The nucleus of Hale-Bopp is estimated to be about 30 to 40 km across - Comet Halley's nucleus was estimated at 8 x 8 x 16 km. The nucleus is exhibiting sudden brief eruptions and a complex mottled surface. Its absolute magnitude of -1 makes it one of the brightest comets to reach the inner solar system in history. Closest approach to Earth will occurred on 22 March 1997 at a distance of 1.3 A.U. It made for a spectacular view in the March morning sky, and will be in the evening skies from mid-March to early May. Closest approach to the Sun was on 31 March at a distance of .91 A.U. The comet is estimated to have last passed by the Sun about 4200 years ago.
Hale-Bopp was visible low in the northern hemisphere pre-dawn sky in February to the ENE just below the constellation Cygnus. By the end of March the comet moved from Cygnus to Lacerta to Andromeda in the NE pre-dawn sky. The comet will be disappearing from the pre-dawn sky at the beginning of April. Since mid-March, however, the comet has also been visible in the early evening sky to the NW to WNW, at the bottom of Perseus. The comet will become higher in the sky through mid-April, and then move down towards the horizon by early May. The comet is currently one of the brightest objects in the sky and the tail is spectacular.
Information on Hale-Bopp
Perihelion distance: 0.9141 AUPerihelion date: 01 April 1997 UT 03:19 (31 March 22:19 EST)
Closest approach to Earth: 1.3 AU
Date of closest approach to Earth: 22 March 1997
Next Perihelion: ~2380 years
Previous Perihelion: ~4200 years ago
Orbital inclination: 89.43 deg.
Orbital eccentricity: 0.9951
Argument of perihelion: 130.59 deg.
Longitude of ascending node: 282.47 deg.
Heliocentric coordinates of Hale-Bopp - for any given dates
Results of IUE and Hubble observations of Hale-Bopp - 27 March 1997
NASA plans to observe Hale-Bopp - 13 March 1997
No comments:
Post a Comment