Nice modeli (Turkish Wikipedia)

Analysis of information sources in references of the Wikipedia article "Nice modeli" in Turkish language version.

Last modified: 19:04:00, 17 May 2026 (UTC)

Ref.Un. Ref.Website

Global rank Turkish rank

5241doi.org

2^nd place

117nih.gov

5^th place

8^th place

53web.archive.org

1^st place

44archive.org

6^th place

4^th place

31core.ac.uk

1,383^rd place

489^th place

11saturnaftercassini.org

low place

11oca.eu

low place

11arxiv.org

49^th place

78^th place

archive.org (Global: 6^th place; Turkish: 4^th place)

Nesvorný (2004). "Collisional Origin of Families of Irregular Satellites". The Astronomical Journal. 127 (3): 1768-1783. doi:10.1086/382099.
Agnor (2006). "Neptune's capture of its moon Triton in a binary-planet gravitational encounter". Nature. 441 (7090): 192-194. doi:10.1038/nature04792. PMID 16688170.
Vokrouhlický (2008). "Irregular Satellite Capture by Exchange Reactions". The Astronomical Journal. 136 (4): 1463-1476. doi:10.1088/0004-6256/136/4/1463.
Bottke (2012). "An Archaean heavy bombardment from a destabilized extension of the asteroid belt". Nature. 485 (7396): 78-81. doi:10.1038/nature10967. PMID 22535245.

arxiv.org (Global: 49^th place; Turkish: 78^th place)

Morbidelli. "Origin and dynamical evolution of comets and their reservoirs". arXiv:astro-ph/0512256 .

core.ac.uk (Global: 1,383^rd place; Turkish: 489^th place)

R. Gomes (2005). "Origin of the cataclysmic Late Heavy Bombardment period of the terrestrial planets" (PDF). Nature. 435 (7041): 466-9. doi:10.1038/nature03676. PMID 15917802. 1 Şubat 2020 tarihinde kaynağından arşivlendi (PDF)30 Haziran 2021.

doi.org (Global: 2^nd place; Turkish: 2^nd place)

doi.org

R. Gomes (2005). "Origin of the cataclysmic Late Heavy Bombardment period of the terrestrial planets" (PDF). Nature. 435 (7041): 466-9. doi:10.1038/nature03676. PMID 15917802. 1 Şubat 2020 tarihinde kaynağından arşivlendi (PDF)30 Haziran 2021.
Tsiganis (2005). "Origin of the orbital architecture of the giant planets of the Solar System" (PDF). Nature. 435 (7041): 459-461. doi:10.1038/nature03539. PMID 15917800. 8 Eylül 2020 tarihinde kaynağından arşivlendi (PDF)30 Haziran 2021.
Nesvorný (2007). "Capture of Irregular Satellites during Planetary Encounters". The Astronomical Journal. 133 (5): 1962-1976. doi:10.1086/512850.
Nesvorný (2004). "Collisional Origin of Families of Irregular Satellites". The Astronomical Journal. 127 (3): 1768-1783. doi:10.1086/382099.
Bottke (2010). "The Irregular Satellites: The Most Collisionally Evolved Populations in the Solar System". The Astronomical Journal. 139 (3): 994-1014. doi:10.1088/0004-6256/139/3/994.
Agnor (2006). "Neptune's capture of its moon Triton in a binary-planet gravitational encounter". Nature. 441 (7090): 192-194. doi:10.1038/nature04792. PMID 16688170.
Vokrouhlický (2008). "Irregular Satellite Capture by Exchange Reactions". The Astronomical Journal. 136 (4): 1463-1476. doi:10.1088/0004-6256/136/4/1463.
Levison (2007). "Origin of the Structure of the Kuiper Belt during a Dynamical Instability in the Orbits of Uranus and Neptune". Icarus. 196 (1): 258-273. doi:10.1016/j.icarus.2007.11.035.
Levison (3 Nisan 2008). "Origin of the structure of the Kuiper belt during a dynamical instability in the orbits of Uranus and Neptune". Icarus. 196 (1): 258-273. doi:10.1016/j.icarus.2007.11.035.
Lovett (2010). "Kuiper Belt may be born of collisions". Nature. doi:10.1038/news.2010.522.
Wolff (2012). "Neptune on Tiptoes: Dynamical Histories that Preserve the Cold Classical Kuiper Belt". The Astrophysical Journal. 746 (2): 171. doi:10.1088/0004-637X/746/2/171.
Batygin (2011). "Retention of a Primordial Cold Classical Kuiper Belt in an Instability-Driven Model of Solar System Formation". The Astrophysical Journal. 738 (1): 13. doi:10.1088/0004-637X/738/1/13.
Brasser (2013). "Oort cloud and Scattered Disc formation during a late dynamical instability in the Solar System". Icarus. 225 (1): 40.49. doi:10.1016/j.icarus.2013.03.012.
Morbidelli (2007). "Dynamics of the Giant Planets of the Solar System in the Gaseous Protoplanetary Disk and Their Relationship to the Current Orbital Architecture". The Astronomical Journal. 134 (5): 1790-1798. doi:10.1086/521705.
Brasser (2009). "Constructing the secular architecture of the solar system II: the terrestrial planets". Astronomy and Astrophysics. 507 (2): 1053-1065. doi:10.1051/0004-6361/200912878.
Morbidelli (2010). "Evidence from the Asteroid Belt for a Violent Past Evolution of Jupiter's Orbit". The Astronomical Journal. 140 (5): 1391-1501. doi:10.1088/0004-6256/140/5/1391.
Levison (2011). "Late Orbital Instabilities in the Outer Planets Induced by Interaction with a Self-gravitating Planetesimal Disk". The Astronomical Journal. 142 (5): 152. doi:10.1088/0004-6256/142/5/152.
Nesvorný (2014). "Capture of Irregular Satellites at Jupiter". The Astrophysical Journal. 784 (1): 22. doi:10.1088/0004-637X/784/1/22.
Nesvorný (2013). "Capture of Trojans by Jumping Jupiter". The Astrophysical Journal. 768 (1): 45. doi:10.1088/0004-637X/768/1/45.
Bottke (2012). "An Archaean heavy bombardment from a destabilized extension of the asteroid belt". Nature. 485 (7396): 78-81. doi:10.1038/nature10967. PMID 22535245.
Vokrouhlický (2016). "Capture of Trans-Neptunian Planetesimals in the Main Asteroid Belt". The Astronomical Journal. 152 (2): 39. doi:10.3847/0004-6256/152/2/39.

