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==baricentric (Jul 2022)== |
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:See [[Template_talk:Infobox_planet#edittemplateprotected]], 20:10, 4 July 2022 (UTC) |
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:New {{para|barycentric}}; (relates to {{para|orbit_ref}}) |
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{{Testcase table |
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|name=both |
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|barycentric=yes |
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|orbit_ref=<ref>Some Ref</ref> |
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| eccentricity = 0.123 |
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}} |
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{{Testcase table |
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|name=bc only |
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|barycentric=yes |
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|orbit_ref= |
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| eccentricity = 0.123 |
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}} |
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{{Testcase table |
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|name=orbitref |
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|barycentric= |
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|orbit_ref=<ref>Some Ref</ref> |
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| eccentricity = 0.123 |
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}} |
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{{Testcase table |
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|name=(no params used) |
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|barycentric= |
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|orbit_ref= |
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| eccentricity = |
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}} |
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== New parameters proposed by Bellezzasolo== |
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{{Testcase table |
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| background = #FFC2E0 |
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| discoverer = [[Roy A. Tucker]]<br />[[David J. Tholen]]<br />[[Fabrizio Bernardi]] |
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| discovery_site = [[Kitt Peak National Observatory|Kitt Peak]] |
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| named_after = [[Apep]] |
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| minorplanet = yes |
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| name = 99942 Apophis |
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| image = 2004MN4 Sormano.gif |
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| image_size = 250 |
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| caption = Animation of ''Apophis'' imaged at the [[Sormano Astronomical Observatory]] |
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| discovery_ref = |
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| discovered = 19 June 2004 |
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| mpc_name = (99942) Apophis |
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| alt_names = {{mp|2004 MN|4}} |
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| mp_category = {{mpcat|Aten}}<br />[[Near-Earth object|NEO]], [[Potentially hazardous object|PHA]] |
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| orbit_ref = |
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| epoch = 7 December 2007 ([[Julian day|JD]] 2454441.5) |
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| uncertainty = 0 |
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| observation_arc = 3635 days (9.95 yr) |
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| aphelion = {{Convert|1.09851|AU|Gm|abbr=on|lk=on}} |
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| period = 0.89 [[Julian year (astronomy)|yr]] (323.5 [[Julian year (astronomy)|d]]) |
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| abs_magnitude = 19.7 ± 0.4 |
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| semimajor = {{Convert|0.92228|AU|Gm|abbr=on}} |
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| perihelion = {{Convert|0.74605|AU|Gm|abbr=on}} |
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| eccentricity = 0.19108 |
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| inclination = 3.33129° |
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| asc_node = 204.45719° |
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| arg_peri = 126.39364° |
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| avg_speed = 30.728 km/[[second|s]] |
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| mean_anomaly = 215.53998[[Degree (angle)|°]] |
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| mean_motion = 1.11278°/day |
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| max_torino = 4 |
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| torino_scale = 0 |
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| closest_earth = 31,200 km |
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| neo_ref = <ref>{{cite web|url=https://cneos.jpl.nasa.gov/news/news146.html|title=NASA Centre for Near Earth Object Studies}}</ref> |
