(514107) Ka'epaoka'awela

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Asteroid
(514107) Ka'epaoka'awela
Properties of the orbit ( animation )
Epoch:  March 23, 2018 ( JD 2,458,200.5)
Major semi-axis 5.1375  AU
eccentricity 0.3805
Perihelion - aphelion 3.1824 AU - 7.0925 AU
Inclination of the orbit plane 163.0005 °
Length of the ascending node 307.3802 °
Argument of the periapsis 257.3803 °
Time of passage of the perihelion January 28, 2016
Sidereal period 11.64 a
Physical Properties
Absolute brightness 16.0 mag
history
Explorer Pan-STARRS 1
Date of discovery November 26, 2014
Another name 2015 BZ 509
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.

(514107) Ka'epaoka'awela is an asteroid about three kilometers in size that moves in a retrograde orbit in the solar system. Computer simulations revealed that the asteroid discovered in 2014 may be of extrasolar origin and was captured by the sun's gravity during the formation of the solar system .

Naming

The name is of Hawaiian origin and was explained as follows:

“In the Hawaiian language Ka'epaoka'āwela means the mischievous opposite-moving companion of Jupiter, evoking the image of a retrograde object of unknown origin. He hoa hōkūna'i 'e'epa no Ka'āwela e holo' ēko'a ana ma ka poe lā. "

- A Hua He Inoa, 'Imiloa Astronomy Center of Hawai'i. :

The naming was announced on April 6, 2019.

Possible extrasolar origin

The retrograde orbit around the sun in constant proximity to the prograde orbit of a planet, Jupiter , distinguishes (514107) 2015 BZ 509 from the few other retrograde objects of the solar system that have been discovered so far. On the basis of computer simulations, Fathi Namouni and Helena Morais assume in a specialist article published in 2018 that the asteroid could not have been formed in the solar system, but was probably captured from another planetary system in the early days of the solar system. It would be the first discovered asteroid of extrasolar origin with orbit around the sun.

See also

Web links

Commons : (514107) 2015 BZ 509  - Collection of images

Individual evidence

  1. a b Ghostly drivers in space. In: Spiegel Online . March 30, 2018, accessed May 23, 2018 .
  2. ^ Paul Wiegert, Martin Connors, Christian Veillet: A retrograde co-orbital asteroid of Jupiter . In: Nature . 2017, pp. 687-689. doi : 10.1038 / nature22029 .
  3. Tilmann Althaus: An interstellar asteroid in the solar system. In: Spectrum of Science. May 21, 2018. Retrieved May 23, 2018 .
  4. Minor Planet Circ. 112435 (PDF)
  5. Fathi Namouni, Helena Morais: An interstellar origin for Jupiter's retrograde co-orbital asteroid . In: Monthly Notices of the Royal Astronomical Society: Letters , Volume 477, Issue 1, June 11, 2018, pp. L117 – L121