(5197) Rottmann

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Asteroid
(5197) Rottmann
Properties of the orbit ( animation )
Epoch:  December 9, 2014 ( JD 2,457,000.5)
Orbit type Main belt asteroid
Asteroid family Eos family
Major semi-axis 3.0075  AU
eccentricity 0.1172
Perihelion - aphelion 2.6550 AU - 3.3600 AU
Inclination of the orbit plane 11.1175 °
Length of the ascending node 27.8370 °
Argument of the periapsis 310.6925 °
Sidereal period 5.22 a
Mean orbital velocity 17.17 km / s
Physical Properties
Absolute brightness 12.2 mag
history
Explorer Cornelis Johannes van Houten ,
Ingrid van Houten-Groeneveld ,
Tom Gehrels
Date of discovery 29th September 1973
Another name 4265 T-2 , 1989 UB 1
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.

(5197) Rottmann is an asteroid of the 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 Second Trojan Survey of 1973, during which Tom Gehrels scanned field plates recorded at the University of Leiden with the 120 cm Oschin Schmidt telescope of the Palomar Observatory .

The asteroid belongs to the Eos family, a group of asteroids, which typically have large semiaxes from 2.95 to 3.1 AU , bounded inward by the Kirkwood gap of the 7: 3 resonance with Jupiter , and orbital inclinations between 8 ° and 12 °. The group is named after the asteroid (221) Eos . The family is believed to have emerged from a collision more than a billion years ago.

(5197) Rottmann was named after the German landscape painter Carl Rottmann (1797–1850), who is known for mythical - heroic landscape painting and whose main work is the Greece cycle.

See also

Web links

Individual evidence

  1. The family membership of (5197) Rottmann in the AstDyS-2 database (English)
  2. David Vokrouhlický , Miroslav Brož , Alessandro Morbidelli , William Bottke , David Nesvorný , Daniel Lazzaro, Andy Rivkin: Yarkovsky footprints in the Eos family ( PDF , English)