(2) Pallas (Polish Wikipedia)

Analysis of information sources in references of the Wikipedia article "(2) Pallas" in Polish language version.

refsWebsite

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21web.archive.org

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18harvard.edu

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12doi.org

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7nasa.gov

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3psi.edu

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2usra.edu

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1springerlink.com

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1ucla.edu

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1spacefiles.blogspot.com

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1planetary.org

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1britannica.com

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1southastrodel.com

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1ueuo.com

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1lanl.gov

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1unipa.it

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1navy.mil

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1cas.cz

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1astrosurf.com

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1johnstonsarchive.net

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1jas.org.jo

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1iau.org

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1bbc.co.uk

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1eso.org

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astrosurf.com

Gérard Faure: Description of the System of Asteroids. Astrosurf.com, 2004-05-20. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2014-07-19)].

bbc.co.uk

news.bbc.co.uk

Paul Rincon: Planets plan boosts tally to 12. BBC News, 2006-08-16. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2013-12-28)].

britannica.com

Pallas, [w:] Encyclopædia Britannica [dostęp 2014-08-19] (ang.).

cas.cz

astro.cas.cz

O. Gingerich: The Path to Defining Planets. [w:] Harvard-Smithsonian Center for Astrophysics and IAU EC Planet Definition Committee chair [on-line]. 2006. [dostęp 2014-07-18]. [zarchiwizowane z tego adresu (2007-03-06)].

doi.org

James Baer, Steven R. Chesley. Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris. „Celestial Mechanics and Dynamical Astronomy”. 100 (2008), s. 27–42, 2008. Springer Science+Business Media B.V. 2007. DOI: 10.1007/s10569-007-9103-8. Bibcode: 2008CeMDA.100...27B. [dostęp 2014-08-19]. [zarchiwizowane z adresu 2011-02-24].
K.J. Johnston, P.K. Seidelmann, C.M. Wade. Observations of 1 Ceres and 2 Pallas at centimeter wavelengths. „The Astronomical Journal”. 87 (11), listopad 1982. DOI: 10.1086/113249. Bibcode: 1982AJ.....87.1593J.
E.V. Pitjeva. High-Precision Ephemerides of Planets–EPM and Determination of Some Astronomical Constants. „Solar System Research”. 39 (3), s. 176, 2005. DOI: 10.1007/s11208-005-0033-2. Bibcode: 2005SoSyR..39..176P.
Benjamin Apthorp Gould. On the symbolic notation of the asteroids. „Astronomical Journal”. 2 (34), s. 80, 1852. DOI: 10.1086/100212. Bibcode: 1852AJ......2...80G.
Drummond, J.D., Cocke, W.J. Triaxial ellipsoid dimensions and rotational pole of 2 Pallas from two stellar occultations. „Icarus”. 78 (2), s. 323–329, 1989. DOI: 10.1016/0019-1035(89)90180-2. Bibcode: 1989Icar...78..323D.
Dunham, D.W. et al.. The size and shape of (2) Pallas from the 1983 occultation of 1 Vulpeculae. „Astronomical Journal”. 99, s. 1636–1662, 1990. DOI: 10.1086/115446. Bibcode: 1990AJ.....99.1636D.
Sato, Kimiyasu; Miyamoto, Masamichi; Zolensky, Michael E. Absorption bands near 3 m.in. diffuse reflectance spectra of carbonaceous chondrites: Comparison with asteroids. „Meteoritics”. 32 (4), s. 503–507, 1997. DOI: 10.1111/j.1945-5100.1997.tb01295.x. Bibcode: 1997M&PS...32..503S.
McCord, T.B.; McFadden, L.A.; Russell, C.T.; Sotin, C.; Thomas, P.C.. Ceres, Vesta, and Pallas: Protoplanets, Not Asteroids. „Transactions of the American Geophysical Union”. 87 (10), s. 105, 2006. DOI: 10.1029/2006EO100002. Bibcode: 2006EOSTr..87..105M.
Gonzalo Tancredi, Sofía Favre. Which are the dwarfs in the Solar System?. „Icarus”. 195 (2), s. 851–862, 2008. DOI: 10.1016/j.icarus.2007.12.020.
Torppa, J.; et al.. Shapes and rotational properties of thirty asteroids from photometric data. „Icarus”. 164 (2), s. 346–383, 2003. DOI: 10.1016/S0019-1035(03)00146-5. Bibcode: 2003Icar..164..346T.
E. Goffin. New determination of the mass of Pallas. „Astronomy and Astrophysics”. 365 (3), s. 627–630, 2001. DOI: 10.1051/0004-6361:20000023. Bibcode: 2001A&A...365..627G.
Ettore Perozzi, Alessandro Rossi, Giovanni B. Valsecchi. Basic targeting strategies for rendezvous and flyby missions to the near-Earth asteroids. „Planetary and Space Science”. 49 (1), s. 3–22, 2001. DOI: 10.1016/S0032-0633(00)00124-0. Bibcode: 2001P&SS...49....3P.

