The object located at 5 hours 55 minutes right ascension and 7 degrees declination is the star Alnitak, which is part of the Orion constellation. Alnitak is the easternmost star in the three-star belt of Orion and is classified as a hot, massive blue supergiant. It is also known as Zeta Orionis and is approximately 800 light-years from Earth.
The hour angle system is a method used to measure the position of a celestial object in the sky. It measures the angular distance of an object from the observer's meridian, usually in hours (equivalent to 15 degrees per hour). By knowing the hour angle, one can determine the right ascension and declination of the object.
By tradition the direction of an object in the sky needs two coordinates to describe it because the normal description does not include the distance. The position (or direction) can be expressed as azimuth (angle round the horizon) and altitude (angle above the horizon). These depend on time an the position of the observer. Only positive altitude angles are seen in the sky. Astronomers prefer to use right ascension and declination. Declination is the latitude where the star passes overhead, and right ascension expresses how many hours the object crosses the meridian after a standard position called the First Point of Aries. The right ascension and declination are preferred because they don't depend on time or the observer's position on the Earth's surface.
"Right Ascension" is a coordinate in one of the main celestial coordinate systems. It is measured eastward along the "celestial equator". The units of measurement are hours, minutes and seconds. Those units are used because the "celestial sphere" appears to rotate once each day. Each hour is the equivalent of 15 degrees. The zero or starting point for right ascension is the "Vernal Equinox". It may seem odd to refer to the Vernal Equinox as the starting point of a coordinate system. The Vernal Equinox is actually a point in space. This point in space is occupied by the Sun at the time we call the Vernal Equinox. You can think of Right Ascension as being the equivalent of the Earth's meridians projected out into space.
That will apply to any object that has a declination of 0 degrees - such as the Sun at certain times of the year (the equinoxes), the Moon at certain times, or stars that have a declination close to zero degrees.
Declination is an astronomical term that refers to the angle between an object in the sky and the celestial equator, measured in degrees north or south. Latitude, on the other hand, is a geographic coordinate that specifies a position on Earth's surface relative to the equator, also measured in degrees north or south. While both are expressed in degrees and relate to the equator, declination pertains to celestial objects, whereas latitude pertains to locations on Earth.
The celestial coordinates you provided indicate an object located in the sky with a right ascension of 17 hours and a declination of -26.8 degrees. From a location at 32 degrees north latitude, this object would be positioned in the southern sky. Depending on the time of year, it may be visible during the evening or early morning hours when it is above the horizon. Observers should check local astronomical charts or software to determine the exact timing of visibility.
The coordinate equivalents on the celestial sphere are right ascension (RA) and declination (Dec). Right ascension is analogous to longitude, measured in hours, minutes, and seconds, indicating an object's position east or west of the vernal equinox. Declination is similar to latitude, measured in degrees north or south of the celestial equator, determining an object's angular distance from it. Together, these coordinates allow precise locating of celestial objects in the sky.
The largest -- about 18 billion solar masses -- is about 3.5 billion years away and is identical to the quasar OJ287. That object is in the constellation of Cancer, approximately at ascension 9 hours and declination 20 degrees.
Indicating the position of a celestial object is similar to latitude latitude and longitude. But it is called right ascension and declination.
The three celestial coordinates are right ascension, declination, and distance. Right ascension is analogous to longitude and measures the angle of a celestial object eastward along the celestial equator. Declination is similar to latitude and indicates how far north or south an object is from the celestial equator. Distance refers to the space between the observer and the celestial object, often measured in light-years or parsecs.
The constellation Perseus does not have a fixed latitude and longitude as it is a celestial object located in space. Its position is measured in right ascension and declination coordinates. Perseus is located in the northern celestial hemisphere and can be seen from latitudes between +90° and -35°.
Declination, which measures the angle between the direction of a celestial object and the celestial equator, ranges from +90 degrees to -90 degrees. A declination of +90 degrees indicates the North Celestial Pole, while -90 degrees indicates the South Celestial Pole. Values between these extremes represent the position of celestial objects in the sky relative to the celestial equator.
These are coordinates that define the position of an object in the sky (on the "celestial sphere"). They are used in a similar way to how latitude and longitude are used, on the Earth's surface.
The hour angle system is a method used to measure the position of a celestial object in the sky. It measures the angular distance of an object from the observer's meridian, usually in hours (equivalent to 15 degrees per hour). By knowing the hour angle, one can determine the right ascension and declination of the object.
By tradition the direction of an object in the sky needs two coordinates to describe it because the normal description does not include the distance. The position (or direction) can be expressed as azimuth (angle round the horizon) and altitude (angle above the horizon). These depend on time an the position of the observer. Only positive altitude angles are seen in the sky. Astronomers prefer to use right ascension and declination. Declination is the latitude where the star passes overhead, and right ascension expresses how many hours the object crosses the meridian after a standard position called the First Point of Aries. The right ascension and declination are preferred because they don't depend on time or the observer's position on the Earth's surface.
A declination is a term used in astronomy to describe the angular distance of a celestial object from the celestial equator. For example, the declination of the star Sirius is approximately -16.7 degrees, indicating its position relative to the celestial equator.
"Right Ascension" is a coordinate in one of the main celestial coordinate systems. It is measured eastward along the "celestial equator". The units of measurement are hours, minutes and seconds. Those units are used because the "celestial sphere" appears to rotate once each day. Each hour is the equivalent of 15 degrees. The zero or starting point for right ascension is the "Vernal Equinox". It may seem odd to refer to the Vernal Equinox as the starting point of a coordinate system. The Vernal Equinox is actually a point in space. This point in space is occupied by the Sun at the time we call the Vernal Equinox. You can think of Right Ascension as being the equivalent of the Earth's meridians projected out into space.