311P/PanSTARRS

311P/PanSTARRS
P/2013 P5 (PanSTARRS) as captured by the Hubble Space Telescope
Discovery [1]
Discovered byBryce T. Bolin using Pan-STARRS
Discovery date27 August 2013
Designations
P/2013 P5 (PANSTARRS)
Orbital characteristics[2]
Epoch 16 November 2013 (JD 2456612.5)
Uncertainty parameter 0
Observation arc13.13 yr (4,797 d)
Earliest precovery date17 January 2005
Aphelion2.4411 AU
Perihelion1.9362 AU
2.1885 AU
Eccentricity0.11530
3.24 yr (1182.575d)
0.3044°/d
314.07°
Inclination4.9685°
279.29°
2024-Jan-01[3]
144.26°
Physical characteristics
~480 meters (1,570 ft)[4]
Mean density
3.30 ± 0.20 g/cm3[4]
~0.240 m/s

311P/PanSTARRS also known as P/2013 P5 (PanSTARRS) is an active asteroid (object with asteroid-like orbit but with comet-like visual characteristics) discovered by Bryce T. Bolin using the Pan-STARRS telescope on 27 August 2013.[1][5] Observations made by the Hubble Space Telescope revealed that it had six comet-like tails.[6] 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.[4] This is similar to 331P/Gibbs, which was found to be a quickly-spinning rubble pile as well.

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,[7] radiation pressure from the Sun then stretched the dust into streams.[6]

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

  1. ^ a b Cite error: The named reference CBET-2013-3639 was invoked but never defined (see the help page).
  2. ^ Cite error: The named reference jpldata was invoked but never defined (see the help page).
  3. ^ Cite error: The named reference Horizons2024 was invoked but never defined (see the help page).
  4. ^ a b c Cite error: The named reference Jewitt2013 was invoked but never defined (see the help page).
  5. ^ "When is a comet not a comet?". Spacetelescope. 7 November 2013.
  6. ^ a b "NASA's Hubble Sees Asteroid Spouting Six Comet-Like Tails". Hubblesite. 7 November 2013.
  7. ^ "She calculated that dust-ejection events occurred on April 15, July 18, July 24, Aug. 8, Aug. 26 and Sept. 4"