eso.org

Carry, B. et al.: Asteroid 2 Pallas Physical Properties from Near-Infrared High-Angular Resolution Imagery. 2007. [dostęp 2014-08-19].

harvard.edu

adsabs.harvard.edu

James Baer, Steven R. Chesley. Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris. „Celestial Mechanics and Dynamical Astronomy”. 100 (2008), s. 27–42, 2008. Springer Science+Business Media B.V. 2007. DOI: 10.1007/s10569-007-9103-8. Bibcode: 2008CeMDA.100...27B. [dostęp 2014-08-19]. [zarchiwizowane z adresu 2011-02-24].
B.E. Schmidt, P.C. Thomas, J.M. Bauer, J.-Y. Li i inni. Hubble takes a look at Pallas: Shape, size, and surface. „39th Lunar and Planetary Science Conference”. 1391, s. 2502, 10–14.03.2008. League City, Texas.. Bibcode: 2008LPI....39.2502S. [dostęp 2014-08-19]. [zarchiwizowane z adresu 2008-10-04].
K.J. Johnston, P.K. Seidelmann, C.M. Wade. Observations of 1 Ceres and 2 Pallas at centimeter wavelengths. „The Astronomical Journal”. 87 (11), listopad 1982. DOI: 10.1086/113249. Bibcode: 1982AJ.....87.1593J.
E.V. Pitjeva. High-Precision Ephemerides of Planets–EPM and Determination of Some Astronomical Constants. „Solar System Research”. 39 (3), s. 176, 2005. DOI: 10.1007/s11208-005-0033-2. Bibcode: 2005SoSyR..39..176P.
Benjamin Apthorp Gould. On the symbolic notation of the asteroids. „Astronomical Journal”. 2 (34), s. 80, 1852. DOI: 10.1086/100212. Bibcode: 1852AJ......2...80G.
Eric G. Forbes. Gauss and the Discovery of Ceres. „Journal for the History of Astronomy”. 2, s. 195–199, 1971. Bibcode: 1971JHA.....2..195F.
Yoshihide Kozai. Kiyotsugu Hirayama and His Families of Asteroids (invited). „Proceedings of the International Conference”, 29 listopada – 3 grudnia 1993. Sagamihara, Japan: Astronomical Society of the Pacific. Bibcode: 1994ASPC...63....1K.
Foglia, S., Masi, G. New clusters for highly inclined main-belt asteroids. „The Minor Planet Bulletin”. 31, s. 100–102, 1999. Bibcode: 2004MPBu...31..100F. [dostęp 2014-08-19].
Drummond, J.D., Cocke, W.J. Triaxial ellipsoid dimensions and rotational pole of 2 Pallas from two stellar occultations. „Icarus”. 78 (2), s. 323–329, 1989. DOI: 10.1016/0019-1035(89)90180-2. Bibcode: 1989Icar...78..323D.
Dunham, D.W. et al.. The size and shape of (2) Pallas from the 1983 occultation of 1 Vulpeculae. „Astronomical Journal”. 99, s. 1636–1662, 1990. DOI: 10.1086/115446. Bibcode: 1990AJ.....99.1636D.
E.V. Pitjeva. Estimations of masses of the largest asteroids and the main asteroid belt from ranging to planets, Mars orbiters and landers. „35th COSPAR Scientific Assembly”, s. 2014, 18–25 czerwca 2004. Paryż. Bibcode: 2004cosp...35.2014P.
Feierberg, M.A., Larson, H.P., Lebofsky, L.A. The 3 Micron Spectrum of Asteroid 2 Pallas. „Bulletin of the American Astronomical Society”. 14, s. 719, 1982. Bibcode: 1982BAAS...14..719F.
