Mart
Cummey
| Mart | |||||
|---|---|---|---|---|---|
| Sorçh | planaid sthie as planaid çheumooie | ||||
| Epennym | Mars, Ares, as aile | ||||
| Moir-red | y Ghrian | ||||
| Red lhiennoo | |||||
| Amm | J2000.0 | ||||
| Croo | 4,540 millioon dy vleeantyn RC | ||||
| Fysserree ishigagh | |||||
| Apoapsis | 249,260,000 km[1] | ||||
| Periapsis | 206,650,000 km (arg (ω): 336.05637)[1] | ||||
| Essylys lieh-vooar a | 227,936,636 km[2] | ||||
| Corrid e | 0.09339[3] | ||||
| Amm cruinlagh P | 686.98 d[1] | ||||
| Amm cruinlagh (synodagh) | 779.94 d | ||||
| Mean-amreiltagh M | 19.412 °[4] | ||||
| Cleayn i | 1.84969 ° ↔ ecliptagh[3] 5.65 ° ↔ mean-chiarkyl ny Greiney 1.67 ° ↔ mean-chiarkyl neuchaghlaaee[5] | ||||
| Foddid y noad ardjeeagh Ω | 49.55954 °[3] | ||||
| Troghyn fishigagh as rollageagh meadragh | |||||
| Foddeeaght veih'n Dowan | 54,600,000 km (perigee (en) 401,400,000 km (apogee (en) | ||||
| Craue raadeeoil | mean radius (en) equatorial radius (en) poullagh: 3,379.2 km[7] | ||||
| Lheanaghey | 0.00589[1] | ||||
| Mooadys baghtal (V) | −2.94[8] | ||||
| Crantessen uillinagh | 3.5 "–25.1 "[9] | ||||
| Eaghtyr y vaare | 144,798,500 km²[10] | ||||
| Glout | 641.691 Yg[11] | ||||
| Thummid | 163,180,000,000 km³[10] | ||||
| Mean-ghlooaght | 3.9335 g/cm³[12] | ||||
| Amm çhyndaaee | 24.6229633 h[13] | ||||
| Ym-hayrn eaghtyragh | 3.71 m/s²[11] | ||||
| Albedo | 0.17 (albedo towse-oaylleeagh)[14] 0.25 (albedo Bond)[4] | ||||
| Çhiassid eaghtyragh |
| ||||
| Aeraght | Co-heiy | ||||
| Ayrn jeh | y Grianchorys sthie | ||||
Ta Mart ny kiaroo planaid magh ass y ghrian ayns Corys ny Greiney. T'ee soit eddyr y Chruinney as y Chryss Roltageagh. Ta'n ennym "y planaid jiarg" currit urree ny keayrtyn er son daah thalloo y phlanaid.
Imraaghyn
[reagh | reagh y bun]- 1 2 3 4 5 6 7 "nssdc.gsfc.nasa.gov".
{{cite web}}:|archive-url=requires|archive-date=(help) - ↑ Imraait ayns: Allen's astrophysical quantities. Author: Arthur N. Cox. Publisher: Springer Science+Business Media. Çhengey yn obbyr ny yn ennym: Baarle. Publication date: 2000.
- 1 2 3 E. Myles Standish (15 Toshiaght Arree 2015). "Keplerian elements for approximate positions of the major planets" (PDF). Keplerian elements for approximate positions of the major planets (ayns Baarle).
- 1 2 "nssdc.gsfc.nasa.gov".
{{cite web}}:|archive-url=requires|archive-date=(help) - ↑ E. Myles Standish (15 Toshiaght Arree 2015). "Keplerian elements for approximate positions of the major planets". Explanatory Supplement to the Ephemeris (ayns Baarle).
- 1 2 Jürgen Oberst (Toshiaght Arree 2011). "Report of the IAU Working Group on Cartographic Coordinates and Rotational Elements: 2009". Celestial Mechanics and Dynamical Astronomy (ayns Baarle) (2): 101–135. doi:10.1007/S10569-010-9320-4.
- ↑ James B. Garvin (1 Boaldyn 1999). "The global topography of Mars and implications for surface evolution.". Science (ayns Baarle) (5419): 1495–1503. doi:10.1126/SCIENCE.284.5419.1495.
- ↑ "nssdc.gsfc.nasa.gov". Er ny hashtey veih y lhieggan bunneydagh er 2 Jerrey Geuree 2025.
- ↑ "NASA FACTS" (ayns Baarle). NASA.
- 1 2 "nssdc.gsfc.nasa.gov".
- 1 2 "ssd.jpl.nasa.gov".
- ↑ Harold Y. McSween (Jerrey Geuree 2002). "The rocks of Mars, from far and near". Meteoritics & Planetary Science (1): 7–25. doi:10.1111/J.1945-5100.2002.TB00793.X.
- 1 2 3 Imraait ayns: Thermal properties of the surface of Mars. Author: Anatoliy P. Vidmachenko. Page(s): 243-252. Çhengey yn obbyr ny yn ennym: Baarle. Publication date: Mayrnt 2023.
- ↑ "The magnitude and albedo of Mars". Icarus (ayns Baarle) (2): 404–416. Mee ny Nollick 2007. doi:10.1016/J.ICARUS.2007.07.011.
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