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| jupiter_moid = {{Convert|4.12656|AU|Gm|abbr=on}} |
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| tisserand = 6.467 |
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| moid = {{Convert|0.000659446|AU|km mi|abbr=on}} |
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| dimensions = {{Convert|0.370|km|abbr=on}} |
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| mean_radius = {{Convert|0.185|km|abbr=on}} |
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| density = ~3.2 g/cm{{sup|3}}<ref>{{cite web|url=http://www.aero.org/conferences/planetarydefense/2007papers/S1-8--Binzel-Brief.pdf|archiveurl=https://web.archive.org/web/20120412135701/http://www.aero.org/conferences/planetarydefense/2007papers/S1-8--Binzel-Brief.pdf|archivedate=2012-04-12|title=Can NEAs be Grouped by Their Common Physical Characteristics?|last=Binzel|first=Richard P.|work=Department of Earth, Atmospheric, and Planetary Sciences, [[Massachusetts Institute of Technology School of Science|Massachusetts Institute of Technology]]|publisher=aero.org|date=2007}}</ref> |
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| escape_velocity = ~0.52 km/h<ref name=estimate>assuming radius of 0.135 km and mass of 2.1e10 kg yields an escape velocity of 0.14 m/s or 0.52 km/h.</ref> |
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| mass = 6.1{{e|10}} kg (assumed) |
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| surface_grav = {{val|0.00027|u=m/s2}} (average) |
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| rotation = {{Convert|30.4|h|d|abbr=on|lk=on}}<br />tumbling:<br />precession period:<br />27.38±0.07 h<br />rotation period:<br />263±6 h<br />period of harmonic with strongest lightcurve amplitude:<br />30.56±0.01 h |
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| spectral_type = Sq |
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| albedo = 0.23 |
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| single_temperature = 270 [[kelvin|K]] |
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}} |
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== 67P/Churyumov–Gerasimenko == |
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{{Testcase table |
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| minorplanet = yes |
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| name = 67P/Churyumov–Gerasimenko |
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| image = Comet 67P on 19 September 2014 NavCam mosaic.jpg |
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| image_upright = 1.35 |
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| caption = [[Greyscale]] photograph of Comet Churyumov–Gerasimenko taken by the [[Rosetta (spacecraft)|''Rosetta'']] spacecraft |
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| discoverer = [[Klim Churyumov|Klim Ivanovych Churyumov]] <br> {{Nowrap|[[Svetlana Gerasimenko|Svetlana Ivanovna Gerasimenko]]}} |
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| discovered = 20 September 1969 |
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| discovery_site = [[Almaty|Alma-Ata]], [[Kazakh SSR]], [[Soviet Union]] <br> [[Kiev]], [[Ukrainian SSR]], Soviet Union |
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| alt_names = 1969 R1, 1969 IV, 1969h, 1975 P1, 1976 VII, 1975i, 1982 VIII, 1982f, 1989 VI, 1988i |
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| orbit_ref = |
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| epoch = 10 August 2014 ([[Julian date|JD]] 2456879.5) |
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| aphelion = {{convert|5.6829|AU|km|abbr=on}} |
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| perihelion = {{convert|1.2432|AU|km|abbr=on}} |
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| semimajor = {{convert|3.4630|AU|km|abbr=on}} |
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| eccentricity = 0.64102 |
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| period = 6.44 [[Julian year (astronomy)|yr]] |
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| inclination = 7.0405° |
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| asc_node = 50.147° |
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| mean_anomaly = 303.71° |
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| arg_peri = 12.780° |
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| time_peri = 13 August 2015 |
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| dimensions = Large lobe: <br> {{convert|4.1|*|3.3|*|1.8|km|mi|1|abbr=on}} <br> Small lobe: <br> {{convert|2.6|*|2.3|*|1.8|km|mi|1|abbr=on}} |
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| volume = {{convert|21.4|km3|abbr=on}} |
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| mass = {{val|1.0|0.1|e=13|u=kg}} |
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| density = {{convert|0.533|±|0.006|g/cm3|abbr=on}}<ref name="Lakdawalla1118">{{cite web |url=http://www.planetary.org/blogs/emily-lakdawalla/2015/dps15-1118-rosetta.html |title=DPS 2015: A little science from Rosetta, beyond perihelion |publisher=The Planetary Society |first=Emily |last=Lakdawalla |date=19 November 2015 |accessdate=8 December 2015}}</ref> |
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| porosity = 0.72<ref name="Lakdawalla1118"/> |
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| escape_velocity = ''est.'' {{convert|1|m/s|ft/s|0|abbr=on}} |
