Mars (planet) (Swedish Wikipedia)

Analysis of information sources in references of the Wikipedia article "Mars (planet)" in Swedish language version.

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19doi.org

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anl.gov

Dave Jacqué (2004-03-18). ”APS X-rays reveal secrets of Mars' core”. Argonne National Laboratory. http://www.anl.gov/Media_Center/News/2003/030926mars.htm. Läst 4 november 2006.

aqua.co.za

Van Zyl, Jan Eben. ”Get to know Mars - 1”. Johannesburg Centre, Astronomical Society of Southern Africa. Arkiverad från originalet den 23 september 2006. https://web.archive.org/web/20060923084435/http://www.aqua.co.za/assa_jhb/new/Canopus/Can2004/c044litu.htm.

archive.is

Yeager, Ashley (19 juli 2008). ”Impact May Have Transformed Mars”. ScienceNews.org. Arkiverad från originalet den 14 september 2012. https://archive.is/20120914153420/http://www.sciencenews.org/view/generic/id/33622/title/Impact_may_have_transformed_Mars_. Läst 12 augusti 2008.

archive.org

Zubrin, Robert (1996). The case for Mars : the plan to settle the red planet and why we must. New York : Free Press. ISBN 978-0-684-82757-5. http://archive.org/details/caseformarsplant00zubr. Läst 30 augusti 2021

arizona.edu

uapress.arizona.edu

Sheehan, William (1997). ”Chapter 4 Areographers”. The Planet Mars: A History of Observation and Discovery. The University of Arizona Press. Arkiverad från originalet den 1 juli 2017. https://web.archive.org/web/20170701062415/http://www.uapress.arizona.edu/onlinebks/MARS/CHAP04.HTM. Läst 10 november 2006.
Sheehan, William (1996). ”2: Pioneers”. The Planet Mars: A History of Observation and Discovery. Tucson: University of Arizona. Bibcode: 1996pmho.book.....S. Läst 11 februari 2024

arxiv.org

Mallama, Anthony; Hilton, James L. (oktober 2018). ”Computing apparent planetary magnitudes for The Astronomical Almanac”. Astronomy and Computing 25: sid. 10–24. doi:10.1016/j.ascom.2018.08.002. https://arxiv.org/abs/1808.01973.

bbcearth.com

Martin Redfern. ”Will we ever set foot on Mars?”. BBC Earth. https://www.bbcearth.com/news/will-we-ever-set-foot-on-mars. Läst 19 januari 2024.

britannica.com

”Mars - Atmosphere, Climate, Dust Storms | Britannica” (på engelska). www.britannica.com. https://www.britannica.com/place/Mars-planet/The-atmosphere. Läst 16 januari 2024.

caltech.edu

coolcosmos.ipac.caltech.edu

”Why is Mars reddish?” (på engelska). Cool Cosmos. https://coolcosmos.ipac.caltech.edu/ask/69-Why-is-Mars-reddish-. Läst 18 februari 2024.

crystalinks.com

”Topography”. Mars. http://www.crystalinks.com/mars2.html. Läst 10 november 2006.

cths.fr

Marjorie Jung, Bruno Delmas (17 oktober 2023). ”MARALDI Jacques-Philippe (Giacomo Filippo)” (på franska). Comité des travaux historiques et scientifiques. https://cths.fr/an/savant.php?id=116993#. Läst 11 februari 2024.

dn.se

DN - Islavin fotograferad på Mars
”Rymdsonden Perseverance har landat på Mars”. Dagens Nyheter. 18 februari 2021. https://www.dn.se/varlden/rymdsonden-perseverance-landar-pa-mars-i-kvall/. Läst 18 februari 2021.

