Tihe (hipotetski planet) (Croatian Wikipedia)

Analysis of information sources in references of the Wikipedia article "Tihe (hipotetski planet)" in Croatian language version.

refsWebsite

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8harvard.edu

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7doi.org

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4semanticscholar.org

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4nasa.gov

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3louisiana.edu

low place

3web.archive.org

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3arxiv.org

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1independent.co.uk

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1space.com

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1dailyvoice.com

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1archive.org

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1chron.com

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1discovermagazine.com

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1calctool.org

low place

1ultoday.com

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1forbes.com

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1arstechnica.com

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1ucla.edu

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archive.org

Harold F. Levison; Luke Donnes. 2007. Comet Populations and Cometary Dynamics. Lucy Ann Adams McFadden; Lucy-Ann Adams; Paul Robert Weissman; Torrence V. Johnson (ur.). Encyclopedia of the Solar System. 2nd izdanje. Academic Press. Amsterdam; Boston. str. 575–588. ISBN 978-0-12-088589-3

arstechnica.com

Sayanagi, Kunio M. 2. ožujka 2011. Where is Tyche, the ~~10th~~ 9th planet? Getting the full story. ArsTechnica. Pristupljeno 21. ožujka 2011.

arxiv.org

Matese, John J.; Whitmire, Daniel P. 2011. Persistent Evidence of a Jovian Mass Solar Companion in the Oort Cloud. Icarus. 211 (2): 926–938. arXiv:1004.4584. Bibcode:2011Icar..211..926M. doi:10.1016/j.icarus.2010.11.009. S2CID 44204219
Seager, S.; Kuchner, M.; Hier-Majumder, C. A.; Militzer, B. 2007. Mass-Radius Relationships for Solid Exoplanets. The Astrophysical Journal. 669 (2): 1279–1297. arXiv:0707.2895. Bibcode:2007ApJ...669.1279S. doi:10.1086/521346. S2CID 8369390 Referenca navodi 500 masa zemlje, (1.6 masa Jupitera). Jupiter ima masu 318 puta veću od zemljine.
Spiegel, David S.; Burrows, Adam; Milson, John A. 2011. The Deuterium-Burning Mass Limit for Brown Dwarfs and Giant Planets. The Astrophysical Journal. 727 (1): 57. arXiv:1008.5150. Bibcode:2011ApJ...727...57S. doi:10.1088/0004-637X/727/1/57. S2CID 118513110

calctool.org

Orbital period of a planet at a distance of 15000 AU with a circular orbit. Pristupljeno 15. veljače 2011.

chron.com

Murray, John B. 1999. Arguments for the Presence of a Distant Large Undiscovered Solar System Planet. Monthly Notices of the Royal Astronomical Society. 309 (1): 31–34. Bibcode:1999MNRAS.309...31M. doi:10.1046/j.1365-8711.1999.02806.x. Sažetak – Houston Chronicle11. listopada 1999.

dailyvoice.com

norwalk.dailyvoice.com

Helhoski, Anna. News 02/16/11 Does the Solar System Have Giant New Planet?. The Norwalk Daily Voice. Pristupljeno 10. srpnja 2012.

discovermagazine.com

blogs.discovermagazine.com

Plait, Phil. 14. veljače 2011. No, there's no proof of a giant planet in the outer Solar System. Discovery Magazine. Inačica izvorne stranice arhivirana 16. travnja 2016. Pristupljeno 15. veljače 2011.

