1551 Argelander
{{Short description|Main-belt asteroid}}
{{Use dmy dates|date=December 2018}}
{{Infobox planet
| minorplanet = yes
| name = 1551 Argelander
| background = #D6D6D6
| image = File:001551-asteroid shape model (1551) Argelander.png
| image_scale =
| caption = Shape model of Argelander from its lightcurve
| discoverer = Y. Väisälä
| discovery_site = Turku Obs.
| discovered = 24 February 1938
| mpc_name = (1551) Argelander
| alt_names = {{mp|1938 DC|1}}{{·}}1930 BL
1940 XD{{·}}{{mp|1951 XG|1}}
{{mp|1953 GD|1}}{{·}}1957 KR
1962 XP
| pronounced =
| named_after = {{nowrap|Friedrich Argelander}}
{{small|(German astronomer)}}
| mp_category = main-belt{{·}}{{small|(inner)}}
background
| epoch = 27 April 2019 (JD 2458600.5)
| uncertainty = 0
| observation_arc = 88.76 yr (32,418 d)
| aphelion = 2.5539 AU
| perihelion = 2.2350 AU
| semimajor = 2.3944 AU
| eccentricity = 0.0666
| period = 3.71 yr (1,353 d)
| mean_anomaly = 147.41°
| mean_motion = {{Deg2DMS|0.2660|sup=ms}} / day
| inclination = 3.7615°
| asc_node = 107.23°
| arg_peri = 233.60°
| mean_diameter = {{val|9.19|0.27|ul=km}}
{{val|10.238|0.122|u=km}}
{{val|10.50|0.50|u=km}}
{{val|11.016|0.073|u=km}}
| rotation = {{val|4.063|0.006|ul=h}}
| albedo = {{val|0.1940}}
{{val|0.217}}
{{val|0.222}}
{{val|0.302}}
| spectral_type = S {{small|(assumed)}}
}}
1551 Argelander, provisional designation {{mp|1938 DC|1}}, is a background asteroid from the inner regions of the asteroid belt, approximately {{convert|10|km|mi|abbr=off|sigfig=2|sp=us}} in diameter. It was discovered on 24 February 1938, by Finnish astronomer Yrjö Väisälä at the Turku Observatory in southwest Finland. The likely S-type asteroid has a rotation period of 4.1 hours. It was named after German astronomer Friedrich Argelander.
Orbit and classification
Argelander is a non-family asteroid from the main belt's background population. It orbits the Sun in the inner main-belt at a distance of 2.2–2.6 AU once every 3 years and 9 months (1,353 days; semi-major axis of 2.39 AU). Its orbit has an eccentricity of 0.07 and an inclination of 4° with respect to the ecliptic. The body's observation arc begins with its first observation as {{mp|1930 BL}} at Heidelberg Observatory in January 1930, or 8 years prior to its official discovery observation at Turku.
Naming
This minor planet was named after Friedrich Wilhelm Argelander (1799–1875), author of the famous Bonner Durchmusterung and 19th-century head of the ancient observatory at Turku and Bonn {{Obscode|520}}. The official {{MoMP|1551|naming citation}} was published by the Minor Planet Center on 30 January 1964 ({{small|M.P.C. 2278}}). The lunar crater Argelander is also named after him.
Physical characteristics
Argelander is an assumed S-type asteroid.
= Rotation period and poles =
In August 2017, a rotational lightcurve of Argelander was obtained from photometric observations at the Chilean Cerro Tololo Inter-American Observatory using the SARA South Telescope. Lightcurve analysis gave a rotation period of {{val|4.063|0.006}} hours and a brightness variation of 0.48 magnitude ({{small|U=2+}}). In January 2012, astronomers at the Palomar Transient Factory had also determined a period of {{val|4.061|0.0023}} with an amplitude of 0.41 magnitude ({{small|U=2}}).
A modeled lightcurve using photometric data from the Lowell Photometric Database was published in 2016. It gave a concurring period of {{val|4.058350|0.000001}} hours, as well as two spin axes at (3.0°, −81.0°) and (183.0°, −72.0°) in ecliptic coordinates (λ, β).
= Diameter and albedo =
According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Argelander measures between 9.2 and 11.0 kilometers in diameter and its surface has an albedo between 0.19 and 0.30. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.20 and calculates a diameter of 9.60 kilometers based on an absolute magnitude of 12.45.