doi.org

dx.doi.org

Seidelmann, P. Kenneth (2007). ”Report of the IAU/IAG Working Group on cartographic coordinates and rotational elements: 2006”. Celestial Mechanics and Dynamical Astronomy 98 (3): sid. 155–180. doi:10.1007/s10569-007-9072-y. http://adsabs.harvard.edu/doi/10.1007/s10569-007-9072-y. Läst 28 augusti 2007.
Mallama, Anthony; Hilton, James L. (oktober 2018). ”Computing apparent planetary magnitudes for The Astronomical Almanac”. Astronomy and Computing 25: sid. 10–24. doi:10.1016/j.ascom.2018.08.002. https://arxiv.org/abs/1808.01973.
J. Laskar et al. (2004), Long term evolution and chaotic diffusion of the insolation quantities of Mars, Icarus, 170, 343–364
B. Jakosky & M. Carr (1985), Possible precipitation of ice at low latitudes of Mars during periods of high obliquity, Nature, 315, 559–561
M. Mischna et al. (2003), On the orbital forcing of Martian water and CO2 cycles: A general circulation model study with simplified volatile schemes, J. Geophys. Res., 108(E6), 5062
T. de Haas; E. Hauber; S. J. Conway; H. van Steijn; A. Johnsson & M. G. Kleinhans (23 juni 2015). ”Earth-like aqueous debris-flow activity on Mars at high orbital obliquity in the last million years”. Nature Communications 6: sid. artikel nummer 7543. doi:10.1038/ncomms8543.
Connerney, J. E. P.; et al. (1999). ”Magnetic Lineations in the Ancient Crust of Mars”. Science 284: sid. 794–798. doi:10.1126/science.284.5415.794.
Connerney, J.; Acuña, M. H.; Ness, N. F.; Reme, H. (2005). ”Tectonic implications of Mars crustal magnetism”. Proc. Natl. Acad. Sci. USA 102 (42): sid. 14970–14975. doi:10.1073/pnas.0507469102.
Carr, M. H.; Head, J. W. (2010). ”Geologic History of Mars”. Earth and Planetary Science Letters 294 (3–4): sid. 185–203. doi:10.1016/j.epsl.2009.06.042. https://zenodo.org/record/1258929/files/article.pdf.
Neukum, G. et al. (2004). ”Recent and episodic volcanic and glacial activity on Mars revealed by the High Resolution Stereo Camera”. Nature 432: sid. 971–979. http://dx.doi.org/10.1038/nature03231.
Jakosky, Bruce M. och Phillips, Roger J. (2001). ”Mars' volatile and climate history”. Nature 412: sid. 237–244. http://dx.doi.org/10.1038/35084184.
Hoffman, Nick (2000). White Mars: A New Model for Mars' Surface and Atmosphere Based on CO₂. "146". sid. 326–342. http://dx.doi.org/10.1006/icar.2000.6398.
”Ekvatorssken på Mars fascinerar”. ESA. 15 mars 2006. http://www.esa.int/esaCP/SEMP6MNVGJE_Sweden_0.html. pressmeddelande baserat på Lundin, R.; et al. (2006). ”Plasma Acceleration Above Martian Magnetic Anomalies”. Science 311 (5763): sid. 980–983. doi:10.1126/science.1122071. http://adsabs.harvard.edu/abs/2006Sci...311..980L.
Heldmann, Jennifer L. (7 maj 2005). ”Formation of Martian gullies by the action of liquid water flowing under current Martian environmental conditions” (PDF). Journal of Geophysical Research "110": s. Eo5004. doi:10.1029/2004JE002261. Arkiverad från originalet den 1 oktober 2008. https://web.archive.org/web/20081001162643/http://daleandersen.seti.org/Dale_Andersen/Science_articles_files/Heldmann%20et%20al.2005.pdf. Läst 17 september 2008. 'conditions such as now occur on Mars, outside of the temperature-pressure stability regime of liquid water' ... 'Liquid water is typically stable at the lowest elevations and at low latitudes on the planet because the atmospheric pressure is greater than the vapor pressure of water and surface temperatures in equatorial regions can reach 273 K for parts of the day [Haberle et al., 2001]'
Lemmon, M. T. (10 april 2004). ”Atmospheric Imaging Results from Mars Rovers”. Science "306" (5702): ss. 1753–1756. doi:10.1126/science.1104474. PMID 15576613.
Formisano, V.; Atreya, S.; Encrenaz, T.; Ignatiev, N.; Giuranna, M. (2004). ”Detection of Methane in the Atmosphere of Mars”. Science 306: sid. 1758–1761. doi:10.1126/science.1101732. PMID 15514118.
Mumma, Michael J. (20 februari 2009). ”Strong Release of Methane on Mars in Northern Summer 2003”. Science "323" (5917): s. 1041–1045. doi:10.1126/science.1165243. PMID 19150811. http://images.spaceref.com/news/2009/Mumma_et_al_Methane_Mars_wSOM_accepted2.pdf.
Craddock, Robert A. (februari 2011). ”Are Phobos and Deimos the result of a giant impact?”. Icarus (2): sid. 1150–1161. doi:10.1016/j.icarus.2010.10.023. https://ui.adsabs.harvard.edu/abs/2011Icar..211.1150C/abstract.
Sagan, Carl; Fox, Paul (augusti 1975). ”The canals of Mars: An assessment after Mariner 9” (på engelska). Icarus 25 (4): sid. 602–612. doi:10.1016/0019-1035(75)90042-1. https://linkinghub.elsevier.com/retrieve/pii/0019103575900421.

