Geology of Venus (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "Geology of Venus" in English language version.

refsWebsite

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21doi.org

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13harvard.edu

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9semanticscholar.org

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3worldcat.org

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2archive.today

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2wolframalpha.com

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2brown.edu

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1nytimes.com

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1nature.com

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archive.today

Chang, Kenneth (26 October 2023). "Billions of Years Ago, Venus May Have Had a Key Earthlike Feature - A new study makes the case that the solar system's hellish second planet once may have had plate tectonics that could have made it more hospitable to life". The New York Times. Archived from the original on 26 October 2023. Retrieved 27 October 2023.
Weller, Matthew B.; et al. (26 October 2023). "Venus's atmospheric nitrogen explained by ancient plate tectonics". Nature Astronomy. doi:10.1038/s41550-023-02102-w. Archived from the original on 27 October 2023. Retrieved 27 October 2023.

arxiv.org

Michael J. Way; et al. (26 August 2016). "Was Venus the First Habitable World of our Solar System?". Geophysical Research Letters. 43 (16): 8376–8383. arXiv:1608.00706. Bibcode:2016GeoRL..43.8376W. doi:10.1002/2016GL069790. PMC 5385710. PMID 28408771.

brown.edu

porter.geo.brown.edu

Basilevsky, A. T.; J. W. Head III (2003). "The surface of Venus" (PDF). Reports on Progress in Physics. 66 (10): 1699–1734. Bibcode:2003RPPh...66.1699B. doi:10.1088/0034-4885/66/10/R04. S2CID 250815558. Archived from the original (PDF) on 2006-03-27.

planetary.brown.edu

Kreslavsky, Mikhail A.; Ivanov, Mikhail A.; Head, James W. (21 December 2014). "The resurfacing history of Venus: Constraints from buffered crater densities" (PDF). Icarus. 250: 438–450. Bibcode:2015Icar..250..438K. doi:10.1016/j.icarus.2014.12.024. Archived from the original (PDF) on 28 July 2019. Retrieved 7 October 2016.

caltech.edu

authors.library.caltech.edu

Stevenson, David J. (15 March 2003). "Planetary magnetic fields" (PDF). Earth and Planetary Science Letters. 208 (1–2): 1–11. Bibcode:2003E&PSL.208....1S. doi:10.1016/S0012-821X(02)01126-3.

