词条 | 51825 Davidbrown |
释义 |
| minorplanet = yes | name = 51825 Davidbrown | background = #D6D6D6 | image = | image_size = | caption = | discovery_ref = | discoverer = NEAT | discovery_site = Palomar Obs. | discovered = 19 July 2001 | mpc_name = (51825) Davidbrown | alt_names = {{mp|2001 OQ|33}}{{·}}{{mp|1994 CZ|14}} {{mp|1999 CO|55}} | pronounced = | named_after = {{nowrap|David McDowell Brown [2]}} {{small|(American astronaut)}} | mp_category = main-belt{{·}}{{small|(outer)}} Eos [3] | orbit_ref = | epoch = 4 September 2017 (JD 2458000.5) | uncertainty = 0 | observation_arc = 23.79 yr (8,691 days) | aphelion = 3.1755 AU | perihelion = 2.7587 AU | semimajor = 2.9671 AU | eccentricity = 0.0702 | period = 5.11 yr (1,867 days) | mean_anomaly = 316.75° | mean_motion = {{Deg2DMS|0.1928|sup=ms}} / day | inclination = 9.6190° | asc_node = 23.457° | arg_peri = 33.210° | dimensions = {{val|4.913|0.760}} km[5] | rotation = | albedo = {{val|0.184|0.032}}[5] | spectral_type = | abs_magnitude = 14.2 }}51825 Davidbrown, provisional designation {{mp|2001 OQ|33}}, is an Eoan asteroid in the outer region of the asteroid belt, approximately 5 kilometers in diameter. It was discovered on 19 July 2001, by astronomers of the Near-Earth Asteroid Tracking program at Palomar Observatory in California, United States. The asteroid was named for American astronaut David Brown, who died in the Space Shuttle Columbia disaster.[8] Orbit and classificationDavidbrown is a member the Eos family ({{small|606}}),[3] the largest family in the outer asteroid belt consisting of nearly 10,000 K-type asteroids.[10]{{rp|23}} It orbits the Sun in the outer main-belt at a distance of 2.8–3.2 AU once every 5 years and 1 month (1,867 days; semi-major axis of 2.97 AU). Its orbit has an eccentricity of 0.07 and an inclination of 10° with respect to the ecliptic.The body's observation arc begins with its first observation as {{mp|1994 CZ|14}} at ESO's La Silla Observatory in February 1994, more than 7 years prior to its official discovery observation at Palomar.[8] Physical characteristicsDiameter and albedoAccording to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Davidbrown measures 4.913 kilometers in diameter and its surface has an albedo of 0.184.[5] Rotation periodAs of 2017, no rotational lightcurve of Davidbrown has been obtained from photometric observations. The asteroid's rotation period, poles and shape remain unknown.[15] NamingThis minor planet was named after American astronaut and mission specialist David McDowell Brown, who was killed in the Columbia space shuttle reentry disaster on 1 February 2003.[2] The approved naming citation was published by the Minor Planet Center on 6 August 2003 ({{small|M.P.C. 49283}}).[17] The following asteroids were also named in memory of the other six members of STS-107: 51823 Rickhusband, 51824 Mikeanderson, 51826 Kalpanachawla, 51827 Laurelclark, 51828 Ilanramon and 51829 Williemccool. References1. ^1 2 {{cite book |title = Dictionary of Minor Planet Names – (51825) Davidbrown, Addendum to Fifth Edition: 2003–2005 |pages = 216 |last = Schmadel | first = Lutz D. |publisher = Springer Berlin Heidelberg |date = 2006 |isbn = 978-3-540-34361-5 |doi = 10.1007/978-3-540-34361-5_2554 |chapter = (51825) Davidbrown [2.97, 0.07, 9.6] }} [1][2][3][4][5][6][7]2. ^1 2 {{cite web |title = 51825 Davidbrown (2001 OQ33) |work = Minor Planet Center |url = http://www.minorplanetcenter.net/db_search/show_object?object_id=51825 |accessdate = 28 December 2017}} 3. ^1 {{cite web |title = MPC/MPO/MPS Archive |work = Minor Planet Center |url = http://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html |accessdate = 28 December 2017}} 4. ^1 2 {{cite web |title = Small Bodies Data Ferret |work = Nesvorny HCM Asteroid Families V3.0 |url = https://sbntools.psi.edu/ferret/PropertySearch/familyForm.action |accessdate = 28 December 2017}} 5. ^1 {{Cite book |first1 = D. |last1 = Nesvorný |first2 = M. |last2 = Broz |first3 = V. |last3 = Carruba |date = December 2014 |title = Identification and Dynamical Properties of Asteroid Families |journal = Asteroids IV |pages = 297–321 |bibcode = 2015aste.book..297N |doi = 10.2458/azu_uapress_9780816532131-ch016 |arxiv = 1502.01628 |isbn = 9780816532131 }} 6. ^1 2 3 {{cite journal |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 = J. |last6 = Dailey |first7 = P. R. M. |last7 = Eisenhardt |first8 = R. S. |last8 = McMillan |first9 = T. B. |last9 = Spahr |first10 = M. F. |last10 = Skrutskie |first11 = D. |last11 = Tholen |first12 = R. G. |last12 = Walker |first13 = E. L. |last13 = Wright |first14 = E. |last14 = DeBaun |first15 = D. |last15 = Elsbury |first16 = T., IV |last16 = Gautier |first17 = S. |last17 = Gomillion |first18 = A. |last18 = Wilkins |date = November 2011 |title = Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M |journal = The Astrophysical Journal |volume = 741 |issue = 2 |page = 20 |bibcode = 2011ApJ...741...68M |doi = 10.1088/0004-637X/741/2/68 |arxiv = 1109.4096 |access-date= 28 December 2017}} 7. ^1 {{cite web |title = LCDB Data for (51825) Davidbrown |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=51825%7CDavidbrown |accessdate = 28 December 2017}} }} External links
5 : Eos asteroids|Discoveries by NEAT|Minor planets named for people|Named minor planets|Astronomical objects discovered in 2001 |
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