elsevier.com

linkinghub.elsevier.com

Sagan, Carl; Fox, Paul (augusti 1975). ”The canals of Mars: An assessment after Mariner 9” (på engelska). Icarus 25 (4): sid. 602–612. doi:10.1016/0019-1035(75)90042-1. https://linkinghub.elsevier.com/retrieve/pii/0019103575900421.

eos.org

Joshua Rapp Learn (27 april 2020). ”The Massive Ice Avalanches of Mars” (på amerikansk engelska). Eos. http://eos.org/articles/the-massive-ice-avalanches-of-mars. Läst 22 januari 2024.

esa.int

”Ekvatorssken på Mars fascinerar”. ESA. 15 mars 2006. http://www.esa.int/esaCP/SEMP6MNVGJE_Sweden_0.html. pressmeddelande baserat på Lundin, R.; et al. (2006). ”Plasma Acceleration Above Martian Magnetic Anomalies”. Science 311 (5763): sid. 980–983. doi:10.1126/science.1122071. http://adsabs.harvard.edu/abs/2006Sci...311..980L.
ESA (15 mars 2007). ”Mars Express radar pejlar vattenmängden vid Mars sydpol”. Pressmeddelande.
ESA (13 december 2006). ”Vetenskapsmän från Mars Express hittar ett annorlunda Mars under ytan”. Pressmeddelande.
”Mars Express confirms methane in the Martian atmosphere”. ESA. 30 mars 2004. Arkiverad från originalet. https://web.archive.org/web/20060224102528/http://www.esa.int/SPECIALS/Mars_Express/SEMZ0B57ESD_0.html. Läst 30 januari 2024.
”Europe’s Mars exploration” (på engelska). www.esa.int. https://www.esa.int/Science_Exploration/Human_and_Robotic_Exploration/Exploration/ExoMars/Europe_s_Mars_exploration. Läst 19 januari 2024.
”Mars500: study overview” (på engelska). www.esa.int. https://www.esa.int/Science_Exploration/Human_and_Robotic_Exploration/Mars500/Mars500_study_overview. Läst 19 januari 2024.

sci.esa.int

”ESA Science & Technology – The Ages of Mars”. sci.esa.int. 1 september 2019. Arkiverad från originalet den 25 september 2019. https://web.archive.org/web/20190925145605/https://sci.esa.int/web/mars-express/-/55481-the-ages-of-mars. Läst 7 december 2021.
”Martian moons: Phobos”. ESA Science & Technology. 1 september 2019. https://sci.esa.int/web/mars-express/-/31031-phobos. Läst 30 januari 2024.
”Martian moons: Deimos”. ESA Science & Technology. 1 september 2019. https://sci.esa.int/web/mars-express/-/50837-deimos. Läst 30 januari 2024.

exploration.esa.int

”ESA - Robotic Exploration of Mars - The enigma of methane on Mars”. exploration.esa.int. https://exploration.esa.int/web/mars/-/46038-methane-on-mars. Läst 22 januari 2024.

feber.se

”NASA har hittat flytande vatten på Mars”. Feber / Vetenskap. http://feber.se/vetenskap/art/335618/nasa_har_hittat_flytande_vatte/. Läst 22 november 2015.