Sato, Kimiyasu; Miyamoto, Masamichi; Zolensky, Michael E. Absorption bands near 3 m.in. diffuse reflectance spectra of carbonaceous chondrites: Comparison with asteroids. „Meteoritics”. 32 (4), s. 503–507, 1997. DOI: 10.1111/j.1945-5100.1997.tb01295.x. Bibcode: 1997M&PS...32..503S.
McCord, T.B.; McFadden, L.A.; Russell, C.T.; Sotin, C.; Thomas, P.C.. Ceres, Vesta, and Pallas: Protoplanets, Not Asteroids. „Transactions of the American Geophysical Union”. 87 (10), s. 105, 2006. DOI: 10.1029/2006EO100002. Bibcode: 2006EOSTr..87..105M.
Torppa, J.; et al.. Shapes and rotational properties of thirty asteroids from photometric data. „Icarus”. 164 (2), s. 346–383, 2003. DOI: 10.1016/S0019-1035(03)00146-5. Bibcode: 2003Icar..164..346T.
E. Goffin. New determination of the mass of Pallas. „Astronomy and Astrophysics”. 365 (3), s. 627–630, 2001. DOI: 10.1051/0004-6361:20000023. Bibcode: 2001A&A...365..627G.
D.B. Taylor. The secular motion of Pallas. „Royal Astronomical Society”. 199, s. 255–265, 1982. Bibcode: 1982MNRAS.199..255T.
Ettore Perozzi, Alessandro Rossi, Giovanni B. Valsecchi. Basic targeting strategies for rendezvous and flyby missions to the near-Earth asteroids. „Planetary and Space Science”. 49 (1), s. 3–22, 2001. DOI: 10.1016/S0032-0633(00)00124-0. Bibcode: 2001P&SS...49....3P.

iau.org

IAU 2006 General Assembly: Result of the IAU Resolution votes. IAU. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2009-07-13)].

jas.org.jo

Moh’d Odeh: The Brightest Asteroids. Jordanian Astronomical Society, 2014-06-11. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2015-11-17)].

johnstonsarchive.net

William Robert Johnston: Other Reports of Asteroid/TNO Companions. Johnson’s Archive, 2007-03-05. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2014-07-18)].

lanl.gov

periodic.lanl.gov

Palladium. Los Alamos National Laboratory. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2014-07-25)].

nasa.gov

dawn.jpl.nasa.gov

Chris Russell, Lucy McFadden, Joe Wise lub Marc Rayman: Dawn mission FAQs. JPL, 2011. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2014-11-12)]. Cytat: It is impossible to reach with a mission in the same class as Dawn because it takes too much thrust to reach Pallas. Pallas is highly inclined to the ecliptic plane. A lot of energy is needed to climb out of the ecliptic plane especially as far out of the plane as Pallas is. I did try to design a mission to reach Pallas and it was impossible with the Dawn spacecraft even if we went nowhere else than Pallas.
Dawn Classrooms > Biographies. Dawn Mission (NASA/JPL). [dostęp 2014-09-03].
Flashbacks > Astronomical Serendipity. Dawn Mission (NASA/JPL). [dostęp 2014-08-19].

