(8597) Sandvicensis

from Wikipedia, the free encyclopedia
Asteroid
(8597) Sandvicensis
Properties of the orbit ( animation )
Epoch:  4th November 2013 ( JD 2,456,600.5)
Orbit type Middle main belt asteroid
Asteroid family Eunomia family
Major semi-axis 2.6863  AU
eccentricity 0.1528
Perihelion - aphelion 2.2757 AU - 3.0968 AU
Inclination of the orbit plane 12.6308 °
Length of the ascending node 3.3736 °
Argument of the periapsis 261.6796 °
Sidereal period 4.40 a
Mean orbital velocity 18.17 km / s
Physical Properties
Absolute brightness 13.0 likes
history
Explorer Cornelis Johannes van Houten ,
Ingrid van Houten-Groeneveld ,
Tom Gehrels
Date of discovery 29th September 1973
Another name 2045 T-2 , 1976 GN 1 , 1980 BF 2 , 1986 RJ 5
Source: Unless otherwise stated, the data comes from JPL Small-Body Database Browser . The affiliation to an asteroid family is automatically determined from the AstDyS-2 database . Please also note the note on asteroid items.

(8597) Sandvicensis is an asteroid of the central main belt that was discovered on September 29, 1973 by the Dutch astronomer couple Cornelis Johannes van Houten and Ingrid van Houten-Groeneveld . The discovery was made during the 2nd Trojan survey, during which Tom Gehrels surveyed field plates recorded with the 120 cm Oschin Schmidt telescope of the Palomar observatory at the University of Leiden , 13 years after the start of the Palomar-Leiden- Surveys .

The asteroid belongs to the Eunomia family, a group named after (15) Eunomia , to which probably five percent of the asteroids in the main belt belong. The timeless (not osculating ) orbital elements of (8597) Sandvicensis are almost identical to those of the smaller, if one of the absolute brightness emanating from 16.0 versus 13.0, asteroid (298170) 2002 TS 145 .

(8597) Sandvicensis is named after the sandwich tern , whose scientific name is Sterna sandvicensis . At the time the asteroid was named on February 2, 1999, the sandwich tern was on the Dutch Red List of Endangered Species . The first letters of the asteroids (8585) to (8600) form the phrase Per aspera ad astra .

Web links

Individual evidence

  1. The family status of the asteroids in the AstDyS-2 database (English, HTML; 51.4 MB)
  2. ^ Lutz D. Schmadel : Dictionary of Minor Planet Names . Springer, Heidelberg 2012, 6th edition, page 645 (English)