globalnet.co.uk

users.globalnet.co.uk

Zubrin, Robert; McKay, Christopher (1993). ”Technological Requirements for Terraforming Mars”. http://www.users.globalnet.co.uk/~mfogg/zubrin.htm.

gu.se

science.gu.se

Eliasson, Carina. ”Mer vatten på Mars än man tidigare trott”. Göteborgs universitet. Arkiverad från originalet den 14 juli 2015. https://web.archive.org/web/20150714114729/http://science.gu.se/aktuellt/nyheter/Nyheter%2520Detalj//mer-vatten-pa-mars-an-man-tidigare-trott.cid1311272. Läst 14 juli 2015.

guardian.co.uk

Sample, Ian (26 juni 2008). ”Cataclysmic impact created north-south divide on Mars”. Science @ guardian.co.uk. http://www.guardian.co.uk/science/2008/jun/26/mars.asteroid?gusrc=rss&feed=science. Läst 12 augusti 2008.

harvard.edu

adsabs.harvard.edu

Seidelmann, P. Kenneth (2007). ”Report of the IAU/IAG Working Group on cartographic coordinates and rotational elements: 2006”. Celestial Mechanics and Dynamical Astronomy 98 (3): sid. 155–180. doi:10.1007/s10569-007-9072-y. http://adsabs.harvard.edu/doi/10.1007/s10569-007-9072-y. Läst 28 augusti 2007.
”Ekvatorssken på Mars fascinerar”. ESA. 15 mars 2006. http://www.esa.int/esaCP/SEMP6MNVGJE_Sweden_0.html. pressmeddelande baserat på Lundin, R.; et al. (2006). ”Plasma Acceleration Above Martian Magnetic Anomalies”. Science 311 (5763): sid. 980–983. doi:10.1126/science.1122071. http://adsabs.harvard.edu/abs/2006Sci...311..980L.
Sheehan, William (1996). ”2: Pioneers”. The Planet Mars: A History of Observation and Discovery. Tucson: University of Arizona. Bibcode: 1996pmho.book.....S. Läst 11 februari 2024

ui.adsabs.harvard.edu

Craddock, R. A. (1994). ”The Origin of PHOBOS and Deimos”. Abstracts of the 25th Lunar and Planetary Science Conference: sid. 293–294. https://ui.adsabs.harvard.edu/link_gateway/1994LPI....25..293C/ADS_PDF.
Craddock, Robert A. (februari 2011). ”Are Phobos and Deimos the result of a giant impact?”. Icarus (2): sid. 1150–1161. doi:10.1016/j.icarus.2010.10.023. https://ui.adsabs.harvard.edu/abs/2011Icar..211.1150C/abstract.

nasa.gov

nih.gov

ncbi.nlm.nih.gov

Lemmon, M. T. (10 april 2004). ”Atmospheric Imaging Results from Mars Rovers”. Science "306" (5702): ss. 1753–1756. doi:10.1126/science.1104474. PMID 15576613.
Formisano, V.; Atreya, S.; Encrenaz, T.; Ignatiev, N.; Giuranna, M. (2004). ”Detection of Methane in the Atmosphere of Mars”. Science 306: sid. 1758–1761. doi:10.1126/science.1101732. PMID 15514118.
Mumma, Michael J. (20 februari 2009). ”Strong Release of Methane on Mars in Northern Summer 2003”. Science "323" (5917): s. 1041–1045. doi:10.1126/science.1165243. PMID 19150811. http://images.spaceref.com/news/2009/Mumma_et_al_Methane_Mars_wSOM_accepted2.pdf.

nineplanets.org

”Phobos”. nineplanets. 17 oktober 2019. https://nineplanets.org/phobos/. Läst 30 januari 2024.

npr.org

”Success! NASA's Ingenuity Makes 1st Powered Flight On Mars”. https://www.npr.org. 19 april 2021. https://www.npr.org/2021/04/19/985588253/success-nasas-ingenuity-makes-first-powered-flight-on-mars. Läst 31 januari 2023.

nytimes.com

”Huge Meteor Strike Explains Mars’s Shape, Reports Say”. New York Times. http://www.nytimes.com/2008/06/26/science/space/26mars.html?em&ex=1214712000&en=bd0be05a87523855&ei=5087%0A. Läst 27 juni 2008.

