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1778 Alfvén

From Wikipedia, the free encyclopedia
Carbonaceous Themistian asteroid

1778 Alfvén
Discovery[1]
Discovered byC. J. van Houten
I. van Houten-G.
Tom Gehrels
Discovery sitePalomar Obs.
Discovery date26 September 1960
Designations
(1778) Alfvén
Named after
Hannes Alfvén(physicist)[2]
4506 P-L · 1936 HK
1952 DD1 · 1958 FB
1959 NN
main-belt · Themis[3]
Orbital characteristics[1]
Epoch 31 May 2021 (JD 2459000.5)
Uncertainty parameter 0
Observation arc66.12 yr (24,152 days) (JPL)
113.65 yr (41,511 days) (MPC)[4]
Aphelion3.5505AU
Perihelion2.7420 AU
3.1462 AU
Eccentricity0.1285
5.58yr (2,038 days)
358.82°
0° 10m 35.4s / day
Inclination2.4742°
106.24°
136.41°
Physical characteristics
Dimensions20.51 km(calculated)[3]
20.623±0.240 km[5][6]
4.8050±0.0027 h[7]
4.82±0.05h[8]
0.08(assumed)[3]
0.095±0.007[5][6]
C[3]
11.59±0.15(R)[8] · 11.6[5] · 11.725±0.003(R)[7] 11.8[1][3] · 12.32±0.54[9]

1778 Alfvén, also designated4506 P-L, is a carbonaceous Themistianasteroid from the outer region of theasteroid belt, approximately 20 kilometers in diameter.

It was discovered on 26 September 1960, by astronomersCornelis van Houten,Ingrid van Houten-Groeneveld andTom Gehrels at the U.S.Palomar Observatory, in California.[4] It was later named after Swedish NobelistHannes Alfvén.[2]

Orbit and classification

[edit]

The darkC-type asteroid is a member of theThemis family, a dynamical family of outer-belt asteroids with nearly coplanarecliptical orbits.Alfvén orbits the Sun in theouter main-belt at a distance of 2.7–3.6 AU once every 5 years and 7 months (2,038 days). Its orbit has aneccentricity of 0.13 and aninclination of 2° with respect to theecliptic.[1]

A firstprecovery was taken atLowell Observatory in 1906, extending the body'sobservation arc by 54 years prior to its official discovery observation.[4]

Physical characteristics

[edit]

Rotation period

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In February 2013, two rotationallightcurves ofAlfvén were obtained from analysis at thePalomar Transient Factory in California. The lightcurves gave arotation period of 4.82 and 4.8050 hours with a brightness variation of 0.40 and 0.36magnitude, respectively (U=3-/2).[8][7]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Alfvén measures 20.62 kilometers in diameter and its surface has analbedo of 0.095,[5][6] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.08 and calculates a diameter of 20.51 kilometers with anabsolute magnitude of 11.8.[3]

Survey designation

[edit]

Thesurvey designation "P-L" stands forPalomar–Leiden, named after Palomar Observatory andLeiden Observatory, which collaborated on the fruitfulPalomar–Leiden survey in the 1960s. Gehrels used Palomar'sSamuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped thephotographic plates to Ingrid and Cornelis van Houten at Leiden Observatory whereastrometry was carried out. The trio are credited with the discovery of several thousand minor planets.[10]

Naming

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Thisminor planet was named after Swedish engineer, physicist and Nobel prize winner,Hannes Alfvén (1908–1995).[2] The officialnaming citation was published by theMinor Planet Center on 15 June 1974 (M.P.C. 3643).[11]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1778 Alfven (4506 P-L)" (2020-10-11 last obs.).Jet Propulsion Laboratory. Retrieved21 February 2021.
  2. ^abcSchmadel, Lutz D. (2007). "(1778) Alfvén".Dictionary of Minor Planet Names – (1778) Alfvén.Springer Berlin Heidelberg. p. 142.doi:10.1007/978-3-540-29925-7_1779.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1778) Alfvén". Asteroid Lightcurve Database (LCDB). Retrieved19 December 2016.
  4. ^abc"1778 Alfven (4506 P-L)".Minor Planet Center. Retrieved21 February 2021.
  5. ^abcdMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal.741 (2): 25.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90.
  6. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; et al. (November 2011)."Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68. Retrieved20 December 2016.
  7. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75. Retrieved19 December 2016.
  8. ^abcChang, Chan-Kao;Ip, Wing-Huen; Lin, Hsing-Wen; Cheng, Yu-Chi; et al. (June 2014)."313 New Asteroid Rotation Periods from Palomar Transient Factory Observations".The Astrophysical Journal.788 (1): 21.arXiv:1405.1144.Bibcode:2014ApJ...788...17C.doi:10.1088/0004-637X/788/1/17. Retrieved19 December 2016.
  9. ^Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007. Retrieved19 December 2016.
  10. ^"Minor Planet Discoverers".Minor Planet Center. 24 April 2016. Retrieved19 December 2016.
  11. ^Schmadel, Lutz D. "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

[edit]
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