Axial tilt.
spherical shape
The altitude of Polaris and the latitude of an observer are directly related. The altitude of Polaris in the sky is approximately equal to the observer's latitude in the Northern Hemisphere. The higher the latitude, the higher Polaris will appear in the sky.
Longitude was historically more difficult to determine than latitude because longitude is determined by measuring time differences between a reference point (such as Greenwich, England) and the observer's location, which required accurate timekeeping devices. Latitude, on the other hand, can be determined by measuring the angle of the North Star or the sun relative to the horizon.
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.
If an observer in Pennsylvania measures the altitude of Polaris to be 40 degrees, they could be approximately 40 degrees north of the equator, which would imply a latitude close to 40 degrees north. This is because the altitude of Polaris above the horizon is equal to the observer's latitude in the Northern Hemisphere.
The observer must be 15.5 degrees south of the Arctic circle, so 51.1 degrees north approximately.
If the altitude of Polaris is 43 degrees above the northern horizon, then the observer is located somewhere within roughly 1/2 degree of 43 degrees north latitude.
The altitude of polaris for an observer is always the same as your latitude so it would be 64oN
The altitude of Polaris and the latitude of an observer are directly related. The altitude of Polaris in the sky is approximately equal to the observer's latitude in the Northern Hemisphere. The higher the latitude, the higher Polaris will appear in the sky.
latitude of the observer.
Longitude was historically more difficult to determine than latitude because longitude is determined by measuring time differences between a reference point (such as Greenwich, England) and the observer's location, which required accurate timekeeping devices. Latitude, on the other hand, can be determined by measuring the angle of the North Star or the sun relative to the horizon.
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.
If an observer in Pennsylvania measures the altitude of Polaris to be 40 degrees, they could be approximately 40 degrees north of the equator, which would imply a latitude close to 40 degrees north. This is because the altitude of Polaris above the horizon is equal to the observer's latitude in the Northern Hemisphere.
The angle between the Pole Star and the horizon is equal to your latitude.
For an observer at latitude 35 degrees, the highest the sun can ever be in his sky is roughly 31.5 degrees above the horizon.
The altitude of Polaris, or the North Star, can be roughly estimated as equal to the latitude of the observer. Mamaroneck, New York, is situated at approximately 40.95° N latitude. Therefore, the altitude of Polaris from Mamaroneck would be about 40.95 degrees above the northern horizon.
The observer must be 15.5 degrees south of the Arctic circle, so 51.1 degrees north approximately.
The idea is there, but a couple of important terms are swapped.The altitude of the North Star above the northern horizon is approximately equal tothe observer's north latitude.