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NGC 2867 (also known as Caldwell 90) is an elliptical [5] Type II [7] planetary nebula in the southern constellation of Carina, just over a degree to the NNW of the star Iota Carinae. [8] It was discovered by John Herschel on April 1, 1834.
Roll-off container sizes are determined by the amount of debris they can hold, measured in cubic yards. [2] Container sizes commonly found in the United States include 10, 15, 20, 30, and 40 cubic yards, equivalent to approximately 7.65 m³, 11.47 m³, 15.29 m³, 22.94 m³, and 30.58 m³.
Caldwell advocates, however, see the catalog as a useful list of some of the brightest and best known non-Messier deep-sky objects. Thus, advocates dismiss any "controversy" as being fabricated by older amateurs simply not able or willing to memorize the new designations despite every telescope database using the Caldwell IDs as the primary ...
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NGC 3532; Observation data (J2000 epoch); Right ascension: 11 h 05 m 33 s [1]: Declination: −58° 43.8′ [1] Distance: 1,321 [2] ly (405 pc): Physical characteristics; Other designations: NGC 3532, [1] Caldwell 91, Cr 238, Mel 103, C 1104-584, Cl* 1104-584, CL 1104-584, Lacaille II.10, [3] Football Cluster, Wishing Well Cluster [4] [5] [6] [7]
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HR diagram showing the main sequence turnoff of NGC 188 and M 67, indicating their relatively high ages. NGC 188 (also known as Caldwell 1 or the Polarissima Cluster [5]) is an open cluster in the constellation Cepheus.
The Double Cluster in Perseus (lower left of center, wide angle view) Greek astronomer Hipparchus cataloged the object (a patch of light in Perseus) as early as 130 BCE. To Bedouin Arabs the cluster marked the tail of the smaller of two fish they visualized in this area, and it was shown on illustrations in Abd al-Rahman al-Sufi's Book of Fixed Stars. [4]
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