The zenith.
No, the celestial equator does not always pass directly overhead. The position of the celestial equator in the sky is determined by the observer's latitude on Earth. If the observer is located at the equator, the celestial equator will pass directly overhead. However, for observers at different latitudes, the celestial equator will appear at an angle to the horizon.
The local zenith is perpendicular to the rotation axis of the Earth at a specific location. It represents the point directly above an observer, pointing towards the celestial sphere. The rotation axis of the Earth is an imaginary line around which the Earth spins.
That's the observer's 'zenith'. Since it's referenced to the "observer's head", each observer has a different zenith.
The altitude of the North Celestial Pole above the northern horizon is equal to the observer's latitude. This means that the higher the observer's latitude, the higher the North Celestial Pole will appear in the sky. For example, an observer at a latitude of 45 degrees will see the North Celestial Pole 45 degrees above the northern horizon.
Greenwich Celestial refers to the Prime Meridian as it crosses the celestial sphere above Greenwich, UK. It serves as the global reference point to measure longitude and is used in celestial navigation and astronomy.
That's called the observer's "zenith".
The point just overhead is called the zenith. The objects visible at that point depend on the date, the time of day or night, and the observer's location.
The zenith.
west
No, the celestial equator does not always pass directly overhead. The position of the celestial equator in the sky is determined by the observer's latitude on Earth. If the observer is located at the equator, the celestial equator will pass directly overhead. However, for observers at different latitudes, the celestial equator will appear at an angle to the horizon.
The imaginary point located directly above an observer's head is called the "zenith." In celestial navigation and astronomy, the zenith is the point in the sky that is vertically aligned with the observer's position on the Earth's surface. It represents the highest point in the sky relative to the observer's location.
The local zenith is perpendicular to the rotation axis of the Earth at a specific location. It represents the point directly above an observer, pointing towards the celestial sphere. The rotation axis of the Earth is an imaginary line around which the Earth spins.
That's the observer's 'zenith'. Since it's referenced to the "observer's head", each observer has a different zenith.
The altitude of the North Celestial Pole above the northern horizon is equal to the observer's latitude. This means that the higher the observer's latitude, the higher the North Celestial Pole will appear in the sky. For example, an observer at a latitude of 45 degrees will see the North Celestial Pole 45 degrees above the northern horizon.
The astronomical triangle is a geometric representation used in celestial navigation and astronomy to solve problems related to the positions of celestial bodies. It is formed by three points: the observer's location on Earth, a celestial object (like a star or planet), and the zenith point directly above the observer. The sides of the triangle represent angles such as the altitude of the celestial object and the azimuth, allowing navigators to calculate positions and distances in the sky. This triangle is essential for determining the latitude and longitude of a location based on celestial observations.
Greenwich Celestial refers to the Prime Meridian as it crosses the celestial sphere above Greenwich, UK. It serves as the global reference point to measure longitude and is used in celestial navigation and astronomy.
Zenith