Jump to content

P/2015 PD229 (Cameron–ISON)

From Wikipedia, the free encyclopedia
P/2015 PD229 (Cameron–ISON)
Discovery[1]
Discovered byDavid A. Cameron
ISON
Discovery siteCerro Tololo, Chile
Siding Spring, Australia
Discovery date27 May 2015
15 August 2015
Designations
K15PM9D[1]
Orbital characteristics[3]
Epoch21 October 2015 (JD 2457316.5)
Observation arc540 days (1.5 years)
Number of
observations
110
Aphelion9.522 AU
Perihelion4.832 AU
Semi-major axis7.177 AU
Eccentricity0.32674
Orbital period19.23 years
Inclination2.027°
342.77°
Argument of
periapsis
352.37°
Last perihelion14 August 2015
Next perihelion11 November 2034[2]
TJupiter2.944
Earth MOID3.821 AU
Jupiter MOID0.106 AU
Physical characteristics[4]
Dimensions13 mi (21 km)
Comet total
magnitude
(M1)
7.1
Comet nuclear
magnitude (M2)
12.6

P/2015 PD229 (Cameron–ISON) is a periodic comet that was initially thought to be an active centaur upon discovery. It orbits the Sun between Jupiter and Saturn once every 19.2 years, and has appeared to have made several close encounters with the giant planets from 1889 to 1949.[5] The orbital period and low inclination mean this comet is classed as a Jupiter family comet.[4] The comet appears to be about 13 miles across, which is bigger than most Jupiter family comets.[4]

References

[edit]
  1. ^ a b G. V. Williams (18 August 2015). "MPEC 2015-Q17: 2015 PD229". www.minorplanetcenter.net. Minor Planet Center. Retrieved 1 January 2025.
  2. ^ S. Yoshida. "P/2015 PD229 (Cameron–ISON)". www.aerith.net. Retrieved 2 January 2025.
  3. ^ "P/2015 PD229 (Cameron–ISON) – JPL Small-Body Database Lookup". ssd.jpl.nasa.gov. Jet Propulsion Laboratory. Retrieved 1 January 2025.
  4. ^ a b c L. Sierra (4 March 2016). "Rochester scientist discovers new comet". pas.rochester.edu. University of Rochester. Retrieved 1 January 2025.
  5. ^ E. E. Mamajek. "Comet P/2015 PD229 (ISON-Cameron)". pas.rochester.edu. University of Rochester. Retrieved 1 January 2025.
[edit]