dx.doi.org

Desch, S. J. (2007). "Mass Distribution and Planet Formation in the Solar Nebula". The Astrophysical Journal. 671 (1): 878-893. DOI:10.1086/522825.
"Solar System Formation". Reviews in Modern Astronomy. 21. 2009. ss. 215-227. DOI:10.1002/9783527629190.ch12. 9783527629190.
Tsiganis, K. (2005). "Origin of the orbital architecture of the giant planets of the Solar System" (PDF). Nature. 435 (7041): 459-461. DOI:10.1038/nature03539. PMID 15917800. 8 Eylül 2020 tarihinde kaynağından arşivlendi (PDF). Erişim tarihi: 30 Haziran 2021.
Morbidelli, A. (2005). "Chaotic capture of Jupiter's Trojan asteroids in the early Solar System" (PDF). Nature. 435 (7041): 462-465. DOI:10.1038/nature03540. PMID 15917801. 21 Şubat 2014 tarihinde kaynağından (PDF) arşivlendi.
Levison, H. F. (2007). "Origin of the Structure of the Kuiper Belt during a Dynamical Instability in the Orbits of Uranus and Neptune". Icarus. 196 (1): 258-273. DOI:10.1016/j.icarus.2007.11.035.
Morbidelli, A. (2010). "Evidence from the Asteroid Belt for a Violent Past Evolution of Jupiter's Orbit". The Astronomical Journal. 140 (5): 1391-1501. DOI:10.1088/0004-6256/140/5/1391.
Nimmo, F. (2012). "Impact-driven ice loss in outer Solar System satellites: Consequences for the Late Heavy Bombardment". Icarus. 219 (1): 508-510. DOI:10.1016/j.icarus.2012.01.016.
Levison, Harold F. (1997). "Dynamical evolution of Jupiter's Trojan asteroids". Nature. 385 (6611): 42-44. DOI:10.1038/385042a0.
Levison, H. F. (2009). "Contamination of the asteroid belt by primordial trans-Neptunian objects". Nature. 460 (7253): 364-366. DOI:10.1038/nature08094. PMID 19606143.
DeMeo, F. E. (2014). "Unexpected D-type interlopers in the inner main belt". Icarus. 229: 392-399. DOI:10.1016/j.icarus.2013.11.026.
Nesvorný, D. (2011). "Young Solar System's Fifth Giant Planet?". The Astrophysical Journal Letters. 742 (2): L22. DOI:10.1088/2041-8205/742/2/L22.
Batygin, K. (2012). "Instability-driven Dynamical Evolution Model of a Primordially Five-planet Outer Solar System". The Astrophysical Journal Letters. 744 (1): L3. DOI:10.1088/2041-8205/744/1/L3.
Nesvorný, D. (2012). "Statistical Study of the Early Solar System's Instability with Four, Five, and Six Giant Planets". The Astronomical Journal. 144 (4): 17. DOI:10.1088/0004-6256/144/4/117.
Nesvorný, D. (2015). "Jumping Neptune Can Explain the Kuiper Belt Kernel". The Astronomical Journal. 150 (3): 68. DOI:10.1088/0004-6256/150/3/68.
Nesvorný, D. (2012). "Statistical Study of the Early Solar System's Instability with Four, Five, and Six Giant Planets". The Astronomical Journal. 144 (4): 117. DOI:10.1088/0004-6256/144/4/117.
Nesvorný, D. (2015). "Evidence for Slow Migration of Neptune from the Inclination Distribution of Kuiper Belt Objects". The Astronomical Journal. 150 (3): 73. DOI:10.1088/0004-6256/150/3/73.
Deienno, R. (2017). "Constraining the giant planets' initial configuration from their evolution: implications for the timing of the planetary instability". The Astronomical Journal. 153 (4): 153. DOI:10.3847/1538-3881/aa5eaa.
Kaib, N. A. (2016). "The fragility of the terrestrial planets during a giant-planet instability". Monthly Notices of the Royal Astronomical Society. 455 (4): 3561-3569. DOI:10.1093/mnras/stv2554.
Walsh, K. J. (2011). "The effect of an early planetesimal-driven migration of the giant planets on terrestrial planet formation". Astronomy and Astrophysics. 526: A126. DOI:10.1051/0004-6361/201015277.
Toliou, A. (2016). "Magnitude and timing of the giant planet instability: A reassessment from the perspective of the asteroid belt". Astronomy & Astrophysics. 592: A72. DOI:10.1051/0004-6361/201628658.