ssd.jpl.nasa.gov

(2) Pallas w bazie Jet Propulsion Laboratory (ang.) [dostęp 2024-12-29]
Obliczone z użyciem JPL Horizons dla 1608-02-15.

iau-comm4.jpl.nasa.gov

E.V. Pitjeva. High-Precision Ephemerides of Planets–EPM and Determination of Some Astronomical Constants. „Solar System Research”. 39 (3), s. 176, 2005. DOI: 10.1007/s11208-005-0033-2. Bibcode: 2005SoSyR..39..176P.

nasa.gov

Hubble Images of Asteroids Help Astronomers Prepare for Spacecraft Visit. JPL/NASA, 2007-06-20. [dostęp 2014-08-19].

navy.mil

aa.usno.navy.mil

James L. Hilton: When did asteroids become minor planets?. [w:] U.S. Naval Observatory [on-line]. 2007-11-16. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2016-06-12)].

planetary.org

Notable Asteroids. The Planetary Society, 2007. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2012-02-07)].

psi.edu

Harris, A.W.; Warner, B.D.; Pravec, P. (red.): Lightcurve Derived Data. NASA Planetary Data System, 2014-03-01. [dostęp 2014-08-19]. (wersja 14.0).
E.F. Tedesco, Noah, P.V.; Noah, M.; Price, S.D: IRAS Minor Planet Survey. IRAS-A-FPA-3-RDR-IMPS-V6.0.. NASA Planetary Data System, 2004. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2009-08-17)].
C. Neese: Asteroid Taxonomy. EAR-A-5-DDR-Taxonomy-V5.0.. NASA Planetary Data System, 2005. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2013-10-21)].

southastrodel.com

Andrew James: Pallas. [w:] Southern Astronomical Delights [on-line]. 2008-09-02. [dostęp 2014-08-19].

spacefiles.blogspot.com

Anonymous: Pre-Dawn: The French-Soviet VESTA mission. Space Files, 2007-11-05. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2012-02-13)].

springerlink.com

James Baer, Steven R. Chesley. Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris. „Celestial Mechanics and Dynamical Astronomy”. 100 (2008), s. 27–42, 2008. Springer Science+Business Media B.V. 2007. DOI: 10.1007/s10569-007-9103-8. Bibcode: 2008CeMDA.100...27B. [dostęp 2014-08-19]. [zarchiwizowane z adresu 2011-02-24].

ucla.edu

newsroom.ucla.edu

Mona Gable: Study of first high-resolution images of Pallas confirms asteroid is actually a protoplanet. University of California, Los Angeles (UCLA). [dostęp 2014-08-19].

ueuo.com

katsba.ueuo.com

Αστεροειδείς. [dostęp 2014-09-12]. (gr.).

unipa.it

astropa.unipa.it

Michael Hoskin: Bode’s Law and the Discovery of Ceres. Observatorio Astronomico di Palermo „Giuseppe S. Vaiana”, 1992-06-26. [dostęp 2014-08-19].

usra.edu

lpi.usra.edu

B.E. Schmidt, P.C. Thomas, J.M. Bauer, J.-Y. Li i inni. Hubble takes a look at Pallas: Shape, size, and surface. „39th Lunar and Planetary Science Conference”. 1391, s. 2502, 10–14.03.2008. League City, Texas.. Bibcode: 2008LPI....39.2502S. [dostęp 2014-08-19]. [zarchiwizowane z adresu 2008-10-04].
James L. Hilton: Asteroid Masses and Densities. [w:] U.S. Naval Observatory [on-line]. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2008-08-19)].