phys.org

”Early Mars was covered in ice sheets, not flowing rivers: study” (på engelska). phys.org. https://phys.org/news/2020-08-early-mars-ice-sheets-rivers.html. Läst 16 oktober 2020.

sciam.com

”Giant Asteroid Flattened Half of Mars, Studies Suggest”. Scientific American. http://www.sciam.com/article.cfm?id=giant-asteroid-flattened. Läst 27 juni 2008.

sciencenews.org

Yeager, Ashley (19 juli 2008). ”Impact May Have Transformed Mars”. ScienceNews.org. Arkiverad från originalet den 14 september 2012. https://archive.is/20120914153420/http://www.sciencenews.org/view/generic/id/33622/title/Impact_may_have_transformed_Mars_. Läst 12 augusti 2008.

serious-science.org

”What Color Is the Sky on Mars?” (på amerikansk engelska). Serious Science. https://serious-science.org/what-color-is-the-sky-on-mars-7310. Läst 16 januari 2024.

seti.org

daleandersen.seti.org

Heldmann, Jennifer L. (7 maj 2005). ”Formation of Martian gullies by the action of liquid water flowing under current Martian environmental conditions” (PDF). Journal of Geophysical Research "110": s. Eo5004. doi:10.1029/2004JE002261. Arkiverad från originalet den 1 oktober 2008. https://web.archive.org/web/20081001162643/http://daleandersen.seti.org/Dale_Andersen/Science_articles_files/Heldmann%20et%20al.2005.pdf. Läst 17 september 2008. 'conditions such as now occur on Mars, outside of the temperature-pressure stability regime of liquid water' ... 'Liquid water is typically stable at the lowest elevations and at low latitudes on the planet because the atmospheric pressure is greater than the vapor pressure of water and surface temperatures in equatorial regions can reach 273 K for parts of the day [Haberle et al., 2001]'

space.com

Daisy Dobrijevic (4 februari 2022). ”Distance to Mars: How Far Away is the Red Planet?” (på engelska). Space.com. https://www.space.com/16875-how-far-away-is-mars.html. Läst 24 augusti 2023.

spaceref.com

images.spaceref.com

Mumma, Michael J. (20 februari 2009). ”Strong Release of Methane on Mars in Northern Summer 2003”. Science "323" (5917): s. 1041–1045. doi:10.1126/science.1165243. PMID 19150811. http://images.spaceref.com/news/2009/Mumma_et_al_Methane_Mars_wSOM_accepted2.pdf.

theoi.com

”Ares Attendants: Deimos & Phobos”. Greek Mythology. http://www.theoi.com/Olympios/AresAttendants.html. Läst 13 juni 2006.

umich.edu

esse.engin.umich.edu

Hand, Eric (21 oktober 2008). ”Plumes of methane identified on Mars”. Nature News. Arkiverad från originalet den 7 mars 2012. https://web.archive.org/web/20120307183317/http://esse.engin.umich.edu/psl/PRESS/Mars/NatureNews_2008.pdf. Läst 2 augusti 2009.

universetoday.com

Nancy Atkinson (17 juli 2007). ”The Mars Landing Approach: Getting Large Payloads to the Surface of the Red Planet”. http://www.universetoday.com/2007/07/17/the-mars-landing-approach-getting-large-payloads-to-the-surface-of-the-red-planet. Läst 18 september 2007.

