Levison, Harold F.; Morbidelli, Alessandro; Van Laerhoven, Christa i dr.. (2007). „Origin of the Structure of the Kuiper Belt during a Dynamical Instability in the Orbits of Uranus and Neptune”. Icarus196 (1): 258. arXiv:0712.0553. Bibcode2008Icar..196..258L. DOI:10.1016/j.icarus.2007.11.035.
Kuiper, Gerard P. (1950). „The Diameter of Pluto”. Publications of the Astronomical Society of the Pacific62 (366): 133–137. Bibcode1950PASP...62..133K. DOI:10.1086/126255.
Millis, Robert L.; Wasserman, Lawrence H.; Franz, Otto G. i dr.. (1993). „Pluto's radius and atmosphere – Results from the entire 9 June 1988 occultation data set”. Icarus105 (2): 282. Bibcode1993Icar..105..282M. DOI:10.1006/icar.1993.1126.
Young, Eliot F.; Binzel, Richard P. (1994). „A new determination of radii and limb parameters for Pluto and Charon from mutual event lightcurves”. Icarus108 (2): 219–224. Bibcode1994Icar..108..219Y. DOI:10.1006/icar.1994.1056.
Zalucha, Angela M.; Gulbis, Amanda A. S.; Zhu, Xun i dr.. (2011). „An analysis of Pluto occultation light curves using an atmospheric radiative-conductive model”. Icarus211 (1). Bibcode2011Icar..211..804Z. DOI:10.1016/j.icarus.2010.08.018.
Close, Laird M.; Merline, William J.; Tholen, David J. i dr.. (2000). „Adaptive optics imaging of Pluto–Charon and the discovery of a moon around the Asteroid 45 Eugenia: the potential of adaptive optics in planetary astronomy”. Proceedings of the International Society for Optical Engineering (European Southern Observatory) 4007: 787–795. Bibcode2000SPIE.4007..787C. DOI:10.1117/12.390379.
Lellouch, Emmanuel; Sicardy, Bruno; de Bergh, Catherine i dr.. (2009). „Pluto's lower atmosphere structure and methane abundance from high-resolution spectroscopy and stellar occultations”. Astronomy and Astrophysics495 (3): L17–L21. arXiv:0901.4882. Bibcode2009A&A...495L..17L. DOI:10.1051/0004-6361/200911633.
Showalter, M. R.; Hamilton, D. P. (3.6. 2015). „Resonant interactions and chaotic rotation of Pluto’s small moons”. Nature522 (7554): 45–49. Bibcode2015Natur.522...45S. DOI:10.1038/nature14469.
Levison, Harold F.; Morbidelli, Alessandro; Van Laerhoven, Christa i dr.. (2007). „Origin of the Structure of the Kuiper Belt during a Dynamical Instability in the Orbits of Uranus and Neptune”. Icarus196 (1): 258. arXiv:0712.0553. Bibcode2008Icar..196..258L. DOI:10.1016/j.icarus.2007.11.035.
Buchwald, Greg; Dimario, Michael; Wild, Walter (2000). „Pluto is Discovered Back in Time”. Amateur—Professional Partnerships in Astronomy (San Francisco: San Francisco: Astronomical Society of the Pacific) 220: 335. Bibcode2000ASPC..220..355B. ISBN1-58381-052-8.
Kuiper, Gerard P. (1950). „The Diameter of Pluto”. Publications of the Astronomical Society of the Pacific62 (366): 133–137. Bibcode1950PASP...62..133K. DOI:10.1086/126255.
Millis, Robert L.; Wasserman, Lawrence H.; Franz, Otto G. i dr.. (1993). „Pluto's radius and atmosphere – Results from the entire 9 June 1988 occultation data set”. Icarus105 (2): 282. Bibcode1993Icar..105..282M. DOI:10.1006/icar.1993.1126.
Young, Eliot F.; Binzel, Richard P. (1994). „A new determination of radii and limb parameters for Pluto and Charon from mutual event lightcurves”. Icarus108 (2): 219–224. Bibcode1994Icar..108..219Y. DOI:10.1006/icar.1994.1056.
Young, Eliot F.; Young, Leslie A.; Buie, Marc W. (2007). „Pluto's Radius”. American Astronomical Society, DPS meeting No. 39, #62.05; Bulletin of the American Astronomical Society39: 541. Bibcode2007DPS....39.6205Y.
Zalucha, Angela M.; Gulbis, Amanda A. S.; Zhu, Xun i dr.. (2011). „An analysis of Pluto occultation light curves using an atmospheric radiative-conductive model”. Icarus211 (1). Bibcode2011Icar..211..804Z. DOI:10.1016/j.icarus.2010.08.018.
