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1334 Lundmarka

From Wikipedia, the free encyclopedia
Main-belt asteroid

1334 Lundmarka
Shape model ofLundmarka from itslightcurve
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date16 July 1934
Designations
(1334) Lundmarka
Named after
Knut Lundmark(astronomer)[2]
1934 OB
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc82.89 yr (30,274 days)
Aphelion3.1912AU
Perihelion2.6376 AU
2.9144 AU
Eccentricity0.0950
4.98yr (1,817 days)
286.14°
0° 11m 53.16s / day
Inclination11.453°
133.23°
129.65°
Physical characteristics
Dimensions27.62±2.33 km[4]
29.82±3.2 km(IRAS:14)[5]
30.35 km(derived)[3]
6.250±0.003h[6]
6.25033±0.00001 h[7]
0.0600±0.016(IRAS:14)[5]
0.1455(derived)[3]
0.242±0.246[4]
X[8] · C[3]
9.95[4] · 10.3[3] · 10.4[1] · 10.71±0.20[8]

1334 Lundmarka, provisional designation1934 OB, is a carbonaceousasteroid from the outer region of theasteroid belt, approximately 30 kilometers in diameter. It was discovered on 16 July 1934, by German astronomerKarl Reinmuth atHeidelberg Observatory in southern Germany, and named after Swedish astronomerKnut Lundmark.[2][9]

Orbit and classification

[edit]

Lundmarka is classified asC-type andX-type asteroid by theLCDB andPan-STARRS, respectively.[3][8] It orbits the Sun in theouter main-belt at a distance of 2.6–3.2 AU once every 4 years and 12 months (1,817 days). Its orbit has aneccentricity of 0.10 and aninclination of 11° with respect to theecliptic.[1] The body'sobservation arc begins with its official discovery observation at Heidelberg, as noprecoveries were taken and no prior identifications were made.[9]

Rotation period

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A rotationallightcurve ofLundmarka was obtained from photometric observations made at the AustralianOakley Southern Sky Observatory (E09) in September 2014. The lightcurve gave arotation period of6.250±0.003 hours with a brightness variation of 0.70 inmagnitude (U=3-).[6]

In March 2016, a second period was published based on data from the Lowell Photometric Database. Using lightcurve inversion and convex shape models, as well as distributed computing power and the help of individual volunteers, a period of6.25033±0.00001 hours was derived from the database's sparse-in-time photometry data (U=n.a.).[7]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical Satellite (IRAS) and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Lundmarka measures 29.8 and 27.6 kilometers in diameter, respectively, and its surface has a correspondingalbedo of 0.06 and 0.24.[1][4] TheCollaborative Asteroid Lightcurve Link derives an intermediary albedo of 0.146 and a diameter of 30.4 kilometers.[3]

Naming

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Thisminor planet was named in memory of Swedish astronomerKnut Lundmark (1889–1958), who was the head of theLund Observatory. He thoroughly analyzed galaxies andglobular clusters, and pioneered inmeasuring galactic distances and absolute stellar magnitudes. Lundmark also appeared in national radio with programs onpopular astronomy and the history of science. The officialnaming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 121).[2] The lunar craterLundmark is also named in his honour.[2]

References

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  1. ^abcde"JPL Small-Body Database Browser: 1334 Lundmarka (1934 OB)" (2017-06-04 last obs.).Jet Propulsion Laboratory. Retrieved25 July 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1334) Lundmarka".Dictionary of Minor Planet Names – (1334) Lundmarka.Springer Berlin Heidelberg. p. 109.doi:10.1007/978-3-540-29925-7_1335.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1334) Lundmarka". Asteroid Lightcurve Database (LCDB). Retrieved17 May 2016.
  4. ^abcdMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8. Retrieved17 May 2016.
  5. ^abTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System.12: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved22 October 2019.
  6. ^abBohn, Lucas; Hibbler, Brianna; Stein, Gregory; Ditteon, Richard (April 2015)."Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2014 September".The Minor Planet Bulletin.42 (2):89–90.Bibcode:2015MPBu...42...89B.ISSN 1052-8091. Retrieved17 May 2016.
  7. ^abDurech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016)."Asteroid models from the Lowell photometric database".Astronomy and Astrophysics.587: 6.arXiv:1601.02909.Bibcode:2016A&A...587A..48D.doi:10.1051/0004-6361/201527573. Retrieved17 May 2016.
  8. ^abcVeres, 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. Retrieved17 May 2016.
  9. ^ab"1334 Lundmarka (1934 OB)".Minor Planet Center. Retrieved17 May 2016.

External links

[edit]
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