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70P/Kojima

From Wikipedia, the free encyclopedia
Periodic comet
For the other comet discovered by Nobuhisa Kojima, seeC/1972 U1 (Kojima).
70P/Kojima
70P/Kojima as imaged from theZwicky Transient Facility on 1 March 2022
Discovery[1]
Discovered byNobuhisa Kojima
Discovery siteIshiki, Aichi, Japan
Discovery date27 December 1970
Designations
P/1970 Y1
P/1977 X1
  • 1970 XII, 1978 X
  • 1986 VII, 1994 VI
  • 1970r, 1977r, 1985o
  • 1992z
Orbital characteristics[3][4]
Epoch13 September 2023 (JD 2460200.5)
Observation arc51.47 years
Number of
observations
2,122
Aphelion5.347 AU
Perihelion2.007 AU
Semi-major axis3.677 AU
Eccentricity0.45411
Orbital period7.050 years
Inclination6.599°
119.25°
Argument of
periapsis
1.780°
Mean anomaly94.901°
Last perihelion3 November 2021
Next perihelion21 November 2028[2]
TJupiter2.904
EarthMOID1.022 AU
JupiterMOID0.140 AU
Physical characteristics[3][5]
Mean diameter
3.64 km (2.26 mi)
22±5 hours
Comet total
magnitude
(M1)
12.2
Comet nuclear
magnitude (M2)
15.0

70P/Kojima is aperiodiccomet in theSolar System with a current orbital period of 7.05 years.[4][6]

Observational history

[edit]

It was discovered at Ishiki, Aichi, Japan byNobuhisa Kojima, who estimated its brightness at magnitude 14.[1] Its parabolic orbit was calculated byKiichirō Furukawa to have a perihelion date of 1 November 1970.[7] This was revised on the basis of further observations to an elliptical orbit with a perihelion of 7 October and an orbital period of 6.16.

Hiroki Kosai and Furukawa relocated the comet on 9 December 1977 at its next predicted apparition with the 105 cm (41 in) Schmidt telescope at theKiso Station of the Tokyo Astronomical Observatory, estimating its brightness at magnitude 16.[8] It was subsequently observed in 1985/1986[9] and 1992/1994[10] bySpacewatch with magnitudes of 20 and 22.1, respectively.[9][10] The comet then passed close to Jupiter, which reduced the perihelion distance from 2.4 AU to 1.97 AU, increased the eccentricity from 0.39 to 0.46 and reduced the orbital period from 7.85 to 6.99 years.

Physical characteristics

[edit]

Its nucleus is estimated to have aneffective radius of1.82±0.09 kilometers and its rotational period is estimated to be22±5 hours.[5]

See also

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References

[edit]
  1. ^abM. Huruhata; N. Kojima; K. Tomita; T. Seki (4 January 1971). B. G. Marsden (ed.)."Comet Kojima (1970r)".IAU Circular.2298.Bibcode:1971IAUC.2298....1H.
  2. ^"Horizons Batch for 70P/Kojima (90000714) on 2028-Nov-21" (Perihelion occurs when rdot flips from negative to positive).JPL Horizons.Archived from the original on 2023-07-07. Retrieved6 July 2023. (JPL#60 Soln.date: 2023-Apr-05)
  3. ^ab"70P/Kojima – JPL Small-Body Database Lookup".ssd.jpl.nasa.gov.Jet Propulsion Laboratory. Retrieved22 April 2025.
  4. ^ab"70P/Kojima Orbit".Minor Planet Center. Retrieved22 April 2025.
  5. ^abP. L. Lamy; I. Toth; H. A. Weaver; M. F. A'Hearn; L. Jorda (2011)."Properties of the nuclei and comae of 10 ecliptic comets from Hubble Space Telescope multi-orbit observations★: HST observations of 10 ecliptic comets".Monthly Notices of the Royal Astronomical Society.412 (3):1573–1590.doi:10.1111/j.1365-2966.2010.17934.x.
  6. ^G. W. Kronk."70P/Kojima".Cometography.com. Retrieved22 February 2015.
  7. ^M. Huruhata; K. Furukawa (6 January 1971). B. G. Marsden (ed.)."Comet Kojima (1970r)".IAU Circular.2299.Bibcode:1971IAUC.2299....1H.
  8. ^K. Furukawa; Y. Kozai; H. Kosai; H. Kinoshita; C. T. Kowal (13 December 1977). B. G. Marsden (ed.)."Periodic Comet Kojima (1977r)".IAU Circular.3151.Bibcode:1977IAUC.3151....1H.
  9. ^abT. Gehrels; J. V. Scotti (25 October 1985). B. G. Marsden (ed.)."Periodic Comet Kojima (1985o)".IAU Circular.4126.Bibcode:1985IAUC.4126....1G.
  10. ^abJ. V. Scotti (4 December 1992). D. W. Green (ed.)."Periodic Comet Kojima (1992z)".IAU Circular.5667.Bibcode:1992IAUC.5667....1S.

External links

[edit]


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