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LabelNameRA (J2000.0), Dec (J2000.0)LII, BII0FGL_name, 1FGL_name,2FGL_name, 3FGL_name,1FHL_name, 2FHL_camera_1FGL, Dec_1FGLRA_2FGL, Dec_2FGLRA_3FGL, Dec_3FGLRA_1FHL, Dec_1FGLRA_2FHL, Dec_2FHLClassUnitSED
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How to fill out right ascension ampamp declination

01
To fill out right ascension and declination, follow these steps:
02
Determine the exact location or celestial object you want to record the coordinates for.
03
Start with right ascension, which measures the east-west position of the object.
04
- Use a telescope or star chart to identify the object's position in hours, minutes, and seconds of time.
05
- Convert these time values to degrees by multiplying the hours by 15, the minutes by 0.25, and the seconds by 0.00417.
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- Add or subtract the converted values based on whether the object is east or west of the prime meridian.
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Move on to declination, which measures the north-south position of the object.
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- Determine the object's position in degrees and minutes of arc using the telescope or star chart.
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- Note that positive declination is for objects in the northern hemisphere, while negative declination is for objects in the southern hemisphere.
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- Record the degrees and minutes directly as they are already in the correct format.
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Combine the right ascension and declination values to form a single coordinate in the format 'right ascension, declination.'
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- The right ascension value should be written in hours, minutes, and seconds separated by colons.
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- The declination value should be written in degrees and minutes separated by colons as well.
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- For example, a completed coordinate could look like '12:34:56, +45:21'.

Who needs right ascension ampamp declination?

01
Right ascension and declination are important for various fields including astronomy, astrophysics, and celestial navigation.
02
Specifically, the following individuals or groups may require right ascension and declination:
03
- Astronomers and astrophysicists: They use these coordinates to accurately locate and study celestial objects in the sky.
04
- Amateur astronomers: They utilize right ascension and declination to find specific stars, planets, or galaxies for observation.
05
- Navigators: Right ascension and declination are used in celestial navigation to determine the exact position of a ship or aircraft.
06
- Telescope operators: They need these coordinates to accurately point telescopes at specific celestial objects of interest.
07
- Planetariums and observatories: These institutions use right ascension and declination to provide accurate celestial coordinates for public viewing and education.
08
- Astronomical software developers: Right ascension and declination are essential parameters in many astronomical software and databases used by professionals and enthusiasts.
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Overall, anyone interested in understanding and exploring the night sky can benefit from understanding and working with right ascension and declination.
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Right ascension and declination are coordinates used in astronomy to locate objects in the sky. Right ascension is similar to longitude on Earth, while declination is similar to latitude.
Astronomers, researchers, and anyone else involved in celestial observations may be required to report right ascension and declination.
Right ascension and declination can be filled out using astronomical tools and software that calculate these coordinates based on observations of celestial objects.
The purpose of right ascension and declination is to accurately record the positions of celestial objects in the sky to study their movements and locations.
The information reported on right ascension and declination includes the coordinates of celestial objects, the date and time of observation, and the location of the observer.
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