Waxaraxir

Waxaraxir
	Global radar view of the surface from Magellan radar imaging between 1990 and 1994
Calaamadayn
Ku Dhawaaqitaan	i/nəs/
Sifo	Venusian or (rarely) Cytherean, Venerean
Sifooyin gaara
	Miisaan J2000
Wareegdhow	108939000 km; 0.728213 AU;
Wareegfog	107477000 km; 0.718440 AU;
Gobol Goobo	108208000 km; 0.723327 AU;
Iskuwareeg Yar	0.0067
Wareega Sanad	224.701 d; 0.615198 yr; 1.92 Venus solar day;
Wakhiga Wareega	583.92 days
Iskucelceliska Xawaaraha Wareega	35.02 km/s
Iskucelceliska Wareega	50.115°
Janjeedhka	3.39458° to Ecliptic; 3.86° to Sun’s equator; 2.19° to Invariable plane;
Loolasha u yaryihiin	76.678°
Wakhtidhan	55.186°
Dayaxyo	None
Gacan	6051.8±1.0 km; 0.9499 Earths;
Sariibadaha	0
Bedka oogada	4.60×108 km2; 0.902 Earths;
Mug	9.28×1011 km3; 0.866 Earths;
Cuf	4.8676×1024 kg; 0.815 Earths;
Macnaha Cufnaanta	5.243 g/cm3
Equatorial surface gravity	8.87 m/s2; 0.904 g;
Escape velocity	10.36 km/s
Mudo wareeg	−243.0185 d (Retrograde)
Xawaare wareeg	6.52 km/h (1.81 m/s)
Foorar	177.36°
Cirifka woqoooyi right ascension	18h 11m 2s; 272.76°;
Cirifka woqooyi declination	67.16°
	0.67 (geometric); 0.90 (Bond);
Apparent magnitude	brightest −4.9; −3.8;
Angular diameter	9.7″ to 66.0″
Jawiga
Cadaadiska oogada	92 bar (9.2 MPa)
Qaab dhismeedka	≈ 96.5% carbon dioxide; ≈ 3.5% nitrogen; 0.015% sulfur dioxide; 0.007% argon; 0.002% water vapour; 0.0017% carbon monoxide; 0.0012% helium; 0.0007% neon; trace carbonyl sulfide; trace hydrogen chloride; trace hydrogen fluoride;

Waxaraxir (Af-Ingiriis: Venus; Af-Carabi: الزهرة; summad : ♀) waa meeraha labaad ee baho cadceedeed iyo kan ugu dhod dhulka. Meeraha Waxaraxir wuxuu ku wareegaa qoraxda 224.7 maalmaha dunida, taasi oo u dhiganta sanadka meerahaasi.^[3] Intaas waxaa dheer, meerahani wuxuu ka tirsan yahay 4ta meere dhagaxleda ah ee laga helo Bahda Qoraxdu Midaysay.^[4]

Qoraalka gudaha oo kooban

Hordhac

Xajmiga Waxarxir marka la barbardhigo Dhulka

Sidaan horay usoo sheegnay, Meeraha Waxaraxir wuxuu ka mid yahay afarta meere ee dhagaxleyda ah, taasi oo dhulku ka mid yahay. Sidoo kale, Waxaraxir waxay aad ugu xug iyo xajmi dhowdahay dhulka, waxaana guud ahaan lagu naaneysaa "Mataanka Dhulka".^[5]

Nidaamka Meeraha

Waxaraxir waa meeraha keliya ee baho cadceedeed kuwaa oo maalin ka dheer tahay sanadka sababtoo ah waxay ku wareegta qorraxda 225 maalmood, waxayse u baahan tahay oo buuxda 243 maalmood isbedel ku wareeg ah oo keliya oo hareeraha dhidibka u gaar ah . Like kale tan iyo Qarniyadii hore ee meerayaasha West loo yaqaan ( kuwa soo baxay iyada oo Saatun ) ayaa loo magacaabay by ahaa Gariig , kaas oo magac hiir our ( Giriigtu waxay sidoo kale sheegaysaa in Venus iyo Triton la xiriira ) . Waxaa la magacaabay ka dib markii ay ilaahadda jacayl Aphrodite , iyo , sida la meerayaasha kale , nidaamka wuxuu u sarreeyey by Romans -ka kuwaas oo magacyadooda ka dibna dhaxlo . Jacaylkoodii ilaahadda magacaabay Venus . Meeraha ayaa waxaa lagu yaqaan ka hor Qarniyadii hore iyo lahaayeen magacyo kala duwan ee dhaqamada kala duwan . Maaddaama ay inta badan waxaa lagu arki karaa macnaha of qorrax iyo qorrax ka soo baxa , waxa la yidhaahdaa waa star fiidkii iyo xiddigta waaberi oo ku qoran afaf dhawr ah . Venus sidoo kale waa jirka oo u nacaan, oo waa muuqataa in Samada ka dib markii Qoraxda iyo Dayaxa .

Muuqaalo

Meeraha Waxaraxir
dayaxa Dione ee meeraha Raage.
dayaxa Mimas ee meeraha Raage.
dayaxa Hyperion ee meeraha Raage.

Sidoo kale fiiri

Xigasho

↑ Lakdawalla, Emily (21 September 2009), Venus Looks More Boring than You Think It Does, Planetary Society Blog (retrieved 4 December 2011)
↑ name="Seidelmann2007"
↑ Lawrence, Pete (2005). "In Search of the Venusian Shadow". Digitalsky.org.uk. Archived from the original on 11 June 2012. Retrieved 13 June 2012.
↑ 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: E00B24. Bibcode:2008JGRE..11300B24H. doi:10.1029/2008JE003134.
↑ Lopes, Rosaly M. C.; Gregg, Tracy K. P. (2004). Volcanic worlds: exploring the Solar System's volcanoes. Springer Publishing. p. 61. ISBN 978-3-540-00431-8.

[1] Lakdawalla, Emily (21 September 2009), Venus Looks More Boring than You Think It Does, Planetary Society Blog (retrieved 4 December 2011)

[2] ="Seidelmann2007"

[3] Lawrence, Pete (2005). "In Search of the Venusian Shadow". Digitalsky.org.uk. Archived from the original on 11 June 2012. Retrieved 13 June 2012.

[4] 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: E00B24. Bibcode:2008JGRE..11300B24H. doi:10.1029/2008JE003134.

[5] Lopes, Rosaly M. C.; Gregg, Tracy K. P. (2004). Volcanic worlds: exploring the Solar System's volcanoes. Springer Publishing. p. 61. ISBN 978-3-540-00431-8.

[3]

[4]

[2]

[5]