Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

1938 Lausanna

From Wikipedia, the free encyclopedia
Main-belt asteroid

1938 Lausanna
Discovery[1]
Discovered byP. Wild
Discovery siteZimmerwald Obs.
Discovery date19 April 1974
Designations
(1938) Lausanna
Named after
Lausanne(Swiss city)[2]
1974 HC · 1934 KA
1947 DB · 1950 CO
1955 VK · 1957 EH
1962 WB1 · 1967 ED1
1971 OX · 1972 XY1
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc82.99 yr (30,312 days)
Aphelion2.5938AU
Perihelion1.8796 AU
2.2367 AU
Eccentricity0.1597
3.35yr (1,222 days)
329.17°
0° 17m 40.56s / day
Inclination3.3343°
171.69°
64.830°
Physical characteristics
Dimensions7.638±0.124 km[4]
7.82 km(calculated)[3]
8.214±0.077 km[5]
2.748±0.001h[a]
2.748±0.001 h[6]
0.1660±0.0301[5]
0.192±0.055[4]
0.24(assumed)[3]
S[3][7]
12.60±0.26[7] · 12.7[1][3] · 13.0[5]

1938 Lausanna, provisional designation1974 HC, is a stony Florianasteroid from the inner regions of theasteroid belt. It is approximately 8 kilometers in diameter, and was discovered on 19 April 1974 by Swiss astronomer,Paul Wild atZimmerwald Observatory near Bern, Switzerland.[8] It is named for the city ofLausanne.[2]

Orbit and classification

[edit]

Lausanna is aS-type asteroid and member of theFlora family, one of the largest collisional populations of stony asteroids in the main-belt. It orbits the Sun in theinner main-belt at a distance of 1.9–2.6 AU once every 3 years and 4 months (1,222 days). Its orbit has aneccentricity of 0.16 and aninclination of 3° with respect to theecliptic.[1] It was first identified as1934 KA atJohannesburg Observatory in 1934, extending the body'sobservation arc by 40 years prior to its official discovery observation at Zimmerwald.[8]

Physical characteristics

[edit]

Rotation period

[edit]

In March 2014, two rotationallightcurves ofLausanna were obtained from photometric observations by American astronomerBrian Skiff and by Johan Warell at Lindby Observatory (K60) in Sweden. Lightcurve analysis gave an identicalrotation period of 2.748 hours with a brightness amplitude of 0.13 and 0.12magnitude, respectively (U=3-/2).[a][6] The short period is near the threshold of 2.2 hours forfast rotating asteroids.

Diameter and albedo

[edit]

According to the space-based survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Lausanna measures 7.64 and 8.21 kilometers in diameter, and its surface has analbedo of 0.166 and 0.192, respectively.[4][5] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the largest member and namesake of its family – and calculates a diameter of 7.82 kilometers based on anabsolute magnitude of 12.7.[3]

Naming

[edit]

Thisminor planet was named for the Swiss city ofLausanne, located in the French-speaking part of the country. The discoverer Paul Wild, known for his unconventional minor-planet namings, discovered three more asteroids during winter of 1973/74. He named these1935 Lucerna,1936 Lugano and1937 Locarno, after the Swiss citiesLucerne,Lugano andLocarno, respectively, hence composing analliterated quartet of sequentially numbered, thematically named minor planets. The officialnaming citation was published by theMinor Planet Center on 1 April 1978 (M.P.C. 4358).[9]

Notes

[edit]
  1. ^abSkiff (2014) web: rotation period2.748±0.001 hours with a brightness amplitude of0.13 mag and a Quality Code of 3-. Summary figures atCollaborative Asteroid Lightcurve Link (CALL) for (1938) Lausanna

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1938 Lausanna (1974 HC)" (2017-05-06 last obs.).Jet Propulsion Laboratory. Retrieved10 June 2017.
  2. ^abSchmadel, Lutz D. (2007). "(1938) Lausanna".Dictionary of Minor Planet Names – (1938) Lausanna.Springer Berlin Heidelberg. p. 155.doi:10.1007/978-3-540-29925-7_1939.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1938) Lausanna". Asteroid Lightcurve Database (LCDB). Retrieved26 January 2017.
  4. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved26 January 2017.
  5. ^abcdMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; 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. ^abWarell, Johan; Pappini, Riccardo (January 2015)."Rotational Period of 1938 Lausanna".The Minor Planet Bulletin.42 (1):20–21.Bibcode:2015MPBu...42...20W.ISSN 1052-8091. Retrieved26 January 2017.
  7. ^abVeres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; 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. Retrieved26 January 2017.
  8. ^ab"1938 Lausanna (1974 HC)".Minor Planet Center. Retrieved26 January 2017.
  9. ^Schmadel, Lutz D. (2009). "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]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=1938_Lausanna&oldid=1313004208"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp