词条 | 1016 Anitra |
释义 |
| minorplanet = yes | name = 1016 Anitra | background = #D6D6D6 | image = | image_size = | caption = | discovery_ref = | discoverer = K. Reinmuth | discovery_site = Heidelberg Obs. | discovered = 31 January 1924 | mpc_name = (1016) Anitra | alt_names = 1924 QG{{·}}{{mp|1929 TE|1}} | pronounced = | named_after = fictional character in drama Peer Gynt [2] | mp_category = main-belt{{·}}{{small|(inner)}} [3] Flora [4] | orbit_ref = | epoch = 4 September 2017 (JD 2458000.5) | uncertainty = 0 | observation_arc = 93.42 yr (34,123 days) | aphelion = 2.5035 AU | perihelion = 1.9356 AU | semimajor = 2.2196 AU | eccentricity = 0.1279 | period = 3.31 yr (1,208 days) | mean_anomaly = 176.01° | mean_motion = {{Deg2DMS|0.2981|sup=ms}} / day | inclination = 6.0352° | asc_node = 8.8588° | arg_peri = 53.320° | satellites = 1[6][7] | dimensions = {{val|9.539|0.078}} km[8] {{val|10.302|0.068}} km[9] 12.97 km {{small|(calculated)}}[3] | rotation = {{val|5.928|0.001}} h[11] {{val|5.9288|0.0005}} h[12] {{val|5.929|0.001}} h[13] {{val|5.9295|0.0005}} h[14] 5.92951 h[3] {{val|5.9294|0.0001}} h[7] {{val|5.9300|0.0001}} h[7] {{val|5.930}} h[18] {{val|5.93|}} h{{efn|name=lcdb-Menke-2011}} {{val|5.9301|0.0003}} h[19] | albedo = 0.20 {{small|(assumed)}}[3] {{val|0.2728|0.0572}}[9] {{val|0.308|0.048}}[8] | spectral_type = SMASS {{=}} S {{·}}S [3] | abs_magnitude = 11.8[3]{{·}}11.9{{·}}12.0[9] }} 1016 Anitra, provisional designation {{mp|1924 QG}}, is a stony Florian asteroid and suspected asynchronous binary system from the inner regions of the asteroid belt, approximately 10 kilometers in diameter. It was discovered on 31 January 1924, by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany.[28] The asteroid was likely named after the fictional character Anitra from Henrik Ibsen's drama Peer Gynt.[2] Orbit and classificationAnitra is a member of the Flora family ({{small|402}}), a giant asteroid family and the largest family of stony asteroids in the main-belt.[4][31]{{rp|23}} It orbits the Sun in the inner main-belt at a distance of 1.9–2.5 AU once every 3 years and 4 months (1,208 days). Its orbit has an eccentricity of 0.13 and an inclination of 6° with respect to the ecliptic. The asteroid's observation arc begins at Heidelberg, 12 days after to its official discovery observation.[28] Physical characteristicsIn the SMASS classification, Anitra is a common, stony S-type asteroid. Rotation periodIn November 2015, a rotational lightcurve of Anitra was obtained from photometric observations by an international collaborations of astronomers who combined their observational results. Lightcurve analysis gave a rotation period of 5.92951 hours with a brightness amplitude of 0.30 magnitude ({{small|U=3}}).[7] Binary systemAnitra is a suspected asynchronous binary asteroid, a system with a fairly large separation, for which tidal forces have been insufficient to synchronize the periods within the system's lifetime.[6][7] The likely minor-planet moon has a rotation period of 2.609 hours and is thought to orbit its primary every 240 hours. The results, however, are still tentative.[3] More than 100 known binaries from the asteroid belt have already been discovered. Diameter and albedoAccording to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Anitra measures 9.539 and 10.302 kilometers in diameter and its surface has an albedo of 0.2728 and 0.308, respectively.[8][9] The Collaborative Asteroid Lightcurve Link assumes an standard albedo for stony S-type asteroids of 0.20 and calculates a diameter of 12.97 kilometers based on an absolute magnitude of 11.8.[3] NamingThis minor planet was probably named after the Arabian dancer Anitra, daughter of a Bedouin chief in Henrik Ibsen's drama Peer Gynt, a five-act play in verse. The music was composed by Edvard Grieg who named one piece "Anitra's Dance".[2] The minor planets {{MoMP|4872|(4872)}} and {{MoMP|5696|(5696)}} are named after Grieg and Ibsen, respectively.[2] The official naming citation is based on research by Lutz Schmadel and feedback from astronomers R. Bremer and I. van Houten-Groeneveld.[2] Notes{{notelist|refs={{efn|name=lcdb-Menke-2011|1=Menke (2011) web: rotation period {{val|5.93}} hours with a brightness amplitude of {{val|0.50}} magnitude and a quality code of 2. Summary figures at Collaborative Asteroid Lightcurve Link (CALL)}}}} References1. ^1 2 3 4 5 {{cite book |title = Dictionary of Minor Planet Names – (1016) Anitra |last = Schmadel | first = Lutz D. |publisher = Springer Berlin Heidelberg |pages = 87–88 |date = 2007 |isbn = 978-3-540-00238-3 |doi = 10.1007/978-3-540-29925-7_1017 |chapter = (1016) Anitra }} [1][2][3][4][5][6][7][8][9][10][11][12][13][14][15]2. ^1 2 {{cite web |title = 1016 Anitra (1924 QG) |work = Minor Planet Center |url = http://www.minorplanetcenter.net/db_search/show_object?object_id=1016 |accessdate = 29 August 2017}} 3. ^1 2 3 {{cite journal |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 |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014ApJ...791..121M |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 |access-date= 29 August 2017}} 4. ^1 2 {{cite web |first1 = Robert |last1 = Johnston |title = (1016) Anitra |publisher = johnstonsarchive.net |date = 16 July 2017 |url = http://www.johnstonsarchive.net/astro/astmoons/am-01016.html |access-date= 29 August 2017}} 5. ^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 = 29 August 2017}} 6. ^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 }} 7. ^1 2 3 4 5 6 7 8 {{cite web |title = LCDB Data for (1016) Anitra |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=1016%7CAnitra |accessdate = 29 August 2017}} 8. ^1 2 3 4 {{cite journal |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. 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9 : Flora asteroids|Baptistina asteroids|Discoveries by Karl Wilhelm Reinmuth|Minor planets named for literary characters|Named minor planets|Peer Gynt|Binary asteroids|S-type asteroids (SMASS)|Astronomical objects discovered in 1924 |
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