Eʼelyaaígíí:Terrestrial_planet_size_comparisons.jpg
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![Eʼelyaaígíí:Terrestrial planet size comparisons.jpg](http://upload.wikimedia.org/wikipedia/commons/thumb/b/b9/Terrestrial_planet_size_comparisons.jpg/800px-Terrestrial_planet_size_comparisons.jpg)
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Summary
DescriptionTerrestrial planet size comparisons.jpg |
Deutsch: Diese Darstellung zeigt die ungefähren relativen Größen der erdähnlichen Planeten, von links nach rechts: Merkur, Venus, Erde und Mars. Die gezeigten Abstände sind hingegen nicht maßstabsgerecht.
Ein erdähnlicher Planet ist ein Planet, der hauptsächlich aus Silikatgestein besteht. Solche Planeten unterscheiden sich wesentlich von Gasriesen. Letztere haben nicht unbedingt eine feste Oberfläche und bestehen hauptsächlich aus einer Mischung von Wasserstoff, Helium und Wasser in verschiedenen physikalischen Zuständen. Erdähnliche Planeten haben alle ungefähr dieselbe Struktur: einen metallenen Kern, größtenteils aus Eisen, darum ein Silikatmantel. Erdähnliche Planeten haben Schluchten, Krater, Berge, ggf. Vulkane und eine Atmosphäre.
English: This diagram shows the approximate relative sizes of the terrestrial planets, from left to right: Mercury, Venus, Earth and Mars. Distances are not to scale.
A terrestrial planet is a planet that is primarily composed of silicate rocks. The term is derived from the Latin word for Earth, "Terra", so an alternate definition would be that these are planets which are, in some notable fashion, "Earth-like". Terrestrial planets are substantially different from gas giants, which might not have solid surfaces and are composed mostly of some combination of hydrogen, helium, and water existing in various physical states. Terrestrial planets all have roughly the same structure: a central metallic core, mostly iron, with a surrounding silicate mantle. Terrestrial planets have canyons, craters, mountains, volcanoes and secondary atmospheres. Français : Les planètes telluriques, de gauche à droite : Mercure, Vénus, Terre, et Mars.
Italiano: Questo diagramma mostra approssimativamente le dimensioni relative dei pianeti terrestri, da sinistra a destra: Mercurio, Venere, Terra e Marte. Le distanze non sono in scala.
Un pianeta terrestre è un pianeta composto per lo più di roccia e metalli. Il termine deriva direttamente dal nome del nostro pianeta (anche in latino), "Terra", quindi una definizione alternativa sarebbe che questi pianeti sonoin qualche modo simili alla Terra. I pianeti terrestri sono sostanzialmente diversi dai giganti gassosi, che potrebbero non avere una superficie solida e sono composti soprattutto di qualche combinazione di idrogeno, elio e acqua presenti in vari stati fisici. I pianeti terrestri hanno tutti più o meno la stessa struttura: un nucleo metallico, soprattutto ferroso, circondato da un mantello di silicato. I pianeti terrestri hanno canyon, crateri, montagne, vulcani e atmosfere secondarie. Русский: Планеты земной группы, слева направо: Меркурий, Венера, Земля, Марс. |
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http://solarsystem.nasa.gov/multimedia/gallery/terr_sizes.jpg Uploaded to commons from the english wikipedia; description page was here
Also previously uploaded as Image:Terr sizes.jpg
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Author | wikipedia user Brian0918 | ||||||
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Captions
Items portrayed in this file
depicts English
inception English
20 Wóózhchʼį́į́d 2006
media type English
image/jpeg
łahgo ádaalyaaígíí
Ńtʼę́ę́ʼígíí yíníʼį́įgo biniiyé, naʼalkid/yoołkáłígíí bikáaʼgi "click" ádíílííł
naʼalkid/yoołkáłígíí | thumbnailígíí | naaniigo/náásee | Choyoołʼįįhí | haneʼ | |
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kʼadígíí | 20:39, 4 Níłchʼitsoh 2018 | ![]() | 1,500 × 653 (314 KIIŁTSOHʼÍÍŁKÉ) | Allice Hunter | Correcting Mars |
17:21, 3 Níłchʼitsoh 2018 | ![]() | 1,500 × 653 (315 KIIŁTSOHʼÍÍŁKÉ) | Allice Hunter | updated: correcting the color of Mars. Based on image of Mars >> File:OSIRIS Mars true color.jpg. There was no distortion in size | |
22:37, 15 Yaʼiishjáástsoh 2012 | ![]() | 1,500 × 653 (276 KIIŁTSOHʼÍÍŁKÉ) | Ubiquinoid | updated: correcting for apparent undersizing of Venus (from 90 to 95% (true) of Earth's diameter) - based on image of Venus w/NASA cloup map (resized) at http://cronodon.com/PlanetTech/Venus.html; centred | |
14:52, 15 Yaʼiishjáástsoh 2012 | ![]() | 1,500 × 653 (79 KIIŁTSOHʼÍÍŁKÉ) | Ubiquinoid | updated: correcting for apparent undersizing of Venus (95% of Earth's diameter) - based on image of Venus w/cloup map (resized) at http://cronodon.com/PlanetTech/Venus.html | |
23:50, 27 Níłchʼitsoh 2007 | ![]() | 1,500 × 653 (456 KIIŁTSOHʼÍÍŁKÉ) | Crotalus horridus~commonswiki | Created identical and more compact version using the "Huffman optimized" feature of jpegcrop. Nothing else has been changed. | |
23:27, 14 Yaʼiishjááshchilí 2006 | ![]() | 1,500 × 653 (488 KIIŁTSOHʼÍÍŁKÉ) | Nicke L | {{Information| |Description= The inner planets, from left to right: en:Mercury, en:Venus, en:Earth, and en:Mars Source: http://solarsystem.nasa.gov/multimedia/gallery/terr_sizes.jpg |Source= |Date= |Author=User [[:en:User:Brian0918|Br |
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Width | 1,500 px |
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Height | 653 px |
Bits per component |
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Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Software used | Adobe Photoshop CS6 (Windows) |
File change date and time | 16:37, 4 Níłchʼitsoh 2018 |
Exif version | 2.21 |
Color space | Uncalibrated |
Unique ID of original document | 9BD8C001C67BC0A0DCDCBFB63D708BEF |
Date and time of digitizing | 09:11, 3 Níłchʼitsoh 2018 |
Date metadata was last modified | 12:37, 4 Níłchʼitsoh 2018 |
IIM version | 60,580 |