doi.org

Keddie, S. T.; Head, J. W. (1994-06-01). "Height and altitude distribution of large volcanoes on Venus". Planetary and Space Science. 42 (6): 455–462. doi:10.1016/0032-0633(94)90088-4. ISSN 0032-0633.
Justin Filiberto; et al. (3 January 2020). "Present-day volcanism on Venus as evidenced from weathering rates of olivine". Science Advances. 6 (1): eaax7445. Bibcode:2020SciA....6.7445F. doi:10.1126/sciadv.aax7445. PMC 6941908. PMID 31922004.
Weller, Matthew B.; et al. (26 October 2023). "Venus's atmospheric nitrogen explained by ancient plate tectonics". Nature Astronomy. doi:10.1038/s41550-023-02102-w. Archived from the original on 27 October 2023. Retrieved 27 October 2023.
Basilevsky, A. T.; J. W. Head III (2003). "The surface of Venus" (PDF). Reports on Progress in Physics. 66 (10): 1699–1734. Bibcode:2003RPPh...66.1699B. doi:10.1088/0034-4885/66/10/R04. S2CID 250815558. Archived from the original (PDF) on 2006-03-27.
Fegley, Bruce (1997-08-01). "Why Pyrite Is Unstable on the Surface of Venus". Icarus. 128 (2): 474–479. Bibcode:1997Icar..128..474F. doi:10.1006/icar.1997.5744.
Shepard, Michael K.; Arvidson, Raymond E.; Brackett, Robert A.; Fegley, Bruce (1994-03-15). "A ferroelectric model for the low emissivity highlands on Venus". Geophysical Research Letters. 21 (6): 469–472. Bibcode:1994GeoRL..21..469S. doi:10.1029/94GL00392. ISSN 1944-8007.
Treiman, Allan; Harrington, Elise; Sharpton, Virgil (2016-12-01). "Venus' radar-bright highlands: Different signatures and materials on Ovda Regio and on Maxwell Montes". Icarus. MicroMars to MegaMars. 280: 172–182. Bibcode:2016Icar..280..172T. doi:10.1016/j.icarus.2016.07.001.
Basilevsky, A. T.; Head, J. W.; Setyaeva, I. V. (1 September 2003). "Venus: Estimation of age of impact craters on the basis of degree of preservation of associated radar-dark deposits". Geophys. Res. Lett. 30 (18): 1950. Bibcode:2003GeoRL..30.1950B. CiteSeerX 10.1.1.556.5966. doi:10.1029/2003GL017504. S2CID 7746232.
Kreslavsky, Mikhail A.; Ivanov, Mikhail A.; Head, James W. (21 December 2014). "The resurfacing history of Venus: Constraints from buffered crater densities" (PDF). Icarus. 250: 438–450. Bibcode:2015Icar..250..438K. doi:10.1016/j.icarus.2014.12.024. Archived from the original (PDF) on 28 July 2019. Retrieved 7 October 2016.
Strom, Robert G.; Schaber, Gerald G.; Dawson, Douglas D. (1994). "The global resurfacing of Venus". Journal of Geophysical Research. 99 (E5): 10899. Bibcode:1994JGR....9910899S. doi:10.1029/94JE00388.
Jiménez-Díaz, Alberto; Ruiz, Javier; Kirby, Jon F.; Romeo, Ignacio; Tejero, Rosa; Capote, Ramón (2015-11-01). "Lithospheric structure of Venus from gravity and topography". Icarus. 260: 215–231. doi:10.1016/j.icarus.2015.07.020. hdl:20.500.11937/33938. ISSN 0019-1035.
Stevenson, David J. (15 March 2003). "Planetary magnetic fields" (PDF). Earth and Planetary Science Letters. 208 (1–2): 1–11. Bibcode:2003E&PSL.208....1S. doi:10.1016/S0012-821X(02)01126-3.
Greeley, R.; et al. (1984). "Windblown sand on Venus". Icarus. 57: 112–124. doi:10.1016/0019-1035(84)90013-7; cited in Craddock, Robert A. (2012). "Aeolian processes on the terrestrial planets: Recent observations and future focus". Progress in Physical Geography. 36: 110–124 [111]. doi:10.1177/0309133311425399. hdl:10088/17607. S2CID 129491924.
Greeley, R.; et al. (1984). "Windblown sand on Venus". Icarus. 57: 112–124. doi:10.1016/0019-1035(84)90013-7; cited in Craddock, Robert A. (2012). "Aeolian processes on the terrestrial planets: Recent observations and future focus". Progress in Physical Geography. 36: 110–124 [112]. doi:10.1177/0309133311425399. hdl:10088/17607. S2CID 129491924.
Craddock, Robert A. (2011). "Aeolian processes on the terrestrial planets: Recent observations and future focus". Progress in Physical Geography. 36 (1): 110–124. doi:10.1177/0309133311425399. S2CID 129491924.
Greeley, R., et al., Aeolian features on Venus: Preliminary Magellan results. Journal of Geophysical Research 97(E8): 13319–13345. 1992.; cited in Craddock, Robert A. (2012). "Aeolian processes on the terrestrial planets: Recent observations and future focus" (PDF). Progress in Physical Geography. 36: 110–124 [112]. doi:10.1177/0309133311425399. S2CID 129491924.
Greeley, R., et al., 1995 Wind-related features and processes on Venus: Summary of Magellan results. Icarus 115: 399–420.; cited in Craddock, Robert A. (2012). "Aeolian processes on the terrestrial planets: Recent observations and future focus" (PDF). Progress in Physical Geography. 36: 110–124 [112]. doi:10.1177/0309133311425399. S2CID 129491924.
Weitz, CM, in Ford, et al. (eds). Surface modification processes. In: Guide to Magellan Image Interpretation. Pasadena, CA: NASA Jet Propulsion Laboratory. NASA-CR-194340 JPL Publication 93-24: 57–73. 1993.; cited in Craddock, Robert A. (2012). "Aeolian processes on the terrestrial planets: Recent observations and future focus" (PDF). Progress in Physical Geography. 36: 110–124 [112]. doi:10.1177/0309133311425399. S2CID 129491924.
Hashimoto, G. L.; Roos-Serote, M.; Sugita, S.; Gilmore, M. S.; Kamp, L. W.; Carlson, R. W.; Baines, K. H. (2008). "Felsic highland crust on Venus suggested by Galileo Near-Infrared Mapping Spectrometer data". Journal of Geophysical Research: Planets. 113 (E9): E00B24. Bibcode:2008JGRE..113.0B24H. doi:10.1029/2008JE003134.
Michael J. Way; et al. (26 August 2016). "Was Venus the First Habitable World of our Solar System?". Geophysical Research Letters. 43 (16): 8376–8383. arXiv:1608.00706. Bibcode:2016GeoRL..43.8376W. doi:10.1002/2016GL069790. PMC 5385710. PMID 28408771.
Bertaux, Jean-Loup; Vandaele, Ann-Carine; Korablev, Oleg; Villard, E.; Fedorova, A.; Fussen, D.; Quémerais, E.; Belyaev, D.; et al. (2007). "A warm layer in Venus' cryosphere and high-altitude measurements of HF, HCl, H2O and HDO" (PDF). Nature. 450 (7170): 646–649. Bibcode:2007Natur.450..646B. doi:10.1038/nature05974. PMID 18046397. S2CID 4421875.