web.archive.org

Eliasson, Carina. ”Mer vatten på Mars än man tidigare trott”. Göteborgs universitet. Arkiverad från originalet den 14 juli 2015. https://web.archive.org/web/20150714114729/http://science.gu.se/aktuellt/nyheter/Nyheter%2520Detalj//mer-vatten-pa-mars-an-man-tidigare-trott.cid1311272. Läst 14 juli 2015.
”ESA Science & Technology – The Ages of Mars”. sci.esa.int. 1 september 2019. Arkiverad från originalet den 25 september 2019. https://web.archive.org/web/20190925145605/https://sci.esa.int/web/mars-express/-/55481-the-ages-of-mars. Läst 7 december 2021.
Sheehan, William (1997). ”Chapter 4 Areographers”. The Planet Mars: A History of Observation and Discovery. The University of Arizona Press. Arkiverad från originalet den 1 juli 2017. https://web.archive.org/web/20170701062415/http://www.uapress.arizona.edu/onlinebks/MARS/CHAP04.HTM. Läst 10 november 2006.
Van Zyl, Jan Eben. ”Get to know Mars - 1”. Johannesburg Centre, Astronomical Society of Southern Africa. Arkiverad från originalet den 23 september 2006. https://web.archive.org/web/20060923084435/http://www.aqua.co.za/assa_jhb/new/Canopus/Can2004/c044litu.htm.
NASA (3 mars 2004). ”Mineral in Mars 'Berries' Adds to Water Story”. Pressmeddelande. Läst 13 juni 2006. Arkiverad från originalet den 9 november 2007.
Heldmann, Jennifer L. (7 maj 2005). ”Formation of Martian gullies by the action of liquid water flowing under current Martian environmental conditions” (PDF). Journal of Geophysical Research "110": s. Eo5004. doi:10.1029/2004JE002261. Arkiverad från originalet den 1 oktober 2008. https://web.archive.org/web/20081001162643/http://daleandersen.seti.org/Dale_Andersen/Science_articles_files/Heldmann%20et%20al.2005.pdf. Läst 17 september 2008. 'conditions such as now occur on Mars, outside of the temperature-pressure stability regime of liquid water' ... 'Liquid water is typically stable at the lowest elevations and at low latitudes on the planet because the atmospheric pressure is greater than the vapor pressure of water and surface temperatures in equatorial regions can reach 273 K for parts of the day [Haberle et al., 2001]'
”Mars Express confirms methane in the Martian atmosphere”. ESA. 30 mars 2004. Arkiverad från originalet. https://web.archive.org/web/20060224102528/http://www.esa.int/SPECIALS/Mars_Express/SEMZ0B57ESD_0.html. Läst 30 januari 2024.
Hand, Eric (21 oktober 2008). ”Plumes of methane identified on Mars”. Nature News. Arkiverad från originalet den 7 mars 2012. https://web.archive.org/web/20120307183317/http://esse.engin.umich.edu/psl/PRESS/Mars/NatureNews_2008.pdf. Läst 2 augusti 2009.
”Planet Gobbling Dust Storms”. Science @ NASA. 16 juli 2001. Arkiverad från originalet den 13 juni 2006. https://web.archive.org/web/20060613062647/http://science.nasa.gov/headlines/y2001/ast16jul_1.htm. Läst 20 februari 2024.

zenodo.org

Carr, M. H.; Head, J. W. (2010). ”Geologic History of Mars”. Earth and Planetary Science Letters 294 (3–4): sid. 185–203. doi:10.1016/j.epsl.2009.06.042. https://zenodo.org/record/1258929/files/article.pdf.

Mars (planet) (Swedish Wikipedia)

anl.gov

aqua.co.za

archive.is

archive.org

arizona.edu

uapress.arizona.edu

arxiv.org

bbcearth.com

britannica.com

caltech.edu

coolcosmos.ipac.caltech.edu

crystalinks.com

cths.fr

dn.se

doi.org

dx.doi.org

elsevier.com

linkinghub.elsevier.com

eos.org

esa.int

esa.int

sci.esa.int

exploration.esa.int

feber.se

globalnet.co.uk

users.globalnet.co.uk

gu.se

science.gu.se

guardian.co.uk

harvard.edu

adsabs.harvard.edu

ui.adsabs.harvard.edu

nasa.gov

nssdc.gsfc.nasa.gov

jpl.nasa.gov

mars.nasa.gov

solarsystem.nasa.gov

mars.jpl.nasa.gov

science.nasa.gov

astrobiology.nasa.gov

www2.jpl.nasa.gov

nasa.gov

nih.gov

ncbi.nlm.nih.gov

nineplanets.org

npr.org

nytimes.com

phys.org

sciam.com

sciencenews.org

serious-science.org

seti.org

daleandersen.seti.org

space.com

spaceref.com

images.spaceref.com

theoi.com

umich.edu

esse.engin.umich.edu

universetoday.com

web.archive.org

zenodo.org