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129 Antigone - Wikipedia, the free encyclopedia
129 Antigone is a large main belt asteroid. Radar observations indicate that it is composed of almost pure nickel-iron. It and other similar asteroids probably originate from the core of a shattered V...
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129 Antigone is a large main belt asteroid. It is composed of almost pure nickel-iron. It and other similar asteroids probably originate from the core of a...
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Photometric observations of 41 Daphne and 129 Antigone were made during the period April-June 1976. The synodic periods of rotation are 0.249492 and...
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(129) Antigone Epoch 2000 Feb. 26.0 TT = JDT 2451600.5 (M-P) Sumzina M 322.60231 (2000.0) P Q n 0.20299318 Peri.
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(129) Antigone Epoch 2001 Apr. 1.0 TT = JDT 2452000.5 Williams M 43.85461 (2000.0) P Q n 0.20303257 Peri. 108.55053 -0.40745424 +0.90150603 a 2.8669860 Node 136.47209 -0.89722706 -0.36541829 e 0.2140466 Incl.
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129 Antigone is a big main belt asteroid. Radar observations indicate that it is made of almost pure nickel-iron. 128 Nemesis | 129 Antigone | 130 Elektra...
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127 Johanna | 128 Nemesis | 129 Antigone...
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(129) Antigone Epoch 2005 Jan. 30.0 TT = JDT 2453400.5 Williams M 328.62470 (2000.0) P Q n 0.20286031 Peri.
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ASTROMETRIC UPDATE: OCCULTATION BY (129) ANTIGONE - 2005 NOV 16 On 2005 Nov 16 UT, the 144 km diameter asteroid (129) Antigone will occult a 11.1 mag star in the constellation Sagittarius for observers along a path across northern Australia from Carnarvon in Western Australia to Tennant Creek in Northern Territory.
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FINDER CHARTS: OCCULTATION BY (129) ANTIGONE - TYC 0792-00329 2004 JAN 03, 15:11 - 2004 JAN 03, 15:26 UT...
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