Skip to content
Surf Wiki
Save to docs
society/religion

From Surf Wiki (app.surf) — the open knowledge base

85 Io

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
background#D6D6D6
name85 Io
image85 Io.png
captionLightcurve-based 3D-model of Io on the top and the image of the asteroid on the bottom.
discovererC. H. F. Peters
discovered19 September 1865
mpc_name(85) Io
alt_namesA899 LAA899 UA
pronounced
adjectiveIonian
named_afterIo
mp_categorymain-belt(middle)
Eunomian interloper
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc151.35 yr (55,280 days)
aphelion3.1679 AU
perihelion2.1379 AU
semimajor2.6529 AU
eccentricity0.1941
period4.32 yr (1,578 days)
mean_anomaly83.678°
mean_motion/ day
inclination11.961°
asc_node203.12°
arg_peri123.11°
dimensions180 × 160 × 160 km
mass(5.034 ± 0.999/1.406) kg
density2.14 ± 0.425/0.598 g/cm3
rotation0.2864 d (6.875 h)
albedo0.0666 ± 0.003
spectral_typeFC (Tholen)
B (SMASSII)
abs_magnitude7.96
Note

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 sunstationary, then retrogradeOppositionMinimal 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

  1. [[Noah Webster]]. (1884). "Incitatus–Ithagenes".
  2. http://www.asteroidoccultation.com/2009_03/0312_85_20455.htm {{dead link. (September 2015)
Info: Wikipedia Source

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.

Want to explore this topic further?

Ask Mako anything about 85 Io — get instant answers, deeper analysis, and related topics.

Research with Mako

Free with your Surf account

Content sourced from Wikipedia, available under CC BY-SA 4.0.

This content may have been generated or modified by AI. CloudSurf Software LLC is not responsible for the accuracy, completeness, or reliability of AI-generated content. Always verify important information from primary sources.

Report