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| rotation = {{val|12.4043|0.0007|u=hours}} |
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| right_asc_north_pole= 69.3° |
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| declination = 64.1° |
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| axial_tilt = 52° |
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| albedo = 0.06 |
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| temp_name1 = [[Kelvin]] |
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| min_temp_1 = 180 |
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| max_temp_1 = 230 |
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| temp_name2 = Celsius |
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| min_temp_2 = −93 |
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| max_temp_2 = −43 |
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| temp_name3 = Fahrenheit |
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| min_temp_3 = −135 |
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| max_temp_3 = −45 |
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}} |
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== (7474) 1992 TC == |
== (7474) 1992 TC == |
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Line 32: | Line 156: | ||
| physical_characteristics = yes |
| physical_characteristics = yes |
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|spectral_type = [[Asteroid spectral types|X]] |
|spectral_type = [[Asteroid spectral types|X]] |
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|family = none |
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| abs_magnitude = 18 |
| abs_magnitude = 18 |
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}} |
}} |
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Line 59: | Line 184: | ||
| dimensions = 20×16×14 km{{sfn|Thomas Burns et al.|1998}} |
| dimensions = 20×16×14 km{{sfn|Thomas Burns et al.|1998}} |
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| volume = ~2,345 km³ |
| volume = ~2,345 km³ |
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| mass = ~2{{ |
| mass = ~2{{E-sp|15}} kg |
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| density = 0.86 g/cm³ (assumed) |
| density = 0.86 g/cm³ (assumed) |
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| surface_grav = ~0.002 [[Acceleration|m/s²]] <br /> (0.0004 g) |
| surface_grav = ~0.002 [[Acceleration|m/s²]] <br /> (0.0004 g) |
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Line 105: | Line 230: | ||
| name = Earth |
| name = Earth |
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| symbol = [[File:Earth symbol.svg|25px|Astronomical symbol of Earth]] |
| symbol = [[File:Earth symbol.svg|25px|Astronomical symbol of Earth]] |
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| image = |
| image = The Earth seen from Apollo 17.jpg |
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| image_upright = 1.25 |
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| image_alt = A planetary disk of white cloud formations, brown and green land masses, and dark blue oceans against a black background. The Arabian peninsula, Africa and Madagascar lie in the upper half of the disk, while Antarctica is at the bottom. |
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| caption = "[[The Blue Marble]]" photograph of Earth,<br>taken from ''[[Apollo 17]]'' |
| caption = "[[The Blue Marble]]" photograph of Earth,<br>taken from ''[[Apollo 17]]'' |
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| alt_names = Terra, Gaia |
| alt_names = Terra, Gaia |
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| flag = {{flagicon| |
| flag = {{flagicon|World Health Organization}} |
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| epoch = [[J2000.0]] |
| epoch = [[J2000.0]] |
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| aphelion = 152,098,232 km<br> 1.01671388 [[astronomical unit|AU]] |
| aphelion = 152,098,232 km<br> 1.01671388 [[astronomical unit|AU]] |
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Line 120: | Line 247: | ||
| arg_peri = 114.20783° |
| arg_peri = 114.20783° |
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| mean_anomaly = 357.51716° |
| mean_anomaly = 357.51716° |
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| period = 365.256363004 |
| period = {{convert|365.256363004|d|yr|comma=gaps|abbr=on|lk=out|disp=x|<br /><small>(|[[julian year (astronomy)|<sub>j</sub>]])</small>}} |
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| synodic_period = {{convert|365.242190402|d|yr|comma=gaps|abbr=on|lk=out|disp=x|<br /><small>(|[[julian year (astronomy)|<sub>j</sub>]])</small>}} |
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| avg_speed = 29.78 km/s<br>107,200 km/h |
| avg_speed = 29.78 km/s<br>107,200 km/h |
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| satellites = 1 natural (the [[Moon]])<br /> 8,300+ [[satellite|artificial]] ({{as of|2001|3|1|lc=on}})<ref>{{cite web|url=http://www.spaceref.com/news/viewpr.html?pid=4008|title=Reentry Assessment - US Space Command Fact Sheet|author=[[US Space Command]]|date=March 1, 2001|publisher=SpaceRef Interactive|accessdate=2011-05-07}}</ref> |
