English Deutsch Français Italiano Español Português 繁體中文 Bahasa Indonesia Tiếng Việt ภาษาไทย
All categories

2 answers

Since planets orbit the Sun, it is much simpler to specify their positions in solar (heliocentric) coordinates rather than Earth (geocentric) coordinates.

The heliocentric longitude is somewhat like right ascension. Heliocentric longitude is zero at the position of the Earth on the vernal equinox and the Earth's heliocentric longitude increases by about 1 degree per day (360 degrees per year).

Precision calculations for planetary positions are usually done in heliocentric longitude (L), elevation above or below the ecliptic (B) and distance from the Sun (R). To figure the place of a planet in the sky, the LBR coordinates of the planet and the Earth are both calculated and the difference is the vector from Earth to the planet.

2007-01-17 13:52:48 · answer #1 · answered by Pretzels 5 · 1 0

Heliocentric Longitude

2016-12-17 14:52:50 · answer #2 · answered by schecter 4 · 0 0

fedest.com, questions and answers