esa.int

"Where did Venus's water go?". European Space Agency. 18 December 2008. Retrieved 19 November 2016.

handle.net

hdl.handle.net

Jiménez-Díaz, Alberto; Ruiz, Javier; Kirby, Jon F.; Romeo, Ignacio; Tejero, Rosa; Capote, Ramón (2015-11-01). "Lithospheric structure of Venus from gravity and topography". Icarus. 260: 215–231. doi:10.1016/j.icarus.2015.07.020. hdl:20.500.11937/33938. ISSN 0019-1035.
Greeley, R.; et al. (1984). "Windblown sand on Venus". Icarus. 57: 112–124. doi:10.1016/0019-1035(84)90013-7; cited in Craddock, Robert A. (2012). "Aeolian processes on the terrestrial planets: Recent observations and future focus". Progress in Physical Geography. 36: 110–124 [111]. doi:10.1177/0309133311425399. hdl:10088/17607. S2CID 129491924.
Greeley, R.; et al. (1984). "Windblown sand on Venus". Icarus. 57: 112–124. doi:10.1016/0019-1035(84)90013-7; cited in Craddock, Robert A. (2012). "Aeolian processes on the terrestrial planets: Recent observations and future focus". Progress in Physical Geography. 36: 110–124 [112]. doi:10.1177/0309133311425399. hdl:10088/17607. S2CID 129491924.

