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)

此作品已由其作者，Tomruen，釋出至公有領域。此授權條款在全世界均適用。 這可能在某些國家不合法，如果是的話： Tomruen授予任何人有權利使用此作品於任何用途，除受法律約束外，不受任何限制。

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，此作品的版權所有人，釋出此作品至公共領域。此授權條款在全世界均適用。 這可能在某些國家不合法，如果是的話： 我授予任何人有權利使用此作品於任何用途，除受法律約束外，不受任何限制。