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4769 Castalia

4769 Castalia
4769Castalia-P36165BC-crop.gif
Arecibo radar image showing Castalia as a contact binary.
Discovery
Discovered by E. F. Helin
Palomar Observatory (675)
Discovery date 9 August 1989
Designations
MPC designation 4769 Castalia (1989 PB)
Named after
Castalia
Apollo NEO,
PHA
Venus-crosser asteroid,
Mars-crosser asteroid
Orbital characteristics
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 0
Observation arc 9467 days (25.92 yr)
Aphelion 1.5770 AU (235.92 Gm) (Q)
Perihelion 0.54957 AU (82.215 Gm) (q)
1.0633 AU (159.07 Gm) (a)
Eccentricity 0.48313 (e)
1.10 yr (400.46 d)
327.23° (M)
0° 53m 56.256s / day (n)
Inclination 8.8863° (i)
325.59° (Ω)
121.35° (ω)
Known satellites contact binary
Earth MOID 0.0199597 AU (2.98593 Gm)
Jupiter MOID 3.67272 AU (549.431 Gm)
Jupiter Tisserand parameter 5.676
Physical characteristics
Dimensions 1.4 km
1.8×0.8 km
Mean radius
0.7 km
Mass 5.0×1011 kg (?)
Mean density
2.1 g/cm³ (?)
4.095 h (0.1706 d)
Sidereal rotation period
4.095 h
Temperature 216–366 K
S (?)
16.9

The asteroid 4769 Castalia (/kəˈstliə/ kə-STAY-lee-ə; previously known by the provisional designation 1989 PB) was the first asteroid to be modeled by radar imaging. It is an Apollo, Mars- and Venus-crosser asteroid. It was discovered on August 9, 1989, by Eleanor F. Helin (Caltech) on photographic plates taken at Palomar Observatory. It is named after Castalia, a nymph in Greek mythology.

On 25 August 1989 Castalia passed 0.0269378 AU (4,029,840 km; 2,504,020 mi) (within eleven lunar distances) of Earth, allowing it to be observed with radar from the Arecibo Observatory by Scott Hudson (Washington State University) and Steven J. Ostro (JPL). The data allowed Hudson et al. to produce a three-dimensional model of the object. During the 1989 passage Castalia peaked at an apparent magnitude of 12.


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