190 Ismene

190 Ismene
Orbital diagram
Discovery
Discovered byC. H. F. Peters, 1878
Discovery date22 September 1878
Designations
Pronunciation/ɪsˈmiːniː/
Named after
Ismene
A878 SA; 1947 QJ;
1951 DB
Main belt (Hilda)
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc121.44 yr (44357 d)
Aphelion4.6480 AU (695.33 Gm)
Perihelion3.3248 AU (497.38 Gm)
3.9864 AU (596.36 Gm)
Eccentricity0.16597
7.96 yr (2907.2 d)
134.92°
0° 7m 25.788s / day
Inclination6.1772°
175.48°
271.47°
Physical characteristics
79.5 km
90 km
Mass(5.23±0.82)×1018 kg
Mean density
2.49 g/cm3
6.52 h (0.272 d)3[link removed]
0.066
P
7.77
7.59

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.

Notes

  1. ↑ Calculated from its standard gravitational parameter GM = 0.349±0.055 km3/s2.
  2. ↑ Assuming a diameter of 159 km.

References

  1. ↑ Noah Webster (1884) A Practical Dictionary of the English Language
  2. 1 2 3 Yeomans, Donald K., "190 Ismene", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, 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 14 July 2014. Retrieved 11 June 2014.
  4. 1 2 Fuentes-Muñoz, Oscar; Farnocchia, Davide; Giorgini, Jon D.; Park, Ryan S. (1 December 2025). "Asteroid Mass Estimation by Mutual Perturbations During Close Encounters After Gaia Focused Product Release". The Astronomical Journal. 170 (6): 353. Bibcode:2025AJ....170..353F. doi:10.3847/1538-3881/ae0cc9. ISSN 0004-6256. S2CID 283347135.
  5. ↑ Warner, Brian D. (December 2007), "Initial Results of a Dedicated H-G Project", The Minor Planet Bulletin, 34 (4): 113–119, Bibcode:2007MPBu...34..113W.
  6. ↑ Dahlgren, M.; Lagerkvist, C.-I. (October 1995), "A study of Hilda asteroids. I. CCD spectroscopy of Hilda asteroids", Astronomy and Astrophysics, 302: 907, Bibcode:1995A&A...302..907D.