doi.org

Murray, John B. 1999. Arguments for the Presence of a Distant Large Undiscovered Solar System Planet. Monthly Notices of the Royal Astronomical Society. 309 (1): 31–34. Bibcode:1999MNRAS.309...31M. doi:10.1046/j.1365-8711.1999.02806.x. Sažetak – Houston Chronicle11. listopada 1999.
Matese, John J.; Whitman, Patrick G.; Whitmire, Daniel P . 1999. Cometary Evidence of a Massive Body in the Outer Oort Clouds. Icarus. 141 (2): 354. Bibcode:1999Icar..141..354M. doi:10.1006/icar.1999.6177
Matese, John J.; Whitmire, Daniel P.; Lissauer, Jack J. 2006. A Widebinary Solar Companion as a Possible Origin of Sedna-like Objects. Earth, Moon, and Planets. 97 (3–4): 459–470. Bibcode:2005EM&P...97..459M. doi:10.1007/s11038-006-9078-6. S2CID 13647204
Matese, John J.; Whitmire, Daniel P. 2011. Persistent Evidence of a Jovian Mass Solar Companion in the Oort Cloud. Icarus. 211 (2): 926–938. arXiv:1004.4584. Bibcode:2011Icar..211..926M. doi:10.1016/j.icarus.2010.11.009. S2CID 44204219
Seager, S.; Kuchner, M.; Hier-Majumder, C. A.; Militzer, B. 2007. Mass-Radius Relationships for Solid Exoplanets. The Astrophysical Journal. 669 (2): 1279–1297. arXiv:0707.2895. Bibcode:2007ApJ...669.1279S. doi:10.1086/521346. S2CID 8369390 Referenca navodi 500 masa zemlje, (1.6 masa Jupitera). Jupiter ima masu 318 puta veću od zemljine.
Spiegel, David S.; Burrows, Adam; Milson, John A. 2011. The Deuterium-Burning Mass Limit for Brown Dwarfs and Giant Planets. The Astrophysical Journal. 727 (1): 57. arXiv:1008.5150. Bibcode:2011ApJ...727...57S. doi:10.1088/0004-637X/727/1/57. S2CID 118513110
Luhman, K. L. 2014. A Search for a Distant Companion to the Sun with the Wide-field Infrared Survey Explorer. The Astrophysical Journal. 781 (1): 4. Bibcode:2014ApJ...781....4L. doi:10.1088/0004-637X/781/1/4

forbes.com

Bruce Dorminey. 31. ožujka 2013. Sun May Still Have Low-Mass Solar Companion, Say Astrophysicists Searching NASA WISE Mission Data. Forbes. Pristupljeno 1. travnja 2013.

harvard.edu

ui.adsabs.harvard.edu

Matese, John J.; Lissauer, Jack J. 6. svibnja 2002. Continuing Evidence of an Impulsive Component of Oort Cloud Cometary Flux (PDF). University of Louisiana at Lafayette, and NASA Ames Research Center. 500: 309. Bibcode:2002ESASP.500..309M. Pristupljeno 21. ožujka 2008.
Murray, John B. 1999. Arguments for the Presence of a Distant Large Undiscovered Solar System Planet. Monthly Notices of the Royal Astronomical Society. 309 (1): 31–34. Bibcode:1999MNRAS.309...31M. doi:10.1046/j.1365-8711.1999.02806.x. Sažetak – Houston Chronicle11. listopada 1999.
Matese, John J.; Whitman, Patrick G.; Whitmire, Daniel P . 1999. Cometary Evidence of a Massive Body in the Outer Oort Clouds. Icarus. 141 (2): 354. Bibcode:1999Icar..141..354M. doi:10.1006/icar.1999.6177
Matese, John J.; Whitmire, Daniel P.; Lissauer, Jack J. 2006. A Widebinary Solar Companion as a Possible Origin of Sedna-like Objects. Earth, Moon, and Planets. 97 (3–4): 459–470. Bibcode:2005EM&P...97..459M. doi:10.1007/s11038-006-9078-6. S2CID 13647204
Matese, John J.; Whitmire, Daniel P. 2011. Persistent Evidence of a Jovian Mass Solar Companion in the Oort Cloud. Icarus. 211 (2): 926–938. arXiv:1004.4584. Bibcode:2011Icar..211..926M. doi:10.1016/j.icarus.2010.11.009. S2CID 44204219
Seager, S.; Kuchner, M.; Hier-Majumder, C. A.; Militzer, B. 2007. Mass-Radius Relationships for Solid Exoplanets. The Astrophysical Journal. 669 (2): 1279–1297. arXiv:0707.2895. Bibcode:2007ApJ...669.1279S. doi:10.1086/521346. S2CID 8369390 Referenca navodi 500 masa zemlje, (1.6 masa Jupitera). Jupiter ima masu 318 puta veću od zemljine.
Spiegel, David S.; Burrows, Adam; Milson, John A. 2011. The Deuterium-Burning Mass Limit for Brown Dwarfs and Giant Planets. The Astrophysical Journal. 727 (1): 57. arXiv:1008.5150. Bibcode:2011ApJ...727...57S. doi:10.1088/0004-637X/727/1/57. S2CID 118513110
Luhman, K. L. 2014. A Search for a Distant Companion to the Sun with the Wide-field Infrared Survey Explorer. The Astrophysical Journal. 781 (1): 4. Bibcode:2014ApJ...781....4L. doi:10.1088/0004-637X/781/1/4

independent.co.uk

Rodgers, Paul. 13. veljače 2011. Up telescope! Search begins for giant new planet. The Independent. Pristupljeno 14. veljače 2011.

