Grus (Pronounciation:Grus, Abbrev:Gru, Latin:Gruis) is a constellation, one of 88 constellations that the night sky is divided into. The sky is not divided up equally between the constellations. Grus takes up 365.513 sq. degrees of the night sky which equates to 0.89% of the night sky. The constellation gets its name as it name means The Crane . It was not one of the original constellations that had been devised by Ptolemy, instead it was created by Pieter Dirkszoon Keyser and Frederick de Houtman years later.
Grus is not a member of the Zodiac group of twelve constellations that appear when the Sun sets. Grus is a southern hemispheric constellation which means it can't be seen easily or at all from the northern hemisphere.
The number of stars that have been catalogued as part of the Hipparcos Star Catalogue from Grus is 1195. The number of stars that are of magnitude 6.0 or lower in the constellation is 39. The number of stars in the constellation that make up the outline is 9.
There are no deep space objects that were identified by Charles Messier in this constellation. There are no non-Messier deep space objects in this constellation that are covered at present on this site.
The nearest star to Earth is Gliese 832 which is roughly about 16.16 Light Years from the Earth. The nearest star to the Earth with an exoplanet is Gliese 832 which is about 16.16 Light Years. The furthest star that can be located in the constellation is HIP 111026 which is located about 163081.7 Light Years away from the Sun. The furthest figure is derived from either the 1997 or 2007 Hipparcos star catalogue parallax figure and it has been known to produce distances that are wrong.
The dimmest star that can be seen in Grus with the naked eye is HD 214953. The dim star has an apparent magnitude of 5.99. The dimmest star that a person is able to see with their naked eye is 6.0 magnitude based on the table in the reference. Ref: University of Michigan
The caveat of these stars are that they are catalogued on this site. If you know of a star that is nearer or further then do let me know in the comments and I'll add it to the site. The stars mentioned are from the Hipparcos catalogue or have been added because of their special status.
There is no Greek Legend behind this constellation. It was created by Pieter Dirkszoon Keyser and Frederick de Houtman to fill in the voids in the astronomical charts.There are no major meteor showers that radiate from within this constellation.
|Is a Zodiac Sign||No|
|Brightest Star||Al Nair|
|Area||365.513 sq. deg.|
|Percentage of Night Sky||0.89%|
|Site Exoplanet Count||6|
|Meteor Shower Count||1|
|Nearest Star||Gliese 832|
|Nearest Star with Exoplanet(s)||Gliese 832|
|Dimmest Star||HD 214953|
|Furthest Star||HIP 111026|
|Bright Star Count||39|
|Hipparcos Star Count||1195|
|Main Star Count||9|
|Messier Deep Space Object Count||0|
|*Non-Messier Deep Space Object Count||0|
|Bordering / Neighbouring / Surrounding Constellations||Piscis Austrinus|
*Note: The number of Non-Messier Deep Space Object Count relates to how many are covered on this site not how many there are.
The map was generated using Night Vision, an awesome free application by Brian Simpson.
|Star||Distance (Lt. Yrs.)||Exoplanet Count||Declination||Right Ascension|
|HD 208487||149.55||1||-37d 45` 48.0||21h 57m 19.77|
|HD 213240||132.53||1||-49d 25` 58.1||22h 31m 00.49|
|HD 215456||124.02||2||-48d 58` 43.3||22h 46m 07.85|
|PSR J2241-5236||1||-52d 36` 36.00||22h 41m 42.00|
|WASP-95||1||-48d 00` 11.16||22h 29m 49.99|
As there's so many stars in the cosmos, not all the stars are listed here. The site has lots of stars not listed so if your star isn't listed and you know the Henry Draper or Hipparcos ID, type https://www.universeguide.com/star/ then followed by the HIPNNNNNN or HDNNNN where NNNNN is the number part of the name. The stars that I do list have either a traditional name, a bayer or other classification name.
|Star||Distance (Lt. Yrs.)||Declination||Right Ascension|
|Al Dhanab||211.11||-37d 21` 53.4||21h 53m 55.65|
|Al Nair||101.01||-46d 57` 38.2||22h 08m 13.88|
|BZ Gruis||468.63||-37d 44` 48.7||21h 57m 02.14|
|Delta1 Gruis||309.45||-43d 29` 44.0||22h 29m 16.15|
|Delta2 Gruis||330.12||-43d 44` 57.2||22h 29m 45.45|
|DL Gruis||918.77||-40d 35` 29.2||23h 10m 09.72|
|Epsilon Gruis||128.92||-51d 19` 00.1||22h 48m 33.20|
|Eta Gruis||414.97||-53d 30` 00.6||22h 45m 37.85|
|Gliese 832||16.16||-49d 00` 25.3||21h 33m 34.02|
|Iota Gruis||183.24||-45d 14` 47.9||23h 10m 21.43|
|Kappa Gruis||364.02||-53d 57` 52.7||23h 04m 39.57|
|Lambda Gruis||242.14||-39d 32` 35.0||22h 06m 06.90|
|Mu1 Gruis||274.78||-41d 20` 48.3||22h 15m 36.88|
|Mu2 Gruis||265.39||-41d 37` 37.9||22h 16m 26.57|
|Nu Gruis||285.11||-39d 07` 53.0||22h 28m 39.18|
|Omicron Gruis||100.36||-52d 43` 18.9||23h 26m 36.54|
|Phi Gruis||115.50||-40d 49` 26.6||23h 18m 09.79|
|Pi1 Gruis||532.08||-45d 56` 52.5||22h 22m 44.18|
|Pi2 Gruis||130.47||-45d 55` 42.0||22h 23m 07.79|
|Rho Gruis||230.34||-41d 24` 50.8||22h 43m 29.97|
|RS Gruis||776.58||-48d 11` 22.0||21h 43m 04.28|
|S Gruis||1456.09||-48d 26` 18.7||22h 26m 05.45|
|Sigma1 Gruis||222.79||-40d 34` 57.0||22h 36m 29.27|
|Sigma2 Gruis||214.72||-40d 35` 27.1||22h 36m 58.82|
|Tau1 Gruis||106.38||-48d 35` 53.1||22h 53m 37.74|
|Tau2 Gruis||155.54||-48d 27` 57.4||22h 55m 16.35|
|Tau2 Gruis B||145.28||-48d 29` 30.8||22h 55m 16.19|
|Tau3 Gruis||243.41||-47d 58` 09.2||22h 56m 47.82|
|Theta Gruis||131.89||-43d 31` 13.2||23h 06m 52.77|
|Tiaki||176.97||-46d 53` 04.4||22h 42m 39.93|
|Upsilon Gruis||284.86||-38d 53` 32.3||23h 06m 53.60|
|W Gruis||1136.46||-43d 50` 28.3||22h 41m 18.67|
|Xi Gruis||465.95||-41d 10` 45.6||21h 32m 05.86|
|Zeta Gruis||108.87||-52d 45` 14.8||23h 00m 52.87|
|F||Yellow-White 6,000 - 7,500k||396|
|K||Light Orange Star 3,700 - 5,200k||355|
|G||Yellow 5,200 - 6,000k||284|
|A||White 7,500 - 10,000k||65|
|M||Red Dwarf Star <3,700k||61|
|B||Blue-White 10,500 - 30,000k||8|
|Ib||Less Luminous Supergiant||1|
|sd||sd Type SubDwarf Star||2|
|S||S-Type Carbon Star||3|
|bill nye the science guy||Tuesday, 3rd October 2017 12:48:04 PM|
|fuck this shit|
|kjn||Wednesday, 24th May 2017 3:13:05 PM|