114 Kassandra is a large and dark main-belt asteroid. It belongs to the rare class T. It was discovered by C. H. F. Peters on July 23, 1871, and is named after Cassandra, the prophetess in the tales of the Trojan War.
_Kassandra.png) 3D convex shape model of 114 Kassandra | |
| Discovery | |
|---|---|
| Discovered by | Christian Heinrich Friedrich Peters |
| Discovery date | 23 July 1871 |
| Designations | |
| (114) Kassandra | |
| Pronunciation | /kəˈsændrə/[1] |
Named after | Cassandra |
| A871 OA | |
| Main belt | |
| Orbital characteristics[2] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 113.62 yr (41501 d) |
| Aphelion | 3.0407 AU (454.88 Gm) |
| Perihelion | 2.31581 AU (346.440 Gm) |
| 2.67825 AU (400.660 Gm) | |
| Eccentricity | 0.13533 |
| 4.38 yr (1600.9 d) | |
Average orbital speed | 18.12 km/s |
| 197.019° | |
| 0° 13m 29.525s / day | |
| Inclination | 4.9367° |
| 164.222° | |
| 352.208° | |
| Earth MOID | 1.3244 AU (198.13 Gm) |
| Jupiter MOID | 1.94976 AU (291.680 Gm) |
| TJupiter | 3.359 |
| Physical characteristics | |
| 94.178±0.954 km[2] 99.798 km[3] 100±14 km[4] | |
| Mass | (1.335 ± 0.597/0.264)×1018 kg[5] |
Mean density | 3.051 ± 1.365/0.603 g/cm3[5] |
Equatorial surface gravity | 0.0402 m/s² |
Equatorial escape velocity | 0.0615 km/s |
| 10.7431 h (0.44763 d)[2] 10.758 h[6] | |
| 0.089±0.014[2] 0.0868 ± 0.0252[3] | |
| Temperature | ~170 K |
| T (Tholen)[3] | |
| 8.51,[2] 8.275[3] | |
This object is classified as a rare T-type asteroid, with parts of the spectrum displaying properties similar to the mineral troilite and to carbonaceous chondrite.[7] The shape of the spectrum also appears similar to fine grain from the Ornans meteorite, which landed in France in 1868.[8] The light curve for this asteroid displays a period of 10.758 ± 0.004 hours with a brightness variation of 0.25 ± 0.01 in magnitude.[6]
In 2001, 114 Kassandra was observed by radar from the Arecibo Observatory. The return signal matched an effective diameter of 100 ± 14 km. This is consistent with the asteroid dimensions computed through other means.[4]
In popular media
editThe 2009 miniseries Meteor featured 114 Kassandra being sent on a collision course with Earth due to a comet impact and the effort by scientists to stop it.
References
edit- ^ 'Cassandra' in Noah Webster (1884) A Practical Dictionary of the English Language
- ^ a b c d e Yeomans, Donald K., "114 Kassandra", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 12 May 2016.
- ^ a b c d Pravec, P.; et al. (May 2012), "Absolute Magnitudes of Asteroids and a Revision of Asteroid Albedo Estimates from WISE Thermal Observations", Asteroids, Comets, Meteors 2012, Proceedings of the conference held May 16–20, 2012 in Niigata, Japan, vol. 1667, no. 1667, p. 6089, Bibcode:2012LPICo1667.6089P.
- ^ a b Magri, Christopher; et al. (January 2007), "A radar survey of main-belt asteroids: Arecibo observations of 55 objects during 1999–2003", Icarus, 186 (1): 126–151, Bibcode:2007Icar..186..126M, doi:10.1016/j.icarus.2006.08.018
- ^ a b Fienga, A.; Avdellidou, C.; Hanuš, J. (February 2020). "Asteroid masses obtained with INPOP planetary ephemerides". Monthly Notices of the Royal Astronomical Society. 492 (1): 589–602. doi:10.1093/mnras/stz3407.
- ^ a b Hutton, R. G.; Blain, A. (December 1988), "V+B Photoelectric Photometry of Asteroid 114 Kassandra", The Minor Planet Bulletin, 15: 39, Bibcode:1988MPBu...15...39H.
- ^ Dotto, E.; et al. (October 2002), "ISO observations of low and moderate albedo asteroids. PHT-P and PHT-S results" (PDF), Astronomy and Astrophysics, 393: 1065–1072, Bibcode:2002A&A...393.1065D, doi:10.1051/0004-6361:20021190.
- ^ Hamilton, Victoria E. (March 2010), "Thermal infrared (vibrational) spectroscopy of Mg-Fe olivines: A review and applications to determining the composition of planetary surfaces", Chemie der Erde - Geochemistry, vol. 70, no. 1, pp. 7–33, Bibcode:2010ChEG...70....7H, doi:10.1016/j.chemer.2009.12.005.
External links
edit- 114 Kassandra at AstDyS-2, Asteroids—Dynamic Site
- 114 Kassandra at the JPL Small-Body Database