References
{{reflist|30em|refs=
|type = 2018-10-20 last obs.
|title = JPL Small-Body Database Browser: 1551 Argelander (1938 DC1)
|url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001551
|publisher = Jet Propulsion Laboratory
|accessdate = 11 December 2018}}
|title = Dictionary of Minor Planet Names – (1551) Argelander
|last = Schmadel | first = Lutz D.
|publisher = Springer Berlin Heidelberg
|page = 123
|date = 2007
|isbn = 978-3-540-00238-3
|doi = 10.1007/978-3-540-29925-7_1552 |chapter = (1551) Argelander }}
|title = 1551 Argelander (1938 DC1)
|work = Minor Planet Center
|url = https://www.minorplanetcenter.net/db_search/show_object?object_id=1551
|accessdate = 11 December 2018}}
|title = Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008)
|chapter = Appendix – Publication Dates of the MPCs
|last = Schmadel |first=Lutz D.
|publisher = Springer Berlin Heidelberg
|page = 221
|isbn = 978-3-642-01964-7
|doi = 10.1007/978-3-642-01965-4|year = 2009
|chapter-url = https://cds.cern.ch/record/1339661
}}
|display-authors = 6
|first1 = Joseph R. |last1 = Masiero
|first2 = T. |last2 = Grav
|first3 = A. K. |last3 = Mainzer
|first4 = C. R. |last4 = Nugent
|first5 = J. M. |last5 = Bauer
|first6 = R. |last6 = Stevenson
|first7 = S. |last7 = Sonnett
|date = August 2014
|title = Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos
|journal = The Astrophysical Journal
|volume = 791
|issue = 2
|page = 11
|bibcode = 2014ApJ...791..121M
|doi = 10.1088/0004-637X/791/2/121
|arxiv = 1406.6645|s2cid = 119293330 }}
|title = Asteroid (1551) Argelander – Proper elements
|publisher = AstDyS-2, Asteroids – Dynamic Site
|url = https://newton.spacedys.com/astdys/index.php?n=1551&pc=1.1.6
|accessdate = 10 December 2018}}
|title = Asteroid 1551 Argelander
|work = Small Bodies Data Ferret
|url = https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1551+Argelander
|accessdate = 11 December 2018}}
|title = LCDB Data for (1551) Argelander
|publisher = Asteroid Lightcurve Database (LCDB)
|url = http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=1551%7CArgelander
|accessdate = 11 December 2018}}
|display-authors = 6
|first1 = A. |last1 = Mainzer
|first2 = T. |last2 = Grav
|first3 = J. |last3 = Masiero
|first4 = E. |last4 = Hand
|first5 = J. |last5 = Bauer
|first6 = D. |last6 = Tholen
|first7 = R. S. |last7 = McMillan
|first8 = T. |last8 = Spahr
|first9 = R. M. |last9 = Cutri
|first10 = E. |last10 = Wright
|first11 = J. |last11 = Watkins
|first12 = W. |last12 = Mo
|first13 = C. |last13 = Maleszewski
|date = November 2011
|title = NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results
|journal = The Astrophysical Journal
|volume = 741
|issue = 2
|page = 25
|bibcode = 2011ApJ...741...90M
|doi = 10.1088/0004-637X/741/2/90
|arxiv = 1109.6407
|s2cid = 35447010 }} ([http://iopscience.iop.org/0004-637X/741/2/68/fulltext/apj398969t1_mrt.txt catalog])
|display-authors = 6
|first1 = Joseph R. |last1 = Masiero
|first2 = A. K. |last2 = Mainzer
|first3 = T. |last3 = Grav
|first4 = J. M. |last4 = Bauer
|first5 = R. M. |last5 = Cutri
|first6 = C. |last6 = Nugent
|first7 = M. S. |last7 = Cabrera
|date = November 2012
|title = Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids
|journal = The Astrophysical Journal Letters
|volume = 759
|issue = 1
|page = 5
|bibcode = 2012ApJ...759L...8M
|doi = 10.1088/2041-8205/759/1/L8
|arxiv = 1209.5794|s2cid = 46350317 }}
|display-authors = 6
|first1 = A. K. |last1 = Mainzer
|first2 = J. M. |last2 = Bauer
|first3 = R. M. |last3 = Cutri
|first4 = T. |last4 = Grav
|first5 = E. A. |last5 = Kramer
