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2099 Öpik

Mars-crossing asteroid


Mars-crossing asteroid

FieldValue
minorplanetyes
name2099 Öpik
background#FA8072
discovery_ref
discovered8 November 1977
discovererE. F. Helin
discovery_sitePalomar Obs.
mpc_name(2099) Opik
alt_names1977 VB
named_afterErnst Öpik
(Estonian astronomer)
mp_categoryMars-crosser
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc60.26 yr (22,009 days)
aphelion3.1370 AU
perihelion1.4710 AU
semimajor2.3040 AU
eccentricity0.3616
period3.50 yr (1,277 days)
mean_anomaly148.76°
mean_motion/ day
inclination26.966°
asc_node218.84°
arg_peri159.18°
moid0.4926 AU
dimensions5.12 km (calculated)
km
rotationh
h
albedo
0.057 (assumed)
spectral_typeS (Tholen)
Ch (SMASS)
C (CALL)
B–V = 0.690
U–B = 0.350
abs_magnitude15.1815.22

(Estonian astronomer) km h 0.057 (assumed) Ch (SMASS) C (CALL) B–V = 0.690 U–B = 0.350

2099 Öpik, provisional designation , is a dark and eccentric asteroid and Mars-crosser from the inner regions of the asteroid belt, approximately 5.1 kilometers in diameter.

The asteroid was discovered on 8 November 1977, by American astronomer Eleanor Helin at the Palomar Observatory in California, and named after Estonian astronomer Ernst Öpik.

Orbit and classification

Öpik orbits the Sun in the inner main-belt at a distance of 1.5–3.1 AU once every 3 years and 6 months (1,277 days). Its orbit has an eccentricity of 0.36 and an inclination of 27° with respect to the ecliptic. The first used precovery was taken at the discovering observatory in 1970, extending the asteroid's observation arc by 7 years prior to its discovery.

Physical characteristics

Originally, the asteroid's spectral type was that of a bright S-type asteroid in the Tholen classification. More recently, it has been characterized as a dark Ch-type, a hydrated subtype of the carbonaceous C-type asteroids in the SMASS classification, which is in agreement with its low albedo (below).

Diameter and albedo

According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Öpik measures 5.17 kilometers in diameter and its surface has an albedo of 0.05. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 5.12 kilometers with an absolute magnitude of 15.18.

Rotation period

In 2005, a photometric lightcurve analysis by several astronomers including Pierre Antonini, rendered a rotation period of hours and with a brightness amplitude of 0.21 in magnitude (), superseding the results of an observation from the 1990s that gave a longer period of 9.3 hours ().

Naming

This minor planet was named after Estonian astronomer and astrophysicist, Ernst Öpik (1893–1985), who has influenced many fields of astronomy during his 60-year long career. He is noted for developing the discipline of statistical celestial mechanics and for methods to estimate the lifetimes of planet-crossing asteroids. In the early 1950s, he calculated the impact probability of Mars-crossing asteroids with Mars, and concluded that a search for impact craters on Mars would be a fruitful. Fourteen years later, Martian craters were discovered by Mariner 4. The official was published by the Minor Planet Center on 1 November 1978 (M.P.C. 4548).

References

Info: Wikipedia Source

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