harvard.edu

ui.adsabs.harvard.edu

Justin Filiberto; et al. (3 January 2020). "Present-day volcanism on Venus as evidenced from weathering rates of olivine". Science Advances. 6 (1): eaax7445. Bibcode:2020SciA....6.7445F. doi:10.1126/sciadv.aax7445. PMC 6941908. PMID 31922004.
Basilevsky, A. T.; J. W. Head III (2003). "The surface of Venus" (PDF). Reports on Progress in Physics. 66 (10): 1699–1734. Bibcode:2003RPPh...66.1699B. doi:10.1088/0034-4885/66/10/R04. S2CID 250815558. Archived from the original (PDF) on 2006-03-27.
Zolotov, M.Y. (1991). "Pyrite Stability on the Surface of Venus". Abstracts of the Lunar and Planetary Science Conference. 22: 1569–1570. Bibcode:1991LPI....22.1569Z.
Fegley, Bruce (1997-08-01). "Why Pyrite Is Unstable on the Surface of Venus". Icarus. 128 (2): 474–479. Bibcode:1997Icar..128..474F. doi:10.1006/icar.1997.5744.
Shepard, Michael K.; Arvidson, Raymond E.; Brackett, Robert A.; Fegley, Bruce (1994-03-15). "A ferroelectric model for the low emissivity highlands on Venus". Geophysical Research Letters. 21 (6): 469–472. Bibcode:1994GeoRL..21..469S. doi:10.1029/94GL00392. ISSN 1944-8007.
Treiman, Allan; Harrington, Elise; Sharpton, Virgil (2016-12-01). "Venus' radar-bright highlands: Different signatures and materials on Ovda Regio and on Maxwell Montes". Icarus. MicroMars to MegaMars. 280: 172–182. Bibcode:2016Icar..280..172T. doi:10.1016/j.icarus.2016.07.001.
Basilevsky, A. T.; Head, J. W.; Setyaeva, I. V. (1 September 2003). "Venus: Estimation of age of impact craters on the basis of degree of preservation of associated radar-dark deposits". Geophys. Res. Lett. 30 (18): 1950. Bibcode:2003GeoRL..30.1950B. CiteSeerX 10.1.1.556.5966. doi:10.1029/2003GL017504. S2CID 7746232.
Kreslavsky, Mikhail A.; Ivanov, Mikhail A.; Head, James W. (21 December 2014). "The resurfacing history of Venus: Constraints from buffered crater densities" (PDF). Icarus. 250: 438–450. Bibcode:2015Icar..250..438K. doi:10.1016/j.icarus.2014.12.024. Archived from the original (PDF) on 28 July 2019. Retrieved 7 October 2016.
Strom, Robert G.; Schaber, Gerald G.; Dawson, Douglas D. (1994). "The global resurfacing of Venus". Journal of Geophysical Research. 99 (E5): 10899. Bibcode:1994JGR....9910899S. doi:10.1029/94JE00388.
Stevenson, David J. (15 March 2003). "Planetary magnetic fields" (PDF). Earth and Planetary Science Letters. 208 (1–2): 1–11. Bibcode:2003E&PSL.208....1S. doi:10.1016/S0012-821X(02)01126-3.
Hashimoto, G. L.; Roos-Serote, M.; Sugita, S.; Gilmore, M. S.; Kamp, L. W.; Carlson, R. W.; Baines, K. H. (2008). "Felsic highland crust on Venus suggested by Galileo Near-Infrared Mapping Spectrometer data". Journal of Geophysical Research: Planets. 113 (E9): E00B24. Bibcode:2008JGRE..113.0B24H. doi:10.1029/2008JE003134.
Michael J. Way; et al. (26 August 2016). "Was Venus the First Habitable World of our Solar System?". Geophysical Research Letters. 43 (16): 8376–8383. arXiv:1608.00706. Bibcode:2016GeoRL..43.8376W. doi:10.1002/2016GL069790. PMC 5385710. PMID 28408771.
Bertaux, Jean-Loup; Vandaele, Ann-Carine; Korablev, Oleg; Villard, E.; Fedorova, A.; Fussen, D.; Quémerais, E.; Belyaev, D.; et al. (2007). "A warm layer in Venus' cryosphere and high-altitude measurements of HF, HCl, H2O and HDO" (PDF). Nature. 450 (7170): 646–649. Bibcode:2007Natur.450..646B. doi:10.1038/nature05974. PMID 18046397. S2CID 4421875.

