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311p/panstarrs

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311p/panstarrs

311P/PANSTARRS
P/2013 P5
P/2013 P5 (PANSTARRS) as captured by the Hubble Space Telescope
Discovery
Discovered by Pan-STARRS
Discovery date 27 August 2013
Designations
asteroid
Main-belt comet
Orbital characteristics[1]
Epoch 2013-Sep-07
Aphelion 2.441 AU
Perihelion 1.936 AU
2.189 AU
Eccentricity 0.1152
3.24 yr (1182.638d)
Average orbital speed
0.3044°/d
292.8°
Inclination 4.969°
279.3°
144.2°
Physical characteristics
Dimensions ~480 meters (1,570 ft) [2]
Mean density
3300±200 kg m3 [3]
~0.240 meters (9.4 in) per second

311P/PANSTARRS also known as P/2013 P5 (PANSTARRS) is an asteroid (or main-belt comet) discovered by the Pan-STARRS telescope on 27 August 2013.[4] Observations made by the Hubble Space Telescope revealed that it had six comet-like tails.[5] The tails are suspected to be streams of material ejected by the asteroid as a result of a rubble pile asteroid spinning fast enough to remove material from it.[2]

Three-dimensional models constructed by Jessica Agarwal of the Max Planck Institute for Solar System Research in Lindau, Germany, showed that the tails could have formed by a series of periodic impulsive dust-ejection events,[6] radiation pressure from the sun then stretched the dust into streams.[5]

Precovery images from the Sloan Digital Sky Survey from 2005 were found, showing negligible cometary activity in 2005.

Characteristics

The asteroid has a radius of about 240 meters (790 ft).[2] The first images taken by Pan-STARRS revealed that the object had an unusual appearance: asteroids generally appear as small points of light, but P/2013 P5 was identified as a fuzzy-looking object by astronomers.[7] The multiple tails were observed by the Hubble Space Telescope on 10 September 2013, Hubble later returned to the asteroid on 23 September, its appearance had totally changed. It looked as if the entire structure had swung around.[8] The Hubble Space Telescope continued to track the object through 11 February 2014.[9] The comet-like appearance has resulted in the asteroid being named as a comet. The object has a low orbital inclination and always stays outside the orbit of Mars.[1]

See also

References

  1. ^ a b
  2. ^ a b c
  3. ^
  4. ^
  5. ^ a b
  6. ^ "She calculated that dust-ejection events occurred on April 15, July 18, July 24, Aug. 8, Aug. 26 and Sept. 4"
  7. ^
  8. ^
  9. ^

External links

  • The Extraordinary Multi-Tailed Main-Belt Comet P/2013 P5 (arXiv:1311.1483 : 6 Nov 2013)
  • The Multi-Tailed Main-Belt Comet P/2013 P5 (Remanzacco Observatory : 8 Nov 2013)
  • Confused Asteroid Sprouts Tails… Six of Them! (Phil Plait : 8 Nov 2013)
  • Orbit diagram from JPL Small-Body Database
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