| satellites = 1 natural (the [[Moon]])<br /> 8,300+ [[satellite|artificial]] ({{as of|2001|3|1|lc=on}})<ref>{{cite web|url=http://www.spaceref.com/news/viewpr.html?pid=4008|title=Reentry Assessment - US Space Command Fact Sheet|author=[[US Space Command]]|date=March 1, 2001|publisher=SpaceRef Interactive|accessdate=2011-05-07}}</ref> |
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Line 137: | Line 265: | ||
| surface_grav = [[Earth's gravity|9.780327]] [[metre per second squared|m/s<sup>2</sup>]]<br>0.99732 [[g-force|''g'']] |
| surface_grav = [[Earth's gravity|9.780327]] [[metre per second squared|m/s<sup>2</sup>]]<br>0.99732 [[g-force|''g'']] |
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| escape_velocity = 11.186 km/s |
| escape_velocity = 11.186 km/s |
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| rotation = {{longitem|{{val|1.0|u=d}} <br /> <small>(24h 00m 00s) average [[solar day|synodic rotation period (solar day)]]</small>}} |
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| sidereal_day = 0.99726968 d <br>23{{smallsup|h}} 56{{smallsup|m}} 4.100{{smallsup|s}} |
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| sidereal_day = {{longitem|{{val|0.99726968|u=d}} <br /> <small>(23h 56m 4.100s)</small>}} |
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| rot_velocity = {{convert|1674.4|km/h|m/s|abbr=on}} |
| rot_velocity = {{convert|1674.4|km/h|m/s|abbr=on}} |
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| axial_tilt = 23°26'21".4119 |
| axial_tilt = 23°26'21".4119 |
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Line 152: | Line 282: | ||
| mean_temp_2 = 14 °C |
| mean_temp_2 = 14 °C |
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| max_temp_2 = 57.8 °C |
| max_temp_2 = 57.8 °C |
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| surface_equivalent_dose_rate = {{convert |2.40 |mSv/yr |μSv/h |disp=out}} |
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| surface_pressure = [[Atmosphere (unit)|101.325]] [[Pascal (unit)|kPa]] ([[Sea level|MSL]]) |
| surface_pressure = [[Atmosphere (unit)|101.325]] [[Pascal (unit)|kPa]] ([[Sea level|MSL]]) |
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| atmosphere_composition = 78.08% [[nitrogen]] (N<sub>2</sub>) (dry air)<br> 20.95% [[oxygen]] (O<sub>2</sub>)<br> 0.93% [[argon]]<br> 0.038% [[carbon dioxide]]<br>About 1% [[water vapor]] (varies with [[climate]]) |
| atmosphere_composition = 78.08% [[nitrogen]] (N<sub>2</sub>) (dry air)<br> 20.95% [[oxygen]] (O<sub>2</sub>)<br> 0.93% [[argon]]<br> 0.038% [[carbon dioxide]]<br>About 1% [[water vapor]] (varies with [[climate]]) |
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Line 163: | Line 294: | ||
|background = #ffc0c0 |
|background = #ffc0c0 |
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|discoverer = [[Seth Barnes Nicholson|S. B. Nicholson]] |
|discoverer = [[Seth Barnes Nicholson|S. B. Nicholson]] |
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|discovered = July 6, 1938<ref name="Nicholson 1938"/> |
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|discovered = July 6, 1938<ref name="Nicholson 1938">{{cite journal |last=Nicholson |first=S.B. |title=Two New Satellites of Jupiter |journal=Publications of the Astronomical Society of the Pacific |year=1938 |volume=50 |pages=292–293 |url=http://adsabs.harvard.edu//full/seri/PASP./0050//0000292.000.html |doi=10.1086/124963 |bibcode=1938PASP...50..292N}}</ref> |
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|adjectives = Lysithean |
|adjectives = Lysithean |
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|mean_orbit_radius = 11,720,000 km<ref name="Jacobson 2000" |
|mean_orbit_radius = 11,720,000 km<ref name="Jacobson 2000"/> |
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|eccentricity = 0.11<ref name="Jacobson 2000"/> |
|eccentricity = 0.11<ref name="Jacobson 2000"/> |
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|period = 259.20 d (0.69 [[Year|a]])<ref name="Jacobson 2000"/> |
|period = 259.20 d (0.69 [[Year|a]])<ref name="Jacobson 2000"/> |
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Line 194: | Line 325: | ||
| name = The Moon |
| name = The Moon |
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| apsis = gee |
| apsis = gee |
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| symbol = [[File:Moon symbol |
| symbol = [[File:Moon decrescent symbol (bold).svg|20px|☾]] |
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| image = FullMoon2010.jpg |
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| image = [[File:FullMoon2010.jpg|280px|alt=Full moon in the darkness of the night sky. It is patterned with a mix of light-tone regions and darker, irregular blotches, and scattered with varying sizes of impact craters, circles surrounded by out-thrown rays of bright ejecta.|Full moon]] |
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| image_upright = 1.25 |
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| image_alt = Full moon in the darkness of the night sky. It is patterned with a mix of light-tone regions and darker, irregular blotches, and scattered with varying sizes of impact craters, circles surrounded by out-thrown rays of bright ejecta. |
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| caption = [[Full moon]] as seen from [[Earth]]'s northern hemisphere |
| caption = [[Full moon]] as seen from [[Earth]]'s northern hemisphere |
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| periapsis = 362,570 km (0.0024 [[Astronomical unit|AU]]) <br /> (356,400–370,400 km) |