nasa.gov

climate.nasa.gov

Michael Cabbage and Leslie McCarthy (11 August 2016). "NASA climate modeling suggests Venus may have been habitable". NASA. Retrieved 19 November 2016.

nature.com

Weller, Matthew B.; et al. (26 October 2023). "Venus's atmospheric nitrogen explained by ancient plate tectonics". Nature Astronomy. doi:10.1038/s41550-023-02102-w. Archived from the original on 27 October 2023. Retrieved 27 October 2023.

newscientist.com

David Shiga (10 October 2007). "Did Venus's ancient oceans incubate life?". New Scientist.

nih.gov

pubmed.ncbi.nlm.nih.gov

Justin Filiberto; et al. (3 January 2020). "Present-day volcanism on Venus as evidenced from weathering rates of olivine". Science Advances. 6 (1): eaax7445. Bibcode:2020SciA....6.7445F. doi:10.1126/sciadv.aax7445. PMC 6941908. PMID 31922004.
Michael J. Way; et al. (26 August 2016). "Was Venus the First Habitable World of our Solar System?". Geophysical Research Letters. 43 (16): 8376–8383. arXiv:1608.00706. Bibcode:2016GeoRL..43.8376W. doi:10.1002/2016GL069790. PMC 5385710. PMID 28408771.
Bertaux, Jean-Loup; Vandaele, Ann-Carine; Korablev, Oleg; Villard, E.; Fedorova, A.; Fussen, D.; Quémerais, E.; Belyaev, D.; et al. (2007). "A warm layer in Venus' cryosphere and high-altitude measurements of HF, HCl, H2O and HDO" (PDF). Nature. 450 (7170): 646–649. Bibcode:2007Natur.450..646B. doi:10.1038/nature05974. PMID 18046397. S2CID 4421875.

ncbi.nlm.nih.gov

Justin Filiberto; et al. (3 January 2020). "Present-day volcanism on Venus as evidenced from weathering rates of olivine". Science Advances. 6 (1): eaax7445. Bibcode:2020SciA....6.7445F. doi:10.1126/sciadv.aax7445. PMC 6941908. PMID 31922004.
Michael J. Way; et al. (26 August 2016). "Was Venus the First Habitable World of our Solar System?". Geophysical Research Letters. 43 (16): 8376–8383. arXiv:1608.00706. Bibcode:2016GeoRL..43.8376W. doi:10.1002/2016GL069790. PMC 5385710. PMID 28408771.

nytimes.com

Chang, Kenneth (26 October 2023). "Billions of Years Ago, Venus May Have Had a Key Earthlike Feature - A new study makes the case that the solar system's hellish second planet once may have had plate tectonics that could have made it more hospitable to life". The New York Times. Archived from the original on 26 October 2023. Retrieved 27 October 2023.

psu.edu

citeseerx.ist.psu.edu

Basilevsky, A. T.; Head, J. W.; Setyaeva, I. V. (1 September 2003). "Venus: Estimation of age of impact craters on the basis of degree of preservation of associated radar-dark deposits". Geophys. Res. Lett. 30 (18): 1950. Bibcode:2003GeoRL..30.1950B. CiteSeerX 10.1.1.556.5966. doi:10.1029/2003GL017504. S2CID 7746232.

sciencedirect.com

Keddie, S. T.; Head, J. W. (1994-06-01). "Height and altitude distribution of large volcanoes on Venus". Planetary and Space Science. 42 (6): 455–462. doi:10.1016/0032-0633(94)90088-4. ISSN 0032-0633.
Jiménez-Díaz, Alberto; Ruiz, Javier; Kirby, Jon F.; Romeo, Ignacio; Tejero, Rosa; Capote, Ramón (2015-11-01). "Lithospheric structure of Venus from gravity and topography". Icarus. 260: 215–231. doi:10.1016/j.icarus.2015.07.020. hdl:20.500.11937/33938. ISSN 0019-1035.

