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40P/Väisälä

From Wikipedia, the free encyclopedia
Periodic comet
For other comets also discovered by Yrjö Väisälä, seeComet Väisälä.

40P/Väisälä
Comet Väisälä 1 imaged from the Vega Observatory on March 18, 2004.
Discovery[1]
Discovered byYrjö Väisälä
Discovery siteUniversity of Turku, Finland
Discovery dateFebruary 8, 1939
Designations
P/1939 CB
P/1949 Y1
  • Väisälä 1
  • 1939 IV, 1949 V
  • 1960 IV, 1971 VII
  • 1982 V, 1993 VIII
Orbital characteristics[4]
EpochMay 5, 2025 (JD 2460800.5)
Observation arc86.16 years
Earliestprecovery dateJanuary 18, 1939
Number of
observations
1,243
Aphelion8.079 AU
Perihelion1.824 AU
Semi-major axis4.951 AU
Eccentricity0.63169
Orbital period11.018 years
Inclination11.639°
128.90°
Argument of
periapsis
52.029°
Mean anomaly342.92°
Last perihelionNovember 15, 2014[2]
Next perihelionNovember 11-12, 2025[3]
TJupiter2.535
EarthMOID0.823 AU
JupiterMOID0.077 AU
Physical characteristics[5]
Mean diameter
4.2 km (2.6 mi)
Comet total
magnitude
(M1)
11.6
Comet nuclear
magnitude (M2)
14.8

40P/Väisälä is aperiodic comet that was discovered on February 8, 1939. Its orbit was determined on April 26, 1939.[2] In 1994, the diameter of itsnucleus was found to be 4.2 km (2.6 mi), similar in size to that ofComet Encke.[5] It was last observed in March 2025 and will come to perihelion on November 11-12, 2025.

Discovery

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Comet Väisälä was discovered accidentally on photographs exposed forminor planets. Originally, it was given theasteroid designation 1939 CB.[1][5] However, additional findings revealed that the object was of cometary nature. Thevisual magnitude of Väisälä at the time of its discovery was 15. The orbital characteristics of the new comet at the time of its discovery were "a period of about 10 years, aperihelion date of April 26, 1939, and a perihelion distance of 1.75 AU (262 million km)."[1]

Orbit

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Orbit of 40P/Väisälä, which crosses the orbit ofJupiter and is frequently gravitationally perturbed

The orbit of Comet Väisälä resembles that of many centaurs, and is therefore unstable[6] over thousands of years due to gravitational interactions with the gas giant Jupiter. One such close approach, 0.41 AU (61 million km) on December 31, 1961, increased its perihelion distance from 1.74 AU to 1.87 AU and increased its orbital period from 10.46 to 11.28 years. On September 21, 1973, an approach of Jupiter 1 AU away decreased perihelion distance from 1.87 AU to 1.80 AU decreased orbital period from 11.28 to 10.88 years.[1] Väisälä will make one more close approach in the 21st century,[5] but it will have a minimal effect.[1] However, in the year 2127, the comet will make a close approach of only 0.096 AU from Jupiter, and reduce perihelion to 1.4 AU.[5]

References

[edit]
  1. ^abcdeG. W. Kronk."40P/Väisälä 1".Cometography.com. RetrievedNovember 3, 2013.
  2. ^abS. Yoshida (2006)."40P/Väisälä 1".www.aerith.net. RetrievedNovember 3, 2013.
  3. ^"Horizons Batch for 40P/Vaisala 1 (90000479) on 2025-Nov-12 ≈00:49 UT" (Perihelion occurs when rdot flips from negative to positive).JPL Horizons.Archived from the original on September 28, 2025. RetrievedSeptember 28, 2025. (JPL#45 Soln.date: 2025-Apr-11)
  4. ^"40P/Väisälä Orbit".Minor Planet Center. RetrievedOctober 29, 2014.
  5. ^abcde"40P/Väisälä 1".ssd.jpl.nasa.gov.Jet Propulsion Laboratory. RetrievedApril 24, 2025.
  6. ^J. Horner; N. W. Evans; M. E. Bailey (2004)."Simulations of the Population of Centaurs I: The Bulk Statistics".Monthly Notices of the Royal Astronomical Society.354 (3):798–810.arXiv:astro-ph/0407400.Bibcode:2004MNRAS.354..798H.doi:10.1111/j.1365-2966.2004.08240.x.S2CID 16002759.

External links

[edit]


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