| periapsis = 362,570 km (0.0024 [[Astronomical unit|AU]]) <br /> (356,400–370,400 km) |
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| apoapsis = 405,410 km (0.0027 AU) <br /> (404,000–406,700 km) |
| apoapsis = 405,410 km (0.0027 AU) <br /> (404,000–406,700 km) |
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| semimajor = 384,399 km ({{val|0.00257|u=AU}}) |
| semimajor = 384,399 km ({{val|0.00257|u=AU}}) |
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| distance_from_sun = ''distance'' |
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| observation_arc_length = 3 days |
| observation_arc_length = 3 days |
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| eccentricity = {{val|0.0549}} |
| eccentricity = {{val|0.0549}} |
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Line 215: | Line 347: | ||
| mean_radius = {{nowrap|1,737.10 km }} {{nowrap|(0.273 Earths)}} |
| mean_radius = {{nowrap|1,737.10 km }} {{nowrap|(0.273 Earths)}} |
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| circumference = {{nowrap|10,921 km}} ([[equator]]ial) |
| circumference = {{nowrap|10,921 km}} ([[equator]]ial) |
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| surface_area = {{nowrap|3.793{{ |
| surface_area = {{nowrap|3.793{{e-sp|7}} km<sup>2</sup> }} {{nowrap|(0.074 Earths)}} |
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| volume = {{nowrap|2.1958{{ |
| volume = {{nowrap|2.1958{{e-sp|10}} km<sup>3</sup> }} {{nowrap|(0.020 Earths)}} |
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| mass = {{nowrap|7.3477{{ |
| mass = {{nowrap|7.3477{{e-sp|22}} kg }} {{nowrap|(0.0123 Earths)}} |
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| density = {{nowrap|3.3464 [[Gram per cubic centimeter|g/cm<sup>3</sup>]]}} |
| density = {{nowrap|3.3464 [[Gram per cubic centimeter|g/cm<sup>3</sup>]]}} |
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| surface_grav = {{nowrap|1.622 [[Metre per second squared|m/s<sup>2</sup>]]}} {{nowrap|(0.165 4 [[G-force|g]])}} |
| surface_grav = {{nowrap|1.622 [[Metre per second squared|m/s<sup>2</sup>]]}} {{nowrap|(0.165 4 [[G-force|g]])}} |
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Line 236: | Line 368: | ||
| mean_temp_2 = 130 K |
| mean_temp_2 = 130 K |
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| max_temp_2 = 230 K |
| max_temp_2 = 230 K |
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| surface_absorbed_dose_rate = 13.2 μGy/h |
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| surface_equivalent_dose_rate = {{convert |1.369 |mSv/d |μSv/h |disp=out}} |
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| atmosphere_ref = |
| atmosphere_ref = |
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| surface_pressure = 10<sup>−7</sup> [[Pascal (unit)|Pa]] (day) <br /> 10<sup>−10</sup> Pa (night) |
| surface_pressure = 10<sup>−7</sup> [[Pascal (unit)|Pa]] (day) <br /> 10<sup>−10</sup> Pa (night) |
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Line 243: | Line 377: | ||
| adjectives = [[wikt:lunar|lunar]], [[wikt:selenic|selenic]] |
| adjectives = [[wikt:lunar|lunar]], [[wikt:selenic|selenic]] |
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}} |
}} |
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== Mercury == |
== Mercury == |
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Line 362: | Line 497: | ||
* Trace amounts of [[argon]], [[nitrogen]], [[carbon dioxide]], [[Water|water vapor]], [[xenon]], [[krypton]] and [[neon]] |
* Trace amounts of [[argon]], [[nitrogen]], [[carbon dioxide]], [[Water|water vapor]], [[xenon]], [[krypton]] and [[neon]] |
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}} |
}} |
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}} |
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== Uranus == |
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{{Testcase table |
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| name = [[Uranus]] |
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| symbol = {{nowrap|[[File:Uranus symbol (bold).svg|24px|⛢]] ([[File:Uranus monogram (bold).svg|24px|♅]])}} |
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| image = Uranus as seen by NASA's Voyager 2 (remastered) - JPEG converted.jpg |
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| caption = Photograph of Uranus in [[False color#True color|true colour]]<br>(by ''[[Voyager 2]]'' in 1986) |
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| background = #f8f9fa |
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| discoverer = [[William Herschel]] |
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| discovered = {{#time:j F Y|{{#property:P575}}}} |
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| orbit_ref = |
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{{efn | These are the mean elements from VSOP87, together with derived quantities.}} |
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| epoch = [[J2000]] |
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| aphelion = {{convert|3006.39|Gm|AU|lk=on|abbr=on|order=flip|comma=gaps}} |
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| perihelion = {{convert|2735.56|Gm|AU|lk=off|abbr=on|order=flip|comma=gaps}} |
