114 Kassandra

Kassandra (minor planet designation: 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. The asteroid is featured in the 2009 film Meteor, in which it is split in two by a comet, and set on a collision course with Earth.

114 Kassandra
3D convex shape model of 114 Kassandra
Discovery
Discovered byChristian Heinrich Friedrich Peters
Discovery date23 July 1871
Designations
MPC designation
(114) Kassandra
Pronunciation/kəˈsændrə/
Named after
Cassandra
Alternative designations
A871 OA
Minor planet category
Main belt
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc113.62 yr (41501 d)
Aphelion3.0407 AU (454.88 Gm)
Perihelion2.31581 AU (346.440 Gm)
Semi-major axis
2.67825 AU (400.660 Gm)
Eccentricity0.13533
Orbital period (sidereal)
4.38 yr (1600.9 d)
Average orbital speed
18.12 km/s
Mean anomaly
197.019°
Mean motion
0° 13m 29.525s / day
Inclination4.9367°
Longitude of ascending node
164.222°
352.208°
Earth MOID1.3244 AU (198.13 Gm)
Jupiter MOID1.94976 AU (291.680 Gm)
TJupiter3.359
Physical characteristics
Mean diameter
94.178±0.954 km
99.798 km
100±14 km
Mass(1.335 ± 0.597/0.264)×1018 kg
Mean density
3.051 ± 1.365/0.603 g/cm3
Equatorial surface gravity
0.0402 m/s²
Equatorial escape velocity
0.0615 km/s
Synodic rotation period
10.7431 h (0.44763 d)
10.758 h
0.089±0.014
0.0868 ± 0.0252
Temperature~170 K
T (Tholen)
8.51, 8.275

    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. The shape of the spectrum also appears similar to fine grain from the Ornans meteorite, which landed in France in 1868. 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.

    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.

    This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.