![]() ![]() ![]() Where /r is /L for leading, subtract S-O-T from 360°.Ī single cycle of Moon images cannot capture libration effects as the NASA SVS images do (see SpaceBread's answer), so Tanner's images look a little different from the actual Moon. Section 1: To simulate the night sky, we will be using the software Stellarium, which is free and easy to download/install. ![]() Where the /r column is /T for trailing, use that value directly. Objective: To become familiar with the phases of the moon and their connection to the orbital positions of the Moon relative to the Earth and Sun. The sun-observer-target elongation angle S-O-T is a close approximation in most cases. Tanner's rendered images appear to be indexed by the difference between lunar and solar ecliptic longitude. Name: Genesis Schat Due Date: Monday, June 8 by 11:50pm Objectives: Determine the Moon’s Rise and Set Times Observe Moon Phases Determine when various Moon Phases are Observable Observe Lunar Eclipses Observe Earth from the Moon Observe the Sun from the Moon Observe the Moon’s Synchronous Rotation Section 1. Where Illu% is the illuminated fraction $k$, and S-T-O is the sun-target-observer phase angle $i$.Īn observer location on the surface of the Earth instead of the geocenter gives slightly different results due to parallax. With a catalog of over 600,000 stars, planets, galaxies and other deep space. aiming your phone in the direction of the sky that you are viewing, you can quickly use Stellarium to help you identify or locate objects in the night sky with ease. It returns results like these: Date_(UT)_HR:MN Illu% S-O-T /r S-T-O ![]()
0 Comments
Leave a Reply. |
Details
AuthorWrite something about yourself. No need to be fancy, just an overview. ArchivesCategories |