Sátúrnù

Sátúrnù ni is the sixth planeti kefa si Orun ati planeti keji totobijulo ninu Sistemu Orun, leyin Jupiteri.

Sátúrnù - Saturn  

Saturn imaged by the Cassini Orbiter
Ìfúnlọ́rúkọ
Ìpolongo	i /ˈsætərn/[1]
Alápèjúwe	Saturnian, Cronian
Àwọn ìhùwà ìgbàyípo[2][3]
Àsìkò J2000.0
Aphelion	1,513,325,783 km 10.115 958 04 AU
Perihelion	1,353,572,956 km 9.048 076 35 AU
Semi-major axis	1,433,449,370 km 9.582 017 20 AU
Eccentricity	0.055 723 219
Àsìkò ìgbàyípo	10,759.22 days 29.4571 yr 24,491.07 Saturn solar days[4]
Synodic period	378.09 days[5]
Average orbital speed	9.69 km/s[5]
Mean anomaly	320.346 750°
Inclination	2.485 240° to Ecliptic 5.51° to Sun’s equator 0.93° to invariable plane[6]
Longitude of ascending node	113.642 811°
Argument of perihelion	336.013 862°
Satellites	~ 200 observed (61 with secure orbits)
Àwọn ìhùwà àdánidá
Ìfẹ̀kiri alágedeméjì	60,268 ± 4 km[7][8] 9.4492 Earths
Ìfẹ̀kiri olóòpó	54,364 ± 10 km[7][8] 8.5521 Earths
Flattening	0.097 96 ± 0.000 18
Ààlà ojúde	4.27 × 1010 km²[8][9] 83.703 Earths
Ìpọ̀sí	8.2713 × 1014 km³[5][8] 763.59 Earths
Àkójọ	5.6846 × 1026 kg[5] 95.152 Earths
Iyeìdáméjì ìṣùpọ̀	0.687 g/cm³[5][8] (less than water)
Equatorial surface gravity	10.44 m/s²[5][8] 1.065 g
Escape velocity	35.5 km/s[5][8]
Sidereal rotation period	10.57 hours[10] (10 hr 34 min)
Equatorial rotation velocity	9.87 km/s[8] 35,500 km/h
Axial tilt	26.73°[5]
North pole right ascension	2h 42m 21s 40.589°[7]
North pole declination	83.537°[7]
Albedo	0.342 (Bond) 0.47 (geometric)[5]
Ìgbónásí ojúde    1 bar level    0.1 bar	min mean max 134 K[5] 84 K[5]
Apparent magnitude	+1.47 to −0.24[11]
Angular diameter	14.5"–20.1"[5] (excludes rings)
Afẹ́fẹ́àyíká[5]
Ìga òṣùwọ̀n	59.5 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)

Itokasi

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. Retrieved 2007-08-08.—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 instantaneous osculating values at the precise J2000 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". Retrieved 2009-08-13.
5. Williams, Dr. David R. (September 7, 2006). "Saturn Fact Sheet". NASA. Retrieved 2007-07-31.
6. "The MeanPlane (Invariable plane) of the Solar System passing through the barycenter". 2009-04-03. Archived from the original on 2009-04-20. Retrieved 2009-04-10. (produced with Solex 10 Archived 2015-05-24 at the Wayback Machine. written by Aldo Vitagliano; see also Invariable plane)
7. Seidelmann, 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. Bibcode 2007CeMDA..98..155S. doi:10.1007/s10569-007-9072-y.
8. Refers 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. Retrieved 2007-10-14.