web.archive.org

Chris Russell, Lucy McFadden, Joe Wise lub Marc Rayman: Dawn mission FAQs. JPL, 2011. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2014-11-12)]. Cytat: It is impossible to reach with a mission in the same class as Dawn because it takes too much thrust to reach Pallas. Pallas is highly inclined to the ecliptic plane. A lot of energy is needed to climb out of the ecliptic plane especially as far out of the plane as Pallas is. I did try to design a mission to reach Pallas and it was impossible with the Dawn spacecraft even if we went nowhere else than Pallas.
James Baer, Steven R. Chesley. Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris. „Celestial Mechanics and Dynamical Astronomy”. 100 (2008), s. 27–42, 2008. Springer Science+Business Media B.V. 2007. DOI: 10.1007/s10569-007-9103-8. Bibcode: 2008CeMDA.100...27B. [dostęp 2014-08-19]. [zarchiwizowane z adresu 2011-02-24].
B.E. Schmidt, P.C. Thomas, J.M. Bauer, J.-Y. Li i inni. Hubble takes a look at Pallas: Shape, size, and surface. „39th Lunar and Planetary Science Conference”. 1391, s. 2502, 10–14.03.2008. League City, Texas.. Bibcode: 2008LPI....39.2502S. [dostęp 2014-08-19]. [zarchiwizowane z adresu 2008-10-04].
E.F. Tedesco, Noah, P.V.; Noah, M.; Price, S.D: IRAS Minor Planet Survey. IRAS-A-FPA-3-RDR-IMPS-V6.0.. NASA Planetary Data System, 2004. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2009-08-17)].
C. Neese: Asteroid Taxonomy. EAR-A-5-DDR-Taxonomy-V5.0.. NASA Planetary Data System, 2005. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2013-10-21)].
Anonymous: Pre-Dawn: The French-Soviet VESTA mission. Space Files, 2007-11-05. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2012-02-13)].
Notable Asteroids. The Planetary Society, 2007. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2012-02-07)].
Palladium. Los Alamos National Laboratory. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2014-07-25)].
James L. Hilton: When did asteroids become minor planets?. [w:] U.S. Naval Observatory [on-line]. 2007-11-16. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2016-06-12)].
James L. Hilton: Asteroid Masses and Densities. [w:] U.S. Naval Observatory [on-line]. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2008-08-19)].
O. Gingerich: The Path to Defining Planets. [w:] Harvard-Smithsonian Center for Astrophysics and IAU EC Planet Definition Committee chair [on-line]. 2006. [dostęp 2014-07-18]. [zarchiwizowane z tego adresu (2007-03-06)].
Gérard Faure: Description of the System of Asteroids. Astrosurf.com, 2004-05-20. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2014-07-19)].
Foglia, S., Masi, G. New clusters for highly inclined main-belt asteroids. „The Minor Planet Bulletin”. 31, s. 100–102, 1999. Bibcode: 2004MPBu...31..100F. [dostęp 2014-08-19].
William Robert Johnston: Other Reports of Asteroid/TNO Companions. Johnson’s Archive, 2007-03-05. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2014-07-18)].
D.R. Williams: Moon Fact Sheet. NASA, 2014-04-25. [dostęp 2014-09-05].
Moh’d Odeh: The Brightest Asteroids. Jordanian Astronomical Society, 2014-06-11. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2015-11-17)].
Earliest Meteorites Provide New Piece in Planetary Formation Puzzle. Particle Physics and Astronomy Research Council, 2005-09-20. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2013-05-06)].
IAU 2006 General Assembly: Result of the IAU Resolution votes. IAU. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2009-07-13)].
Paul Rincon: Planets plan boosts tally to 12. BBC News, 2006-08-16. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2013-12-28)].
The MeanPlane (Invariable plane) of the Solar System passing through the barycenter. 2009-04-03. [dostęp 2014-08-19]. [zarchiwizowane z tego adresu (2013-10-28)]. (obliczono z użyciem Solex 10 autorstwa Aldo Vitagliano).
Obliczone z użyciem programu Solex: Aldo Vitagliano: Solex. [dostęp 2009-03-19].