Close, Laird M.; Merline, William J.; Tholen, David J. i dr.. (2000). „Adaptive optics imaging of Pluto–Charon and the discovery of a moon around the Asteroid 45 Eugenia: the potential of adaptive optics in planetary astronomy”. Proceedings of the International Society for Optical Engineering (European Southern Observatory) 4007: 787–795. Bibcode2000SPIE.4007..787C. DOI:10.1117/12.390379.
Lellouch, Emmanuel; Sicardy, Bruno; de Bergh, Catherine i dr.. (2009). „Pluto's lower atmosphere structure and methane abundance from high-resolution spectroscopy and stellar occultations”. Astronomy and Astrophysics495 (3): L17–L21. arXiv:0901.4882. Bibcode2009A&A...495L..17L. DOI:10.1051/0004-6361/200911633.
Showalter, M. R.; Hamilton, D. P. (3.6. 2015). „Resonant interactions and chaotic rotation of Pluto’s small moons”. Nature522 (7554): 45–49. Bibcode2015Natur.522...45S. DOI:10.1038/nature14469.
Levison, Harold F.; Morbidelli, Alessandro; Van Laerhoven, Christa i dr.. (2007). „Origin of the Structure of the Kuiper Belt during a Dynamical Instability in the Orbits of Uranus and Neptune”. Icarus196 (1): 258. arXiv:0712.0553. Bibcode2008Icar..196..258L. DOI:10.1016/j.icarus.2007.11.035.
Young, Eliot F.; Binzel, Richard P.; Crane, Keenan (2000). „A Two-Color Map of Pluto Based on Mutual Event Lightcurves”. Bulletin of the American Astronomical Society (AA(SwRI), AB(M.I.T.), AC (Boulder High School)) 32: 1083. Bibcode2000DPS....32.4601Y.
„Pluto's still the same Pluto”. Independent Newspapers. Associated Press. 21 October 2006. Pristupljeno 29 November 2011. »Mickey Mouse has a cute dog.«
jhuapl.edu
pluto.jhuapl.edu
„The Inside Story”. pluto.jhuapl.edu – NASA New Horizons mission site. Johns Hopkins University Applied Physics Laboratory. 2007. Arhivirano iz originala na datum 2018-10-05. Pristupljeno 15 February 2014.
„Colossal Cousin to a Comet?”. pluto.jhuapl.edu – NASA New Horizons mission site. Johns Hopkins University Applied Physics Laboratory. Arhivirano iz originala na datum 2014-11-13. Pristupljeno 15 February 2014.
otkriće Harona 1978. dozvolilo je astronomima da točno izmjere masu plutonskog sustava. Ali to nije ukazivalo na individualnu masu tih dvaju tijela, koja su procijenjena tek nakon otkrića ostalih Plutonovih mjeseca 2005. Zbog toga, jer je Pluton ušao u perihel 1989, većina procjena se temeljilo na težištu Pluton-Haron. Haron je ušau u perihel 4.9. 1989. Težište Pluton–Haron je ušlo u perihel 5.9. 1989. Pluton je ušao u perihel 8.9. 1989.
„Name Pluto Given to Body Believed to Be Planet X”. The New York Times. Associated Press: str. 1. 25 May 1930. ISSN0362-4331. »Pluto, the title of the Roman gods of the region of darkness, was announced tonight at Lowell Observatory here as the name chosen for the recently discovered trans-Neptunian body, which is believed to be the long-sought Planet X.«
Heinrichs, Allison M. (2006). „Dwarfed by comparison”. Pittsburgh Tribune-Review. Arhivirano iz originala na datum 2009-09-02. Pristupljeno 26 March 2007.
Heinrichs, Allison M. (2006). „Dwarfed by comparison”. Pittsburgh Tribune-Review. Arhivirano iz originala na datum 2009-09-02. Pristupljeno 26 March 2007.
„The Inside Story”. pluto.jhuapl.edu – NASA New Horizons mission site. Johns Hopkins University Applied Physics Laboratory. 2007. Arhivirano iz originala na datum 2018-10-05. Pristupljeno 15 February 2014.
„Colossal Cousin to a Comet?”. pluto.jhuapl.edu – NASA New Horizons mission site. Johns Hopkins University Applied Physics Laboratory. Arhivirano iz originala na datum 2014-11-13. Pristupljeno 15 February 2014.
„Name Pluto Given to Body Believed to Be Planet X”. The New York Times. Associated Press: str. 1. 25 May 1930. ISSN0362-4331. »Pluto, the title of the Roman gods of the region of darkness, was announced tonight at Lowell Observatory here as the name chosen for the recently discovered trans-Neptunian body, which is believed to be the long-sought Planet X.«