|first6 = J. R. |last6 = Masiero
|first7 = C. R. |last7 = Nugent
|first8 = S. M. |last8 = Sonnett
|first9 = R. A. |last9 = Stevenson
|first10 = E. L. |last10 = Wright
|date = June 2016
|title = NEOWISE Diameters and Albedos V1.0
|url = https://sbnarchive.psi.edu/pds3/non_mission/EAR_A_COMPIL_5_NEOWISEDIAM_V1_0/data/neowise_mainbelt.tab
|journal = NASA Planetary Data System
|pages = EAR-A-COMPIL-5-NEOWISEDIAM-V1.0
|bibcode = 2016PDSS..247.....M
|access-date= 11 December 2018}}
|display-authors = 6
|first1 = Fumihiko |last1 = Usui
|first2 = Daisuke |last2 = Kuroda
|first3 = Thomas G. |last3 = Müller
|first4 = Sunao |last4 = Hasegawa
|first5 = Masateru |last5 = Ishiguro
|first6 = Takafumi |last6 = Ootsubo
|first7 = Daisuke |last7 = Ishihara
|first8 = Hirokazu |last8 = Kataza
|first9 = Satoshi |last9 = Takita
|first10 = Shinki |last10 = Oyabu
|first11 = Munetaka |last11 = Ueno
|first12 = Hideo |last12 = Matsuhara
|first13 = Takashi |last13 = Onaka
|date = October 2011
|title = Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey
|journal = Publications of the Astronomical Society of Japan
|volume = 63
|issue = 5
|pages = 1117–1138
|bibcode = 2011PASJ...63.1117U
|doi = 10.1093/pasj/63.5.1117
|doi-access=
}} ([http://vizier.cfa.harvard.edu/viz-bin/VizieR-5?-source=J/PASJ/63/1117/acua_v1&Num=1551 online], [https://core.ac.uk/download/pdf/43545172.pdf AcuA catalog p. 153])
|first1 = Michael |last1 = Fauerbach
|first2 = Austin |last2 = Brown
|date = July 2018
|title = Lightcurve Analysis of Minor Planets 1132 Hollandia, 1184 Gaea 1322 Coppernicius, 1551 Argelander, and 3230 Vampilov
|journal = The Minor Planet Bulletin
|volume = 45
|issue = 3
|pages = 240–241
|issn = 1052-8091
|bibcode = 2018MPBu...45..240F
}}
|first1 = J. |last1 = Durech
|first2 = J. |last2 = Hanus
|first3 = D. |last3 = Oszkiewicz
|first4 = R. |last4 = Vanco
|date = March 2016
|title = Asteroid models from the Lowell photometric database
|journal = Astronomy and Astrophysics
|volume = 587
|page = 6
|bibcode = 2016A&A...587A..48D
|doi = 10.1051/0004-6361/201527573
|arxiv = 1601.02909
|s2cid = 118427201
}}
|display-authors = 6
|first1 = Adam |last1 = Waszczak
|first2 = Chan-Kao |last2 = Chang
|first3 = Eran O. |last3 = Ofek
|first4 = Russ |last4 = Laher
|first5 = Frank |last5 = Masci
|first6 = David |last6 = Levitan
|first7 = Jason |last7 = Surace
|first8 = Yu-Chi |last8 = Cheng
|first9 = Wing-Huen |last9 = Ip
|first10 = Daisuke |last10 = Kinoshita
|first11 = George |last11 = Helou
|first12 = Thomas A. |last12 = Prince
|first13 = Shrinivas |last13 = Kulkarni
|date = September 2015
|title = Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry
|journal = The Astronomical Journal
|volume = 150
|issue = 3
|page = 35
|bibcode = 2015AJ....150...75W
|doi = 10.1088/0004-6256/150/3/75
|arxiv = 1504.04041|s2cid = 8342929 }}
}}
External links
- [http://www.minorplanet.info/PHP/lcdbsummaryquery.php Asteroid Lightcurve Database (LCDB)], query form ([http://www.minorplanet.info/lightcurvedatabase.html info] {{Webarchive|url=https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html |date=16 December 2017 }})
- [https://books.google.com/books?id=aeAg1X7afOoC&pg Dictionary of Minor Planet Names], Google books
- [https://www.minorplanetcenter.net/iau/lists/NumberedMPs000001.html Discovery Circumstances: Numbered Minor Planets (1)-(5000)] – Minor Planet Center
- {{AstDys|1551}}
- {{JPL small body}}
{{Minor planets navigator |1550 Tito |number=1551 |1552 Bessel}}
{{Small Solar System bodies}}
{{Authority control}}
{{DEFAULTSORT:Argelander}}