louisiana.edu

ucs.louisiana.edu

Astrophysics Homepage of John J. Matese. Ucs.louisiana.edu. 21. rujna 2011. Pristupljeno 1. travnja 2013.
Daniel P. Whitmire. Ucs.louisiana.edu. Pristupljeno 1. travnja 2013.
Matese, John J.; Lissauer, Jack J. 6. svibnja 2002. Continuing Evidence of an Impulsive Component of Oort Cloud Cometary Flux (PDF). University of Louisiana at Lafayette, and NASA Ames Research Center. 500: 309. Bibcode:2002ESASP.500..309M. Pristupljeno 21. ožujka 2008.

nasa.gov

jpl.nasa.gov

Whitney Clavin. 18. veljače 2011. Can WISE Find the Hypothetical 'Tyche'?. NASA/JPL. Pristupljeno 19. veljače 2011.
NASA Releases New WISE Mission Catalog of Entire Infrared Sky. NASA/JPL. 14. ožujka 2012. Inačica izvorne stranice arhivirana 4. lipnja 2012. Pristupljeno 15. ožujka 2012.
Clavin, Whitney; Harrington, J.D. 7. ožujka 2014. NASA's WISE Survey Finds Thousands of New Stars, But No 'Planet X'. NASA. Pristupljeno 7. ožujka 2014.

nssdc.gsfc.nasa.gov

Seager, S.; Kuchner, M.; Hier-Majumder, C. A.; Militzer, B. 2007. Mass-Radius Relationships for Solid Exoplanets. The Astrophysical Journal. 669 (2): 1279–1297. arXiv:0707.2895. Bibcode:2007ApJ...669.1279S. doi:10.1086/521346. S2CID 8369390 Referenca navodi 500 masa zemlje, (1.6 masa Jupitera). Jupiter ima masu 318 puta veću od zemljine.

semanticscholar.org

api.semanticscholar.org

Matese, John J.; Whitmire, Daniel P.; Lissauer, Jack J. 2006. A Widebinary Solar Companion as a Possible Origin of Sedna-like Objects. Earth, Moon, and Planets. 97 (3–4): 459–470. Bibcode:2005EM&P...97..459M. doi:10.1007/s11038-006-9078-6. S2CID 13647204
Matese, John J.; Whitmire, Daniel P. 2011. Persistent Evidence of a Jovian Mass Solar Companion in the Oort Cloud. Icarus. 211 (2): 926–938. arXiv:1004.4584. Bibcode:2011Icar..211..926M. doi:10.1016/j.icarus.2010.11.009. S2CID 44204219
Seager, S.; Kuchner, M.; Hier-Majumder, C. A.; Militzer, B. 2007. Mass-Radius Relationships for Solid Exoplanets. The Astrophysical Journal. 669 (2): 1279–1297. arXiv:0707.2895. Bibcode:2007ApJ...669.1279S. doi:10.1086/521346. S2CID 8369390 Referenca navodi 500 masa zemlje, (1.6 masa Jupitera). Jupiter ima masu 318 puta veću od zemljine.
Spiegel, David S.; Burrows, Adam; Milson, John A. 2011. The Deuterium-Burning Mass Limit for Brown Dwarfs and Giant Planets. The Astrophysical Journal. 727 (1): 57. arXiv:1008.5150. Bibcode:2011ApJ...727...57S. doi:10.1088/0004-637X/727/1/57. S2CID 118513110

space.com

Wolchover, Natalie. 15. veljače 2011. Article: Astronomers Doubt Giant Planet 'Tyche' Exists in Our Solar System. Space.com. Pristupljeno 15. veljače 2011.

ucla.edu

astro.ucla.edu

Wide-field Infrared Survey Explorer

ultoday.com

Have UL Physicists Identified a New Planet?. University of Louisiana. 14. veljače 2011. Inačica izvorne stranice arhivirana 1. kolovoza 2015. Pristupljeno 16. veljače 2011.

web.archive.org

Plait, Phil. 14. veljače 2011. No, there's no proof of a giant planet in the outer Solar System. Discovery Magazine. Inačica izvorne stranice arhivirana 16. travnja 2016. Pristupljeno 15. veljače 2011.
Have UL Physicists Identified a New Planet?. University of Louisiana. 14. veljače 2011. Inačica izvorne stranice arhivirana 1. kolovoza 2015. Pristupljeno 16. veljače 2011.
NASA Releases New WISE Mission Catalog of Entire Infrared Sky. NASA/JPL. 14. ožujka 2012. Inačica izvorne stranice arhivirana 4. lipnja 2012. Pristupljeno 15. ožujka 2012.