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Sátúrnù

Lát'ọwọ́ Wikipedia, ìwé ìmọ̀ ọ̀fẹ́
Sátúrnù - Saturn  ♄
The planet Saturn during equinox
Saturn imaged by theCassini Orbiter
Ìfúnlọ́rúkọ
ÌpolongoGbígbọ́i/ˈsætərn/[1]
AlápèjúweSaturnian, Cronian
ÀsìkòJ2000.0
Aphelion1,513,325,783 km
10.115 958 04AU
Perihelion1,353,572,956 km
9.048 076 35 AU
Semi-major axis1,433,449,370 km
9.582 017 20 AU
Eccentricity0.055 723 219
Àsìkò ìgbàyípo10,759.22 days
29.4571yr
24,491.07 Saturnsolar days[4]
Synodic period378.09 days[5]
Average orbital speed9.69 km/s[5]
Mean anomaly320.346 750°
Inclination2.485 240° toEcliptic
5.51° toSun’s equator
0.93° toinvariable plane[6]
Longitude of ascending node113.642 811°
Argument of perihelion336.013 862°
Satellites~ 200 observed (61 with secure orbits)
Àwọn ìhùwà àdánidá
Ìfẹ̀kirialágedeméjì60,268 ± 4 km[7][8]
9.4492 Earths
Ìfẹ̀kiriolóòpó54,364 ± 10 km[7][8]
8.5521 Earths
Flattening0.097 96 ± 0.000 18
Ààlà ojúde4.27 × 1010 km²[8][9]
83.703 Earths
Ìpọ̀sí8.2713 × 1014 km³[5][8]
763.59 Earths
Àkójọ5.6846 × 1026 kg[5]
95.152 Earths
Iyeìdáméjììṣùpọ̀0.687 g/cm³[5][8]
(less thanwater)
Equatorial surface gravity10.44m/s²[5][8]
1.065g
Escape velocity35.5 km/s[5][8]
Sidereal rotation
period
10.57 hours[10]
(10 hr 34 min)
Equatorial rotation velocity9.87 km/s[8]
35,500 km/h
Axial tilt26.73°[5]
North poleright ascension2h 42m 21s
40.589°[7]
North poledeclination83.537°[7]
Albedo0.342 (Bond)
0.47 (geometric)[5]
Ìgbónásí ojúde
   1 bar level
   0.1 bar
minmeanmax
134 K[5]
84 K[5]
Apparent magnitude+1.47 to −0.24[11]
Angular diameter14.5"–20.1"[5]
(excludes rings)
Afẹ́fẹ́àyíká[5]
Ìga òṣùwọ̀n59.5 km
Ìkósínú
~96%Hydrogen (H2)
~3%Helium
~0.4%Methane
~0.01%Ammonia
~0.01%Hydrogen deuteride (HD)
0.000 7%Ethane
Ices:
Ammonia
water
ammonium hydrosulfide(NH4SH)

Sátúrnù ni is the sixthplaneti kefa siOrun ati planeti keji totobijulo ninuSistemu Orun, leyinJupiteri.


Àyọkà yìí tàbí apá rẹ̀ únfẹ́ àtúnṣe sí.

Ẹ lefẹ̀ jù báyìí lọ tàbí kí ẹṣàtúnṣe rẹ̀ lọ́nà tí yíò mu kúnrẹ́rẹ́. Ẹ ran Wikipedia lọ́wọ́ látifẹ̀ẹ́ jù báyìí lọ.

Itokasi

[àtúnṣe |àtúnṣe àmìọ̀rọ̀]
  1. Walter, Elizabeth (April 21, 2003). Cambridge Advanced Learner's Dictionary (Second ed.). Cambridge University Press. ISBN 0521531063. 
  2. Yeomans, Donald K. (2006-07-13)."HORIZONS System". NASA JPL. Retrieved2007-08-08. —At the site, go to the "web interface" then select "Ephemeris Type: ELEMENTS", "Target Body: Saturn Barycenter" and "Center: Sun".
  3. Orbital elements refer to the barycenter of the Saturn system and are the instantaneousosculating values at the preciseJ2000 epoch. Barycenter quantities are given because, in contrast to the planetary centre, they do not experience appreciable changes on a day-to-day basis from to the motion of the moons.
  4. Seligman, Courtney."Rotation Period and Day Length". Retrieved2009-08-13. 
  5. 5.005.015.025.035.045.055.065.075.085.095.105.115.12Williams, Dr. David R. (September 7, 2006)."Saturn Fact Sheet". NASA. Archived fromthe original on 2010-01-06. Retrieved2007-07-31. 
  6. "The MeanPlane (Invariable plane) of the Solar System passing through the barycenter". 2009-04-03.Archived from the original on 2009-04-20. Retrieved2009-04-10.  (produced withSolex 10Archived 2015-05-24 at theWayback Machine. written by Aldo Vitagliano; see alsoInvariable plane)
  7. 7.07.17.27.3Seidelmann, P. Kenneth; Archinal, B. A.; A’hearn, M. F.; et al. (2007). "Report of the IAU/IAGWorking Group on cartographic coordinates and rotational elements: 2006". Celestial Mech. Dyn. Astr. 90 (3): 155–180. Bibcode2007CeMDA..98..155S. doi:10.1007/s10569-007-9072-y. 
  8. 8.08.18.28.38.48.58.68.7Refers to the level of 1 bar atmospheric pressure
  9. NASA: Solar System Exploration: Planets: Saturn: Facts & Figures
  10. 'Astronews' (New Spin For Saturn). Astronomy. November 2009. p. 23. 
  11. Schmude, Richard W Junior (2001)."Wideband photoelectric magnitude measurements of Saturn in 2000". Georgia Journal of Science. Retrieved2007-10-14. 
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