Zeus in Greek mythology. Io is also the name of the volcanic satellite of Jupiter. With a two-digit number and a two-letter name, 85 Io has the shortest designation of all minor planets.
Orbit and physical characteristics
Io is a retrograde rotator, with its pole pointing towards one of ecliptic coordinates (β, λ) = (-45°, 105°) or (-15°, 295°) with a 10° uncertainty. This gives an axial tilt of about 125° or 115°, respectively. Its shape is quite regular.
In the SMASS classification, Io is a carbonaceous C-type asteroid, which means that it is probably a primitive body composed of carbonates. Like 141 Lumen it is an interloper that orbits within the Eunomia asteroid family but it is not related to the shattered parent body.
An Ionian diameter of 178 kilometres was measured from an occultation of a star on 10 December 1995. Another asteroid occultation of Io (magnitude 13.2) occurred on 12 March 2009, from the eastern United States, with the star 2UCAC 35694429 (magnitude 13.8).
| Conjunction to sun | stationary, then retrograde | Opposition | Minimal distance (AE) | Maximum brightness (mag) | stationary, then prograde | |||||
|---|---|---|---|---|---|---|---|---|---|---|
| 27. April 2004 | ||||||||||
| 3.August 2005 | ||||||||||
| 17.October 2006 | ||||||||||
| 7. March 2008 | ||||||||||
| 8. July 2009 | ||||||||||
| 21. September 2010 | ||||||||||
| 7. January 2012 | ||||||||||
| 9.June 2013 | ||||||||||
| 29.August 2014 | ||||||||||
| 22.November 2015 | ||||||||||
| 3.May 2017 | ||||||||||
| 6.August 2018 | ||||||||||
| 21.October 2019 |
Notes
References
|access-date=1 November 2017}}
|display-authors=etal
|doi-access=free}}
References
- [[Noah Webster]]. (1884). "Incitatus–Ithagenes".
- http://www.asteroidoccultation.com/2009_03/0312_85_20455.htm {{dead link. (September 2015)
This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.
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