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| time_periastron = 17–19 August 2050<ref >Jean Meeus, ''Astronomical Algorithms'' (Richmond, Virginia: Willmann-Bell, 1998) p271. Bretagnon's complete VSOP87 model. It gives the 17th @ 18.283075301au. http://vo.imcce.fr/webservices/miriade/?forms {{Webarchive|url=https://web.archive.org/web/20210907050257/http://vo.imcce.fr/webservices/miriade/?forms |date=7 September 2021 }} IMCCE Observatoire de Paris / CNRS Calculated for a series of dates, five or ten days apart, in August 2050, using an interpolation formula from ''Astronomical Algorithms''. Perihelion came very early on the 17th. INPOP planetary theory</ref><ref name=horizons-perihelion>{{Cite web|url=https://ssd.jpl.nasa.gov/horizons_batch.cgi?batch=1&COMMAND=%27799%27&START_TIME=%272050-08-01%27&STOP_TIME=%272050-08-30%27&STEP_SIZE=%273%20hours%27&QUANTITIES=%2719%27|title=HORIZONS Planet-center Batch call for August 2050 Perihelion|website=ssd.jpl.nasa.gov|type=Perihelion for Uranus planet-center (799) occurs on 2050-Aug-19 at 18.28307512au during a rdot flip from negative to positive|publisher=NASA/JPL|access-date=2021-09-07|archive-date=7 September 2021|archive-url=https://web.archive.org/web/20210907215700/https://ssd.jpl.nasa.gov/horizons_batch.cgi?batch=1&COMMAND=%27799%27&START_TIME=%272050-08-01%27&STOP_TIME=%272050-08-30%27&STEP_SIZE=%273%20hours%27&QUANTITIES=%2719%27|url-status=live}}</ref> |
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| semimajor = {{convert|2870.972|Gm|AU|lk=off|abbr=on|order=flip|comma=gaps}} |
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| eccentricity = {{val|0.04717}} |
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| period = |
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{{plainlist | |
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* {{val|84.0205|u=[[julian year (astronomy)|yr]]}} |
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* {{nowrap|{{val|fmt=commas|30688.5|u=days}}}} |
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* {{nowrap|{{val|fmt=commas|42718}}}} Uranian [[solar day]]s |
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}} |
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| synodic_period = 369.66 days |
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| avg_speed = 6.80 km/s |
|||
| inclination = {{ubl|{{val|0.773|u=°}} to [[ecliptic]]|6.48° to [[Sun]]'s [[equator]]|0.99° to [[invariable plane]]}} |
|||
| asc_node = {{val|74.006|u=°}} |
|||
| arg_peri = {{val|96.998857|u=°}} |
|||
| mean_anomaly = {{val|142.238600|u=°}} |
|||
| satellites = [[Moons of Uranus|27]] |
|||
| flattening = {{val|0.0229|0.0008}}{{efn | Calculated using data from Seidelmann, 2007. }} |
|||
| equatorial_radius = {{nowrap|{{val|fmt=commas|25559|4|u=km}}}}<br />4.007 Earths |
|||
| polar_radius = {{nowrap|{{val|fmt=commas|24973|20|u=km}}}}<br />3.929 Earths |
|||
| mean_radius = {{nowrap|{{val|fmt=commas|25362|7|u=km}}}} |
|||
| circumference = {{nowrap|{{val|fmt=commas|159354.1|u=km}}}} |
|||
| surface_area = {{val|8.1156|e=9|u=km2}} <br /> 15.91 Earths |
|||
| volume = {{val|6.833|e=13|u=km3}} <br /> 63.086 Earths |
|||
| mass = {{val|8.6810|0.0013|e=25|u=kg}} <br /> 14.536 Earths <br /> |
|||
[[standard gravitational parameter|GM]]={{nowrap|{{val|fmt=commas|5793939|13|u=km<sup>3</sup>/s<sup>2</sup>}}}} |
|||
| density = {{val|1.27|u=g/cm3}} |
|||
| surface_grav = {{val|8.69|ul=m/s2}}<br />0.886 [[g-force|g]] |
|||
| moment_of_inertia_factor = {{val|0.23|}}<ref name="PS15">{{cite book |last2=Lissauer |first2=Jack J. |last1=de Pater |first1=Imke |author-link1=Imke de Pater |title=Planetary Sciences |date=2015 |url=https://books.google.com/books?id=stFpBgAAQBAJ&pg=PA250 |page=250 |publisher=Cambridge University Press |location=New York |isbn=978-0521853712 |edition=2nd updated |access-date=17 August 2016 |archive-date=26 November 2016 |archive-url=https://web.archive.org/web/20161126120848/https://books.google.com/books?id=stFpBgAAQBAJ&pg=PA250 |url-status=live }}</ref> (estimate) |
|||
| escape_velocity = 21.3 km/s |
|||
| rotation = {{val|−0.71832|u=days}}<br/>−17 h 14 m 23 s<br/>([[retrograde motion|retrograde]]) |
|||
| sidereal_day = {{val|-0.71833|u=day}}<br /> {{nowrap|−17 h 14 min 24 s}}<br/>(retrograde) |
|||
| rot_velocity = 2.59 km/s <br /> 9,320 km/h |
|||
| axial_tilt = 97.77° (to orbit) |
|||
| right_asc_north_pole = {{RA|17|9|15}}<br />257.311° |
|||
| declination = −15.175° |
|||
| albedo = 0.300 ([[Bond albedo|Bond]])<br />0.488 ([[Geometric albedo|geom.]])| magnitude =5.38 to 6.03 |
|||
| angular_size = 3.3″ to 4.1″ |
|||
| temp_name1 = 1 [[bar (unit)|bar]] level |
|||
| min_temp_1 = |
|||
| mean_temp_1 = {{convert|76|K|C}} |
|||
| max_temp_1 = |
|||
| temp_name2 = 0.1 bar<br />([[tropopause]]) |
|||
| min_temp_2 = 47 K |
|||
| mean_temp_2 = 53 K |
|||
| max_temp_2 = 57 K |
|||
| pronounced = {{IPAc-en|audio=uranus.ogg|ˈ|jʊər|ə|n|ə|s}} or {{IPAc-en|audio=en-us-Uranus.ogg|j|ʊ|ˈ|r|eɪ|n|ə|s}} |
|||
| adjectives = Uranian ({{IPAc-en|j|ʊ|ˈ|r|eɪ|n|i|ə|n}})<ref>{{OED|Uranian}}</ref> |
|||
| named_after = the Latin form ''Ūranus'' of the Greek god [[Uranus (mythology)|Οὐρανός]] ''Ouranos'' |
|||
| atmosphere = yes |
|||
| atmosphere_ref = |
|||
{{efn | Calculation of He, H<sub>2</sub> and CH<sub>4</sub> molar fractions is based on a 2.3% mixing ratio of methane to hydrogen and the 15/85 He/H<sub>2</sub> proportions measured at the tropopause. }} |
|||
| scale_height = 27.7 km |
|||
| atmosphere_composition = ''(Below 1.3 bar)''<br /> |
|||
'''Gases''': |
|||
* 83 ± 3% [[hydrogen]] ({{chem2|H2}}) |
|||
* 15 ± 3% [[helium]] (He) |
|||
* 2.3% [[methane]] ({{chem2|CH4}}) |