scientificamerican.com

Shannon Hall (10 August 2016). "Hellish Venus Might Have Been Habitable for Billions of Years". Scientific American. Retrieved 19 November 2016.

semanticscholar.org

api.semanticscholar.org

Basilevsky, A. T.; J. W. Head III (2003). "The surface of Venus" (PDF). Reports on Progress in Physics. 66 (10): 1699–1734. Bibcode:2003RPPh...66.1699B. doi:10.1088/0034-4885/66/10/R04. S2CID 250815558. Archived from the original (PDF) on 2006-03-27.
Basilevsky, A. T.; Head, J. W.; Setyaeva, I. V. (1 September 2003). "Venus: Estimation of age of impact craters on the basis of degree of preservation of associated radar-dark deposits". Geophys. Res. Lett. 30 (18): 1950. Bibcode:2003GeoRL..30.1950B. CiteSeerX 10.1.1.556.5966. doi:10.1029/2003GL017504. S2CID 7746232.
Greeley, R.; et al. (1984). "Windblown sand on Venus". Icarus. 57: 112–124. doi:10.1016/0019-1035(84)90013-7; cited in Craddock, Robert A. (2012). "Aeolian processes on the terrestrial planets: Recent observations and future focus". Progress in Physical Geography. 36: 110–124 [111]. doi:10.1177/0309133311425399. hdl:10088/17607. S2CID 129491924.
Greeley, R.; et al. (1984). "Windblown sand on Venus". Icarus. 57: 112–124. doi:10.1016/0019-1035(84)90013-7; cited in Craddock, Robert A. (2012). "Aeolian processes on the terrestrial planets: Recent observations and future focus". Progress in Physical Geography. 36: 110–124 [112]. doi:10.1177/0309133311425399. hdl:10088/17607. S2CID 129491924.
Craddock, Robert A. (2011). "Aeolian processes on the terrestrial planets: Recent observations and future focus". Progress in Physical Geography. 36 (1): 110–124. doi:10.1177/0309133311425399. S2CID 129491924.
Greeley, R., et al., Aeolian features on Venus: Preliminary Magellan results. Journal of Geophysical Research 97(E8): 13319–13345. 1992.; cited in Craddock, Robert A. (2012). "Aeolian processes on the terrestrial planets: Recent observations and future focus" (PDF). Progress in Physical Geography. 36: 110–124 [112]. doi:10.1177/0309133311425399. S2CID 129491924.
Greeley, R., et al., 1995 Wind-related features and processes on Venus: Summary of Magellan results. Icarus 115: 399–420.; cited in Craddock, Robert A. (2012). "Aeolian processes on the terrestrial planets: Recent observations and future focus" (PDF). Progress in Physical Geography. 36: 110–124 [112]. doi:10.1177/0309133311425399. S2CID 129491924.
Weitz, CM, in Ford, et al. (eds). Surface modification processes. In: Guide to Magellan Image Interpretation. Pasadena, CA: NASA Jet Propulsion Laboratory. NASA-CR-194340 JPL Publication 93-24: 57–73. 1993.; cited in Craddock, Robert A. (2012). "Aeolian processes on the terrestrial planets: Recent observations and future focus" (PDF). Progress in Physical Geography. 36: 110–124 [112]. doi:10.1177/0309133311425399. S2CID 129491924.
Bertaux, Jean-Loup; Vandaele, Ann-Carine; Korablev, Oleg; Villard, E.; Fedorova, A.; Fussen, D.; Quémerais, E.; Belyaev, D.; et al. (2007). "A warm layer in Venus' cryosphere and high-altitude measurements of HF, HCl, H2O and HDO" (PDF). Nature. 450 (7170): 646–649. Bibcode:2007Natur.450..646B. doi:10.1038/nature05974. PMID 18046397. S2CID 4421875.

