You can find the language-neutral modification of this image here: Image:Lunarparallax_22_3_1988_neutral.png

Example of lunar parallax from 4 points on earth

This is a simulated image, combining of 4 views of the sky and the moon's location relative to the background stars at a single point in time.

The bright stars visible are the star cluster Pleiades.

The date March 22, 1988 was chosen because the moon occulted stars within the pleides as visible from North America.

NOTE: This diagram is geometrically accurate, although not physically possible to see since the moon was not actually above the horizon in half the views. Specifically you can never see the Pleiades from the south pole! They were just picked as extreme views from the earth, the limit of what might be seen from a set of four locations in a square on a great circle and a moon just above the horizon in all four locations.

Credit: Tom Ruen, Full Sky Observatory

• This image was generated by my own solar system viewing software.
• Source bitmap for projection from Nasa's Clementine Spacecraft:
  • USGS: Global simple cylindrical projection at 10 km/pixel. (https://astrogeology.usgs.gov/Projects/Clementine/images/albedo.simp750.jpeg)

本作品已被作者Tomruen释出到公有领域。这适用于全世界。 在一些国家这可能不合法；如果是这样的话，那么： Tomruen无条件地授予任何人以任何目的使用本作品的权利，除非这些条件是法律规定所必需的。

en:Image:Lunarparallax 22 3 1988.png

history on en: 02:12, 21 May 2004 . . en:user:Tomruen . . 554x508 (31311 bytes) (Example of lunar parallax from 4 points on earth)

我，本作品著作权人，释出本作品至公有领域。这适用于全世界。 在一些国家这可能不合法；如果是这样的话，那么： 我无条件地授予任何人以任何目的使用本作品的权利，除非这些条件是法律规定所必需的。