(8585) Purpurea

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Asteroid
(8585) Purpurea
Properties of the orbit ( animation )
Epoch:  March 23, 2018 ( JD 2,458,200.5)
Orbit type Main outer belt asteroid
Major semi-axis 3.2179  AU
eccentricity 0.1677
Perihelion - aphelion 2.6784 AU - 3.7574 AU
Inclination of the orbit plane 9.5236 °
Length of the ascending node 358.3974 °
Argument of the periapsis 232.0510 °
Time of passage of the perihelion December 14, 2015
Sidereal period 5.77 a
Mean orbital velocity 16.63 km / s
Physical Properties
Medium diameter 16.823 (± 0.200) km
Albedo 0.045 (± 0.008)
Absolute brightness 12.4 mag
history
Explorer Cornelis Johannes van Houten ,
Ingrid van Houten-Groeneveld ,
Tom Gehrels
Date of discovery September 24, 1960
Another name 2025 PL , 1992 EQ 21
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.

(8585) Purpurea is an asteroid of the outer main belt , which was discovered on September 24, 1960 by the Dutch astronomer couple Cornelis Johannes van Houten and Ingrid van Houten-Groeneveld . The discovery came about as part of the Palomar-Leiden survey , during which Tom Gehrels examined field plates recorded at the University of Leiden with the 120 cm Oschin Schmidt telescope of the Palomar observatory .

The mean diameter of the asteroid was calculated to be 16.823 (± 0.200) km .

According to the SMASS classification ( Small Main-Belt Asteroid Spectroscopic Survey ), a spectroscopic study by Gianluca Masi , Sergio Foglia and Richard P. Binzel at (8585) Purpurea assumed a dark surface, so it could, roughly speaking, be trade a C asteroid . The albedo was actually later calculated to be 0.045 (± 0.008).

(8585) Purpurea is named after the purple heron , whose scientific name is Ardea purpurea . At the time the asteroid was named on February 2, 1999, the purple heron 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. ^ Gianluca Masi, Sergio Foglia, Richard P. Binzel: Search for Unusual Spectroscopic Candidates Among 40313 minor planets from the 3rd Release of the Sloan Digital Sky Survey Moving Object Catalog . (English)
  2. subdivision of asteroids to S-types, C-types and V-types (English)