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 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.
it would be 30 degrees It is 15 degrees. (360 degrees/24 hours = 15).
Right angles have 90 degrees.
A right angle is 90 degrees
Right ascension: 21 h Declination: −20°
Right ascension is 21 h and declination is −36°.
The right ascension of Corona Borealis is approximately 16 hours, and the declination is around +30 degrees. These coordinates indicate the position of the constellation in the sky and are used by astronomers to locate it.
Right ascension: 8 h Declination: +5°
Right ascension: 11 h Declination: +15°
Depends on the declination in question. There are 24 hours of right ascension in 360 degrees, so at the celestial equator (declination = 0 degrees) 1 hour of right ascension is equal to 15 degrees. But as you increase or decrease declination the right ascension lines converge to the celestial pole (like longitude lines on a globe). The angle covered by 1 hour of right ascension is therefore equal to (15 degrees x cos(declination) ), so at the celestial poles (declination = +/- 90 degrees) 1 hour of RA is 0 degrees.
the right ascension is 19.11h and the declination is -25.8 degrees
The right ascension of the star Procyon is approximately 7 hours and 39 minutes, while its declination is approximately +5 degrees and 14 minutes. These coordinates are for the epoch J2000.
60o, or 62o I believe the Right Ascension is about 1h as well.
The Right ascension is 07h 55m 19.7973s-09h 22m 35.0364s and the Declination is 33.1415138°-6.4700689°.
On February 5th, Polaris has a declination of approximately +89 degrees 15 minutes and a right ascension of about 2 hours 31 minutes. These values may vary slightly depending on the year and time of observation.
Right Ascension in space is equivalent to Longitude on Earth but it is measured in hours minutes and seconds rather than degrees, minutes and seconds. 1 hour of RA is equivalent to 15° of longitude. Declination in Space is equivalent to Latitude on Earth. Both are measure in degrees, minutes and seconds. Declination is measured from the Celestial Equator, + being north and - being south, just like Latitude.