|||
* 0.009% (0.007–0.015%) [[hydrogen deuteride]] (HD) |
|||
* [[hydrogen sulfide|hydrogen sulphide]] ({{chem2|H2S}})<ref>{{cite journal |title=Detection of hydrogen sulfide above the clouds in Uranus's atmosphere |journal=Nature Astronomy |volume=2 |issue=5 |pages=420–427 |first1=Patrick G. J. |last1=Irwin |first2=Daniel |last2=Toledo |first3=Ryan |last3=Garland |first4=Nicholas A. |last4=Teanby |first5=Leigh N. |last5=Fletcher |first6=Glenn A. |last6=Orton |first7=Bruno |last7=Bézard |display-authors=1 |date=23 April 2018 |doi=10.1038/s41550-018-0432-1 |bibcode=2018NatAs...2..420I |hdl=2381/42547 |s2cid=102775371 |url=https://lra.le.ac.uk/bitstream/2381/42547/2/uranus_nature9.pdf |access-date=25 August 2019 |archive-date=28 April 2019 |archive-url=https://web.archive.org/web/20190428143940/https://lra.le.ac.uk/bitstream/2381/42547/2/uranus_nature9.pdf |url-status=dead }}</ref> |
|||
'''Ices''': |
|||
* [[ammonia]] ({{chem2|NH3}}) |
|||
* [[water (molecule)|water]] ({{chem2|H2O}}) |
|||
* [[ammonium hydrosulfide]] ({{chem2|NH4SH}}) |
|||
* [[methane hydrate]] |
|||
}} |
}} |
||
Line 370: | Line 586: | ||
| alt_names = Uranus V |
| alt_names = Uranus V |
||
| adjectives = Mirandan, Mirandian |
| adjectives = Mirandan, Mirandian |
||
| image = [[File:Miranda.jpg|200px|Miranda]] |
| image = [[File:PIA18185 Miranda's Icy Face.jpg|200px|Miranda]] |
||
| discovery = yes |
| discovery = yes |
||
| discoverer = [[Gerard P. Kuiper]] |
| discoverer = [[Gerard P. Kuiper]] |
||
Line 386: | Line 602: | ||
| surface_area = 700 000 km<sup>2</sup> |
| surface_area = 700 000 km<sup>2</sup> |
||
| volume = 54 835 000 km<sup>3</sup> |
| volume = 54 835 000 km<sup>3</sup> |
||
| mass = {{nowrap|6.59 ± 0.75{{ |
| mass = {{nowrap|6.59 ± 0.75{{E-sp|19}} [[kilogram|kg]]}} |
||
(1.103{{ |
(1.103{{E-sp|–5}} Earths) |
||
| density = {{nowrap|1.20 ± 0.15 g/cm<sup>3</sup>}} |
| density = {{nowrap|1.20 ± 0.15 g/cm<sup>3</sup>}} |
||
| surface_grav = {{Gr|0.0659|235.8|3}} [[Acceleration|m/s<sup>2</sup>]] |
| surface_grav = {{Gr|0.0659|235.8|3}} [[Acceleration|m/s<sup>2</sup>]] |
||
Line 436: | Line 652: | ||
| note = no |
| note = no |
||
}} |
}} |
||
== Test conditional designations param == |
|||
{{Testcase table |
|||
| name = 7225 Huntress |
|||
| background = #FFFFC0 |
|||
| minorplanet = yes |
|||
| discovery_ref =  <ref name="jplssd" /> |
|||
| discoverer = [[E. Bowell]] |
|||
| discovered = 22 January 1983 |
|||
| discovery_site = [[Anderson Mesa Station of the Lowell Observatory]] |
|||
|designations = some value********** |
|||
| mp_category = |
|||
| alt_names = |
|||
<!-- |
|||
| mp_category = [[main-belt]] |
|||
| alt_names = 1983 BH; 1989 XJ |
|||
| mp_name = 7225 Huntress |
|||
| named_after = [[Wesley T. Huntress]] |
|||
| adjective = adj.-sg. |
|||
| adjectives = adj.-pl. (dominates) |
|||
| pronounce = pronounce-sg. (dominates) |
|||
| pronounced = pronounce-pl. |
|||
--> |
|||
| orbit_ref =  <ref name="jplssd" /> |
|||
| epoch = 27 June 2015 ([[Julian day|JD]] 2457200.5) |
|||
| uncertainty = 0 |
|||
| observation_arc = 54.41 yr (19,872 days) |
|||
| aphelion = 2.8176 [[Astronomical unit|AU]] |
|||
| perihelion = 1.8646 AU |
|||
| semimajor = 2.3411 AU |
|||
| eccentricity = 0.2035 |
|||
| period = 3.58 [[Julian year (astronomy)|yr]] (1,308.4 days) |
|||
| mean_anomaly = 22.044[[degree (angle)|°]] |
|||
| inclination = 6.8705° |
|||
| asc_node = 275.75° |
|||
| arg_peri = 203.60° |
|||
| moid = 0.8837 AU |
|||
| rotation = 2.43995 [[hour|h]] |
|||
| albedo = |
|||
| spectral_type = S {{small|([[SMASS]]II)}} |
|||
| abs_magnitude = 13.1 mag |
|||
}} |
|||
{{hidden refs|lower-alpha}} |
{{hidden refs|lower-alpha}} |
Latest revision as of 11:04, 30 August 2024
This is the template test cases page for the sandbox of Template:Infobox planet. to update the examples. If there are many examples of a complicated template, later ones may break due to limits in MediaWiki; see the HTML comment "NewPP limit report" in the rendered page. You can also use Special:ExpandTemplates to examine the results of template uses. You can test how this page looks in the different skins and parsers with these links: |
baricentric (Jul 2022)
[edit]- See Template_talk:Infobox_planet#edittemplateprotected, 20:10, 4 July 2022 (UTC)
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New parameters proposed by Bellezzasolo
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67P/Churyumov–Gerasimenko
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(7474) 1992 TC
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Adrastea
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Carme
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Earth
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Lysithea
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The Moon
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Mercury
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Uranus
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Miranda
[edit]{{Infobox planet}} | {{Infobox planet/sandbox}} | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Nereid
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Test conditional designations param
[edit]{{Infobox planet}} | {{Infobox planet/sandbox}} | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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References
- ^ Some Ref
- ^ Some Ref
- ^ "NASA Centre for Near Earth Object Studies".
