Suppose you want to photograph the Moon, and you want to know what it will look like in the photo. Given a location on the Earth, and a date/time, this program calculates the orientation of the sunlit side of the Moon with respect to the top of your photo image. It assumes the camera faces directly toward the Moon's azimuth and tilts upward to its altitude angle above the horizon. The angles are defined counterclockwise from the zenith, as shown here:
Finds when the Sun, Moon, and planets reach their highest position in the sky on a given date, as seen by an observer at a specified location on the Earth. Culmination is also the moment a body crosses the meridian, the imaginary semicircle in the sky that passes from due north on the horizon, through the zenith (straight up), and then toward due south on the horizon.
This is a more advanced example. It shows how to use coordinate transforms to find where the ecliptic intersects with an observer's horizon at a given date and time.
Calculates details about the first 10 partial/total lunar eclipses after the given date and time.
This example shows how to determine the Moon's current phase, and how to predict when the next few quarter phases will occur.
Calculates equatorial and horizontal coordinates of the Sun, Moon, and planets.
Shows how to calculate sunrise, sunset, moonrise, and moonset times.
Calculates the equinoxes and solstices for a given calendar year.
An example of how to use the Sun's hour angle to calculate true solar time.
Given the geographic coordinates of two observers, and angular
directions they are looking in, determines geographic coordinates
of the point they are both looking at. This example demonstrates
use of the geoid functions VectorObserver and ObserverVector
that convert between geographic coordinates and vectors.
Complete documentation for all the functions and types available in the C# version of Astronomy Engine.