1930 Lucifer: Perbedaan antara revisi

{{Infobox Planet|minorplanet=yes|name=1930 Lucifer|background=#D6D6D6|image=1930Lucifer (Lightcurve Inversion).png|image_size=265|caption={{longitem|3D model berdasarkan [[Kurva cahaya]] dari ''Lucifer''|style=padding: 4px 0; line-height: 1.4em;}}|discovered=29 October 1964|discoverer=[[Elizabeth Roemer|E. Roemer]]|discovery_site=[[United States Naval Observatory Flagstaff Station|NOFS]] ([[United States Naval Observatory|USNO]])|mpc_name=(1930) Lucifer|alt_names=1964 UA{{·}}1954 SQ<br />1954 TC|pronounced={{IPAc-en|ˈ|lj|uː|s|ɪ|f|ər}} {{respell|LEW|si|fər}}|named_after=[[Lucifer|Lucifer]] {{small|(kepercayaan)}}|mp_category=[[Sabuk asteroid]]{{·}}{{small|([[Kirkwood gap|Terluar]])}}|epoch=4 September 2017 ([[Julian day|JD]] 2458000.5)|uncertainty=0|observation_arc=62.61 th (22,870 hari)|aphelion=3.3078 [[Satuan astronomi|SA]]|perihelion=2.4883 SA|semimajor=2.8981 SA|eccentricity=0.1414|period=4.93 [[Tahun Julian|th]] (1,802 hari)|mean_anomaly=334.70[[Derajat (satuan sudut)|°]]|mean_motion={{Deg2DMS|0.1998|sup=ms}} / hari|inclination=14.057°|asc_node=318.53°|arg_peri=341.37°|dimensions=26.90 km {{small|(derived)}}<br />{{val|27.00|3.2}} km<br />{{val|30.92|0.84}} km<br />{{val|34.04|11.55}} km<br />{{val|34.437|0.168}} km<br />{{val|36.335|0.376}} km<br />{{val|39.61|0.50}} km|rotation={{val|13.0536|0.0005}} h<br />{{val|13.054|0.004}} [[Hour|h]]<br />{{val|13.056|0.005}} h<br />{{val|13.092|0.0808}} h|albedo={{val|0.05|0.03}}<br />{{val|0.050|0.001}}<br />{{val|0.0584|0.0081}}<br />{{val|0.067|0.007}}<br />{{val|0.074|0.011}}<br />0.0886 {{small|(derived)}}<br />{{val|0.1058|0.030}}|spectral_type=[[SMASS classification|SMASS]] = Cgh{{·}}[[C-type asteroid|C]]|abs_magnitude={{val|10.818|0.002}} {{small|(R)}}{{·}}10.9{{·}}11.00{{·}}11.1{{·}}}}

''Lucifer'' mengorbit Matahari dari bagian terluar [[sabuk asteroid]] pada jarak 2.5-3.3 [[Satuan astronomi|SA]], sekali dalam 4 tahun 11 bulan, atau lebih tepatnya 1802 hari. Lintasan orbitnya memiliki [[Eksentrisitas orbit|eksentrisitas]] sebesar 0.14 dan [[inklinasi]] sebesar 14° dari sumbu [[ekliptika]]<ref>{{Cite book|last=Schmadel|first=Lutz D.|date=2003|url=https://en.wiki-indonesia.club/wiki/Special:BookSources/978-3-540-00238-3|title=Dictionary of minor planet names / Lutz D. Schmadel. Hauptbd.|location=Berlin Heidelberg New York Hong Kong London Milan Paris Tokyo|publisher=Springer|isbn=978-3-540-00238-3|edition=5., rev. and enl. ed|series=Physics and astronomy online library}}</ref>.

Pada Januari 2005, observasi yang dilakukan astronomer Horacio Correia juga mendapatkan hasil yang serupa yaitu periode rotasinya sebesar 13.054 jam<ref>{{Cite web|title=CdR&CdL: Courbe de rotation et luminosité d'astéroïdes, de comètes et d'étoiles variables|url=http://obswww.unige.ch/~behrend/page4cou.html#001930|website=obswww.unige.ch|access-date=2023-05-25}}</ref>. Pada tahun 2013, kurva cahaya lainnya didapatkan dari Palomar Transient Factory<ref>{{Cite journal|last=Warner|first=Brian D.|date=2005-09-01|title=Asteroid lightcurve analysis at the Palmer Divide Observatory - winter 2004-2005|url=https://ui.adsabs.harvard.edu/abs/2005MPBu...32...54W|journal=Minor Planet Bulletin|volume=32|pages=54–58|issn=1052-8091}}</ref>, dan model kurva cahaya dari berbagai sumber data termasuk database AstDyS juga mendapatkan hasil yang serupa 13.0536 jam dengan sumbu rotasi pada ([[Tata koordinat langit|32°,17°]])<ref>{{Cite journal|last=Waszczak|first=Adam|last2=Chang|first2=Chan-Kao|last3=Ofek|first3=Eran O.|last4=Laher|first4=Russ|last5=Masci|first5=Frank|last6=Levitan|first6=David|last7=Surace|first7=Jason|last8=Cheng|first8=Yu-Chi|last9=Ip|first9=Wing-Huen|date=2015-09-01|title=Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry|url=https://ui.adsabs.harvard.edu/abs/2015AJ....150...75W|journal=The Astronomical Journal|volume=150|pages=75|doi=10.1088/0004-6256/150/3/75|issn=0004-6256}}</ref>.