- ^ Binzel, Richard P. (2007). "Can NEAs be Grouped by Their Common Physical Characteristics?" (PDF). Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology. aero.org. Archived from the original (PDF) on 2012-04-12.
- ^ assuming radius of 0.135 km and mass of 2.1e10 kg yields an escape velocity of 0.14 m/s or 0.52 km/h.
- ^ a b Lakdawalla, Emily (19 November 2015). "DPS 2015: A little science from Rosetta, beyond perihelion". The Planetary Society. Retrieved 8 December 2015.
- ^ a b c d Evans Porco et al. 2002.
- ^ a b c d Burns Simonelli et al. 2004.
- ^ a b c d Thomas Burns et al. 1998.
- ^ a b Nicholson, S. B. (1938). "Two New Satellites of Jupiter". Publications of the Astronomical Society of the Pacific. 50: pp.292–293. Bibcode:1938PASP...50..292N. doi:10.1086/124963.
{{cite journal}}
:|pages=
has extra text (help) - ^ a b c d e f g h Jacobson, R. A. (2000). "The Orbits of Outer Jovian Satellites". Astronomical Journal. 120 (5): pp.2679–2686. Bibcode:2000AJ....120.2679J. doi:10.1086/316817.
{{cite journal}}
:|pages=
has extra text (help) - ^ a b c d e f g h i "Planetary Satellite Physical Parameters". JPL (Solar System Dynamics). 2008-10-24. Retrieved 2008-12-12.
- ^ US Space Command (March 1, 2001). "Reentry Assessment - US Space Command Fact Sheet". SpaceRef Interactive. Retrieved 2011-05-07.
- ^ a b World Geodetic System (WGS-84). Available online from National Geospatial-Intelligence Agency.
- ^ a b Vasavada, Ashwin R.; Paige, David A.; Wood, Stephen E. (19 February 1999). "Near-Surface Temperatures on Mercury and the Moon and the Stability of Polar Ice Deposits" (PDF). Icarus. 141: 179–193. Bibcode:1999Icar..141..179V. doi:10.1006/icar.1999.6175. Figure 3 with the "TWO model"; Figure 5 for pole.
- ^ Jean Meeus, Astronomical Algorithms (Richmond, Virginia: Willmann-Bell, 1998) p271. Bretagnon's complete VSOP87 model. It gives the 17th @ 18.283075301au. http://vo.imcce.fr/webservices/miriade/?forms Archived 7 September 2021 at the Wayback Machine IMCCE Observatoire de Paris / CNRS Calculated for a series of dates, five or ten days apart, in August 2050, using an interpolation formula from Astronomical Algorithms. Perihelion came very early on the 17th. INPOP planetary theory
- ^ "HORIZONS Planet-center Batch call for August 2050 Perihelion". ssd.jpl.nasa.gov (Perihelion for Uranus planet-center (799) occurs on 2050-Aug-19 at 18.28307512au during a rdot flip from negative to positive). NASA/JPL. Archived from the original on 7 September 2021. Retrieved 2021-09-07.
- ^ de Pater, Imke; Lissauer, Jack J. (2015). Planetary Sciences (2nd updated ed.). New York: Cambridge University Press. p. 250. ISBN 978-0521853712. Archived from the original on 26 November 2016. Retrieved 17 August 2016.
- ^ "Uranian". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
- ^ Irwin, Patrick G. J.; et al. (23 April 2018). "Detection of hydrogen sulfide above the clouds in Uranus's atmosphere" (PDF). Nature Astronomy. 2 (5): 420–427. Bibcode:2018NatAs...2..420I. doi:10.1038/s41550-018-0432-1. hdl:2381/42547. S2CID 102775371. Archived from the original (PDF) on 28 April 2019. Retrieved 25 August 2019.