si.edu

repository.si.edu

Greeley, R., et al., Aeolian features on Venus: Preliminary Magellan results. Journal of Geophysical Research 97(E8): 13319–13345. 1992.; cited in Craddock, Robert A. (2012). "Aeolian processes on the terrestrial planets: Recent observations and future focus" (PDF). Progress in Physical Geography. 36: 110–124 [112]. doi:10.1177/0309133311425399. S2CID 129491924.
Greeley, R., et al., 1995 Wind-related features and processes on Venus: Summary of Magellan results. Icarus 115: 399–420.; cited in Craddock, Robert A. (2012). "Aeolian processes on the terrestrial planets: Recent observations and future focus" (PDF). Progress in Physical Geography. 36: 110–124 [112]. doi:10.1177/0309133311425399. S2CID 129491924.
Weitz, CM, in Ford, et al. (eds). Surface modification processes. In: Guide to Magellan Image Interpretation. Pasadena, CA: NASA Jet Propulsion Laboratory. NASA-CR-194340 JPL Publication 93-24: 57–73. 1993.; cited in Craddock, Robert A. (2012). "Aeolian processes on the terrestrial planets: Recent observations and future focus" (PDF). Progress in Physical Geography. 36: 110–124 [112]. doi:10.1177/0309133311425399. S2CID 129491924.

uliege.be

orbi.uliege.be

Bertaux, Jean-Loup; Vandaele, Ann-Carine; Korablev, Oleg; Villard, E.; Fedorova, A.; Fussen, D.; Quémerais, E.; Belyaev, D.; et al. (2007). "A warm layer in Venus' cryosphere and high-altitude measurements of HF, HCl, H2O and HDO" (PDF). Nature. 450 (7170): 646–649. Bibcode:2007Natur.450..646B. doi:10.1038/nature05974. PMID 18046397. S2CID 4421875.

usgs.gov

pubs.usgs.gov

Ivanov, Mikhail A.; Head, James W. (2010). Scientific Pamphlet, Geologic Map of the Lakshmi Planum Quadrangle (V–7), Venus (PDF). USGS. Retrieved 27 September 2016.

usra.edu

hou.usra.edu

Battaglia, Steven M. (March 2016). "Venus: Could Resurfacing Events be Triggered by Sun's Oscillations through the Galactic Mid-Plane?" (PDF). The 47th Lunar and Planetary Science Conference.

web.archive.org

Basilevsky, A. T.; J. W. Head III (2003). "The surface of Venus" (PDF). Reports on Progress in Physics. 66 (10): 1699–1734. Bibcode:2003RPPh...66.1699B. doi:10.1088/0034-4885/66/10/R04. S2CID 250815558. Archived from the original (PDF) on 2006-03-27.
Kreslavsky, Mikhail A.; Ivanov, Mikhail A.; Head, James W. (21 December 2014). "The resurfacing history of Venus: Constraints from buffered crater densities" (PDF). Icarus. 250: 438–450. Bibcode:2015Icar..250..438K. doi:10.1016/j.icarus.2014.12.024. Archived from the original (PDF) on 28 July 2019. Retrieved 7 October 2016.

wolframalpha.com

"Wolfram-Alpha: Computational Knowledge Engine". wolframalpha.com.
"Wolfram-Alpha: Computational Knowledge Engine". wolframalpha.com.

worldcat.org

search.worldcat.org

Keddie, S. T.; Head, J. W. (1994-06-01). "Height and altitude distribution of large volcanoes on Venus". Planetary and Space Science. 42 (6): 455–462. doi:10.1016/0032-0633(94)90088-4. ISSN 0032-0633.
Shepard, Michael K.; Arvidson, Raymond E.; Brackett, Robert A.; Fegley, Bruce (1994-03-15). "A ferroelectric model for the low emissivity highlands on Venus". Geophysical Research Letters. 21 (6): 469–472. Bibcode:1994GeoRL..21..469S. doi:10.1029/94GL00392. ISSN 1944-8007.
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