[meteorite-list] 16 Psyche data for epoch 2000
From: Bernd Pauli HD <bernd.pauli_at_meteoritecentral.com>
Date: Thu Apr 22 09:43:28 2004 Message-ID: <3B3F71CD.AC1FC6E_at_lehrer1.rz.uni-karlsruhe.de> Hello All, Below is more recent data for asteroid 16 Psyche. For some unknown reason, the entry for 16 Psyche is missing in the Almanac for 2001, so I chose last year's data. These parameters would place 16 Psyche at the edge of main belt IIIa where it borders on the Koronis zone. ... and another passage from Cunningham (p.52); Employing polarimetry, Dollfus et al. (1979) concluded that M-type asteroids have a surface texture that is a powder of small metallic fragments with grain sizes between 20 and 50 microns. It was later shown by Feierberg et al. (1983) that this powder is mixed with a significant amount of fine silicate dust, thus ruling out a pure metallic surface. Best wishes, Bernd Astronomical Almanac for the year 2000, Section G10: Elements for Epoch 2000, September, Ecliptic and Equinox J2000.0: Magnitude Parameters: H = 5.90 / G = 0.20 Opposition Date: Dec 06 / Magnitude 9.4 Diameter: 250 km Inclination: i = 3.092° Long. of ascending node: 150.434° Argument of perihelion: w = 229.032° Mean distance: a = 2.9234 (= the semimajor axis of an elliptic orbit) Daily motion: n = 0.19718° Eccentricity: e = 0.1391 Mean anomaly*: M = 26.095° * M = in undisturbed elliptic motion, the product of the mean motion of an orbiting body and the interval of time since the body passed pericenter (= the point in an orbit that is nearest to the center of force). Explanations from CUNNINGHAM C.J. (1988) Introduction To Asteroids (Willmann-Bell Inc., p. 40): H = absolute magnitude G = slope parameter i = angle between the plane of the asteroid's orbit and that of the Earth => ecliptic Long. of ascending node = the angular distance measured eastward in the plane of the Earth's orbit, from the vernal equinox to the point where the asteroid crosses the ecliptic from south to north. w = defines how the major axis of the ellipse is oriented in its orbital plane by giving the angle between the ascending node and the perihelion point, measured in the direction of motion. e = c/a, where c is the distance from the sun to the center of the ellipse and a is the length of the semi-major axis. Received on Sun 01 Jul 2001 02:54:05 PM PDT |
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