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File:Newton revolving orbit e0.6 precession.ogv

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Newton_revolving_orbit_e0.6_precession.ogv ‎(Ogg Theora video file, length 32 s, 400 × 400 pixels, 380 kbps, file size: 1.46 MB)

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English: OGG Theora version of Image:Precessing Kepler orbit 280frames e0.6 smaller.gif.
Polski: Zgodnie z twierdzeniem Newtona o obrotach orbit, planety krążą wokół Słońca po orbitach eliptycznych (owalnych), które obracają się stopniowo wraz z upływem czasu (ruch peryhelium). Mimośród tej elipsy jest wyolbrzymiony dla celów wizualizacji. Większość orbit w Układzie Słonecznym ma znacznie mniejsze mimośrody, dzięki czemu są prawie kołowe.
Čeština: Podle Newtonova theorému oběžných drah obíhají planety kolem Slunce po eliptických (oválných) oběžných drahách, které se postupně otáčejí (apsidálni precese). Excentricita dráhy je zvýrazněna v tomto videu. Většina oběžných planetárních drah ve sluneční soustavě má však mnohem nižší excentricitu a jejich oběžné dráhy jsou téměř kruhové.
Македонски: Според Њутновата теорема, планетите околу Сонцето следат елиптични (јајчести) орбити кои постепено се вртат (перихелна прецесија).
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Author WillowW
 
This video was created with Blender by ogg.

Assessment[edit]

Media of the day This file was selected as the media of the day for 25 September 2016. It was captioned as follows:
English: According the Newton's theorem of revolving orbits the planets revolving the Sun follow elliptical (oval) orbits that rotate gradually over time (apsidal precession). The eccentricity of this ellipse is exaggerated for visualization. Most orbits in the Solar System have a much smaller eccentricity, making them nearly circular.
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Čeština: Podle Newtonova theorému oběžných drah obíhají planety kolem Slunce po eliptických (oválných) oběžných drahách, které se postupně otáčejí (apsidálni precese). Excentricita dráhy je zvýrazněna v tomto videu. Většina oběžných planetárních drah ve sluneční soustavě má však mnohem nižší excentricitu a jejich oběžné dráhy jsou téměř kruhové.
English: According the Newton's theorem of revolving orbits the planets revolving the Sun follow elliptical (oval) orbits that rotate gradually over time (apsidal precession). The eccentricity of this ellipse is exaggerated for visualization. Most orbits in the Solar System have a much smaller eccentricity, making them nearly circular.
Македонски: Според Њутновата теорема, планетите околу Сонцето следат елиптични (јајчести) орбити кои постепено се вртат (перихелна прецесија).
Polski: Zgodnie z twierdzeniem Newtona o obrotach orbit, planety krążą wokół Słońca po orbitach eliptycznych (owalnych), które obracają się stopniowo wraz z upływem czasu (ruch peryhelium). Mimośród tej elipsy jest wyolbrzymiony dla celów wizualizacji. Większość orbit w Układzie Słonecznym ma znacznie mniejsze mimośrody, dzięki czemu są prawie kołowe.

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Date/TimeThumbnailDimensionsUserComment
current16:50, 15 August 200832 s, 400 × 400 (1.46 MB)WillowW (talk | contribs){{Information |Description=Improved version with thicker curve for the orbit. |Source= |Date=15 August 2008 |Author=WillowW |Permission= |other_versions= }}
12:15, 15 August 200832 s, 400 × 400 (1.62 MB)WillowW (talk | contribs){{Information |Description={{en|1=OGG Theora version of Image:Precessing Kepler orbit 280frames e0.6 smaller.gif.}} |Source=Own work by uploader |Author=WillowW |Date=15 August 2008 |Permission= |other_versions= }} <!--{{ImageUpload

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VP9 360P 98 kbps Completed 21:47, 4 September 2018 11 s
Streaming 360p (VP9) Not ready Unknown status
VP9 240P 48 kbps Completed 21:47, 4 September 2018 7.0 s
Streaming 240p (VP9) 48 kbps Completed 00:38, 6 February 2024 1.0 s
WebM 360P 484 kbps Completed 13:42, 9 February 2017 12 s
Streaming 144p (MJPEG) 444 kbps Completed 21:36, 15 November 2023 2.0 s

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