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Original file (WebM audio/video file, VP8/Opus, length 1 min 28 s, 1,280 × 720 pixels, 1.29 Mbps overall, file size: 13.56 MB) This is a file from the Wikimedia Commons . Information from its description page there is shown below.
Equatorial gravity: m/s 2 g: 274.0 27.94 Escape velocity: km/s: 617.7 Rotation period days: 25.38 Orbital period about Galactic Center [4] million years 225–250 Mean orbital speed [4] km/s: ≈ 220 Axial tilt to the ecliptic: deg. 7.25 Axial tilt to the galactic plane: deg. 67.23 Mean surface temperature: K: 5,778 Mean coronal temperature [5 ...
Date/Time Thumbnail Dimensions User Comment; current: 16:34, 10 December 2022: 1,871 × 622 (40 KB) Wikideas1: updated with Earth's moon gravity: 07:46, 9 December 2022: 1,873 × 622 (36 KB) Wikideas1: Uploaded own work with UploadWizard
[8] [13] Long years of continuous observation has found that the determination of even zonal, normalized gravity coefficient C l=2, m=0, and odd zonal, normalized gravity coefficient C l=3, m=0 are crucial for outlining the time-variable gravity due to such mass exchange, [24] [8] [31] [32] where is the degree while is the order.
The methodology used in Timelapse of the Entire Universe.. In 2012, a short, one-and-a-half-minute film by Boswell, Our Story in 1 Minute, is published.It is a shorter version of Timelapse of the Entire Universe, specifically in one minute and 29 seconds, and used closed captions to evoke reflection on humanity.
NASA’s Perseverance Mars rover used its right-front navigation camera to capture this first view over the rim of Jezero Crater on Dec. 10, 2024, the 1,354th Martian day, or sol, of the mission.
Highest Lowest Highest Lowest Highest Lowest Sun: N/A 5,000,000 K In a solar flare [33] 1240 K In a sunspot [34] Mercury: 3 kilometres (1.9 mi) Caloris Montes, northwest Caloris Basin rim mountains [35] [36] 723 K Dayside of Mercury [37] 89 K Permanently shaded polar craters [38] Venus: 11 kilometres (6.8 mi) Maxwell Montes, Ishtar Terra [39 ...
The gravity g′ at depth d is given by g′ = g(1 − d/R) where g is acceleration due to gravity on the surface of the Earth, d is depth and R is the radius of the Earth. If the density decreased linearly with increasing radius from a density ρ 0 at the center to ρ 1 at the surface, then ρ ( r ) = ρ 0 − ( ρ 0 − ρ 1 ) r / R , and the ...