Astronomy:190 Ismene

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190 Ismene
Орбита астероида 190.png
Orbital diagram
Discovery
Discovered byC. H. F. Peters, 1878
Discovery date22 September 1878
Designations
(190) Ismene
Pronunciation/ɪsˈmn/[1]
Named afterIsmene
A878 SA; 1947 QJ;
1951 DB
Minor planet categoryMain belt (Hilda)
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc121.44 yr (44357 d)
|{{{apsis}}}|helion}}4.6480 astronomical unit|AU (695.33 Gm)
|{{{apsis}}}|helion}}3.3248 AU (497.38 Gm)
3.9864 AU (596.36 Gm)
Eccentricity0.16597
Orbital period7.96 yr (2907.2 d)
Mean anomaly134.92°
Mean motion0° 7m 25.788s / day
Inclination6.1772°
Longitude of ascending node175.48°
271.47°
Physical characteristics
Mean radius79.5 km [2]
90 km [3]
Rotation period6.52 h (0.272 d)3
Geometric albedo0.066
P
Absolute magnitude (H)7.77[4]
7.59[2]


Ismene (minor planet designation: 190 Ismene) is a very large main belt asteroid. It was discovered by German-American astronomer C. H. F. Peters on September 22, 1878, in Clinton, New York, and named after Ismene, the sister of Antigone in Greek mythology.

Being a P-type asteroid, it has a very dark surface. Ismene orbits near the outer edge of the asteroid belt. It is one of the largest members of the Hilda asteroid family, which are locked in 3:2 resonance with the planet Jupiter.[5]

References

  1. Noah Webster (1884) A Practical Dictionary of the English Language
  2. 2.0 2.1 2.2 Yeomans, Donald K., "190 Ismene", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=190, retrieved 6 May 2016. 
  3. "IOTA/IOTA-ES occultation update for (190) Ismene / TYC 0790-00635-1 event on 2014 Jan 18, 19:57 UT". Archived from the original on 2014-07-14. https://web.archive.org/web/20140714172851/http://www.asteroidoccultation.com/2014_01/0118_190_32108_Summary.txt. Retrieved 2014-06-11. 
  4. Warner, Brian D. (December 2007), "Initial Results of a Dedicated H-G Project", The Minor Planet Bulletin 34: pp. 113–119, Bibcode2007MPBu...34..113W. 
  5. Dahlgren, M.; Lagerkvist, C.-I. (October 1995), "A study of Hilda asteroids. I. CCD spectroscopy of Hilda asteroids", Astronomy and Astrophysics 302: 907, Bibcode1995A&A...302..907D. 

External links