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(110–210 Earth radii) 6.36×10 6 –1.27×10 7: The space dominated by Earth's magnetic field and its magnetotail, shaped by the solar wind. [17] Earth's orbit: 299.2 million km [b] 2 AU [c] 2.99×10 8: The average diameter of the orbit of the Earth relative to the Sun. Encompasses the Sun, Mercury and Venus. [18] Inner Solar System ~6.54 AU ...
Earth's rotational velocity also varies in a phenomenon known as length-of-day variation. [172] Earth's annual orbit is elliptical rather than circular, and its closest approach to the Sun is called perihelion. In modern times, Earth's perihelion occurs around 3 January, and its aphelion around 4 July.
Earth → Solar System → Local Interstellar Cloud → Local Bubble → Gould Belt → Orion Arm → Milky Way → Milky Way subgroup → Local Group → Local Sheet → Virgo Supercluster → Laniakea Supercluster → Local Hole → Observable universe → Universe Each arrow (→) may be read as "within" or "part of".
The known densities of TNOs in this size range are remarkably low (1–1.2 g/cm 3), implying that the objects retain significant internal porosity from their formation and were never gravitationally compressed into fully solid bodies. [10]
In this map of the Observable Universe, objects appear enlarged to show their shape. From left to right celestial bodies are arranged according to their proximity to the Earth. This horizontal (distance to Earth) scale is logarithmic.
Another thing: I much prefer the resolution of File:Earth's Location in the Universe SMALLER (JPEG).jpg. It's easier to take in at full size. And also, it would be nice to have a scale (in lightyears) for each depiction, so we get an idea of how large it gets (and how tiny the Earth really is!). Jujutacular talk 02:58, 5 April 2011 (UTC)
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