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126P/IRAS is a Jupiter-family comet with an orbital period of 13.4 years. It was discovered in images taken by the Infrared Astronomical Satellite (IRAS) on 28 July 1983 by J. Davies. The discovery was confirmed with images taken with the 1.2-m Schmidt telescope at Palomar Observatory.

Key facts

Comet.M2
14.9
Comet.name
126P/IRAS
Comet.image
126P 2023-07-27 image ZTF-sso-555-zr-size-11arcmin.png
Comet.caption
Comet 126P/IRAS photographed from the Zwicky Transient Facility on 27 July 2023
Comet.discoverer
Infrared Astronomical Satellite
Comet.discovery_date
26 July 1983
Comet.mpc_name
P/1983 M1, P/1996 P1
Comet.designations
1983 XIV, 1983j
Comet.epoch
27 May 2021 (JD 2459361.5)
Comet.observation_arc
27.52 years
Comet.obs
1,717
Comet.perihelion
1.713 AU
Comet.aphelion
9.573 AU
Comet.semimajor
5.640 AU
Comet.eccentricity
0.69628
Comet.period
13.395 years
Comet.inclination
45.869°
Comet.asc_node
357.86°

via Wikipedia infobox

~2 min read

Encyclopedic overview

5 sections
Contents
  • Observational history
  • Physical characteristics
  • Possible meteor shower
  • References
  • External links

126P/IRAS is a Jupiter-family comet with an orbital period of 13.4 years. It was discovered in images taken by the Infrared Astronomical Satellite (IRAS) on 28 July 1983 by J. Davies. The discovery was confirmed with images taken with the 1.2-m Schmidt telescope at Palomar Observatory.

== Observational history == Upon discovery the comet had an apparent magnitude of 15 and appeared stellar in appearance. The comet brightened and in mid September 1983 reached an apparent magnitude of 11 while a tail 3.5 arcminutes long was observed. Brian G. Marsden computed its orbit and found it is a short period comet with an orbital period of 13.32 years. The comet was observed again during its next apparition in 1996, when it brightened up to magnitude of about 11 in September 1996 and faded to about 12 in October. The comet was observed during its 2010 and 2023 apparitions.

Excerpted from Wikipedia’s “126P/IRAS” article, available under the CC BY-SA 4.0 licence.

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