nih.gov (Global: 5^th place; Turkish: 8^th place)

ncbi.nlm.nih.gov

R. Gomes (2005). "Origin of the cataclysmic Late Heavy Bombardment period of the terrestrial planets" (PDF). Nature. 435 (7041): 466-9. doi:10.1038/nature03676. PMID 15917802. 1 Şubat 2020 tarihinde kaynağından arşivlendi (PDF)30 Haziran 2021.
Tsiganis, K. (2005). "Origin of the orbital architecture of the giant planets of the Solar System" (PDF). Nature. 435 (7041): 459-461. DOI:10.1038/nature03539. PMID 15917800. 8 Eylül 2020 tarihinde kaynağından arşivlendi (PDF). Erişim tarihi: 30 Haziran 2021.
Morbidelli, A. (2005). "Chaotic capture of Jupiter's Trojan asteroids in the early Solar System" (PDF). Nature. 435 (7041): 462-465. DOI:10.1038/nature03540. PMID 15917801. 21 Şubat 2014 tarihinde kaynağından (PDF) arşivlendi.
Levison, H. F. (2009). "Contamination of the asteroid belt by primordial trans-Neptunian objects". Nature. 460 (7253): 364-366. DOI:10.1038/nature08094. PMID 19606143.
Tsiganis (2005). "Origin of the orbital architecture of the giant planets of the Solar System" (PDF). Nature. 435 (7041): 459-461. doi:10.1038/nature03539. PMID 15917800. 8 Eylül 2020 tarihinde kaynağından arşivlendi (PDF)30 Haziran 2021.
Agnor (2006). "Neptune's capture of its moon Triton in a binary-planet gravitational encounter". Nature. 441 (7090): 192-194. doi:10.1038/nature04792. PMID 16688170.
Bottke (2012). "An Archaean heavy bombardment from a destabilized extension of the asteroid belt". Nature. 485 (7396): 78-81. doi:10.1038/nature10967. PMID 22535245.

oca.eu (Global: low place; Turkish: low place)

www-n.oca.eu

Tsiganis (2005). "Origin of the orbital architecture of the giant planets of the Solar System" (PDF). Nature. 435 (7041): 459-461. doi:10.1038/nature03539. PMID 15917800. 8 Eylül 2020 tarihinde kaynağından arşivlendi (PDF)30 Haziran 2021.

saturnaftercassini.org (Global: low place; Turkish: low place)

Turrini & Marzari, 2008, Phoebe and Saturn's irregular satellites: implications for the collisional capture scenario 3 Mart 2016 tarihinde Wayback Machine sitesinde arşivlendi.

web.archive.org (Global: 1^st place; Turkish: 1^st place)

R. Gomes (2005). "Origin of the cataclysmic Late Heavy Bombardment period of the terrestrial planets" (PDF). Nature. 435 (7041): 466-9. doi:10.1038/nature03676. PMID 15917802. 1 Şubat 2020 tarihinde kaynağından arşivlendi (PDF)30 Haziran 2021.
Turrini & Marzari, 2008, Phoebe and Saturn's irregular satellites: implications for the collisional capture scenario 3 Mart 2016 tarihinde Wayback Machine sitesinde arşivlendi.
Tsiganis (2005). "Origin of the orbital architecture of the giant planets of the Solar System" (PDF). Nature. 435 (7041): 459-461. doi:10.1038/nature03539. PMID 15917800. 8 Eylül 2020 tarihinde kaynağından arşivlendi (PDF)30 Haziran 2021.

Nice modeli (Turkish Wikipedia)

archive.org (Global: 6th place; Turkish: 4th place)

arxiv.org (Global: 49th place; Turkish: 78th place)

core.ac.uk (Global: 1,383rd place; Turkish: 489th place)

doi.org (Global: 2nd place; Turkish: 2nd place)