Neptunus: Perbedaan antara revisi
Konten dihapus Konten ditambahkan
k Melindungi "Neptunus": Perlindungan sebagian bawaan untuk semua AP. ([Sunting=Hanya untuk pengguna terdaftar otomatis] (selamanya)) |
Add 5 books for Wikipedia:Pemastian (20210913sim)) #IABot (v2.0.8.1) (GreenC bot Tag: halaman dengan galat kutipan |
||
Baris 263:
|last=Stanley|first=Sabine|author2=Bloxham, Jeremy
|title=Convective-region geometry as the cause of Uranus' and Neptune's unusual magnetic fields
|url=https://archive.org/details/sim_nature-uk_2004-03-11_428_6979/page/151|journal=Nature|date=March 11, 2004
|volume=428|pages=151–153
|doi=10.1038/nature02376
Baris 507:
|author2=Macintosh, B. A.; Gibbard, S. G.; Gavel, D. T.; Roe, H. G.; de Pater, I.; [[Andrea Ghez|Ghez, A. M.]]; Acton, D. S.; Lai, O.; Stomski, P.; Wizinowich, P. L.
|title=Cloud Structures on Neptune Observed with Keck Telescope Adaptive Optics
|url=https://archive.org/details/sim_astronomical-journal_2003-01_125_1/page/364|journal=The Astronomical Journal,
|year=2003|volume=125|issue=1|pages=364–375
|bibcode=2003AJ....125..364M
Baris 542:
|last=Varadi|first=F.
|title=Periodic Orbits in the 3:2 Orbital Resonance and Their Stability
|url=https://archive.org/details/sim_astronomical-journal_1999-11_118_5/page/2526|journal=The Astronomical Journal
|year=1999|volume=118
|issue=5|pages=2526–2531
Baris 548:
|doi=10.1086/301088}}</ref> Resonansi 3:4, 3:5, 4:7 dan 2:5 kurang padat.<ref>{{cite book|title=Beyond Pluto: Exploring the outer limits of the solar system|url=https://archive.org/details/beyondplutoexplo00davi|author=John Davies|publisher=Cambridge University Press|year=2001|pages=[https://archive.org/details/beyondplutoexplo00davi/page/104 104]|isbn=0521800196}}</ref>
Neptunus memiliki beberapa [[Troya (astronomi)|benda troya]] yang menempati [[titik Lagrangian]] {{L4}} [[Matahari]]-Neptunus— sebuah kawasan gravitasi stabil yang mengatur orbitnya.<ref>{{cite journal|title=Resonance Occupation in the Kuiper Belt: Case Examples of the 5 : 2 and Trojan Resonances|url=https://archive.org/details/sim_astronomical-journal_2003-07_126_1/page/430|first=E. I.|last=Chiang|author2=Jordan, A. B.; Millis, R. L.; M. W. Buie; Wasserman, L. H.; Elliot, J. L.; Kern, S. D.; Trilling, D. E.; Meech, K. J.; Wagner, R. M.|year=2003|doi=10.1086/375207|journal=The Astronomical Journal|volume=126|pages=430–443|bibcode=2003AJ....126..430C|arxiv = astro-ph/0301458}}</ref> Benda [[troya Neptunus]] dapat dilihat dengan resonansi 1:1 bersama Neptunus. Troya Neptunus sangat stabil orbitnya dan mungkin memang terbentuk di pinggir Neptunus, bukan terjebak oleh gravitasinya. Benda pertama sekaligus satu-atunya yang teridentifikasi berkaitan dengan [[titik Lagrangian]] {{L5}} jalur Neptunus adalah [[2008 LC18]].<ref name="Sheppard">{{Cite journal|last = Sheppard|first = Scott S.|authorlink = Scott S. Sheppard|author2= Trujillo, Chadwick A.|title = Detection of a Trailing (L5) Neptune Trojan|journal = [[Science (jurnal)|Science]]|volume = 329|issue = 5997|pages = 1304|date = September 10, 2010|doi = 10.1126/science.1189666|pmid=20705814|bibcode = 2010Sci...329.1304S}}</ref>
== Pembentukan dan perpindahan ==
Baris 639:
|date=August 19, 2004
|title=Discovery of five irregular moons of Neptune
|url=https://archive.org/details/sim_nature-uk_2004-08-19_430_7002/page/865
|journal=Nature|volume=430|pages=865–867
|doi=10.1038/nature02832
| |||