NGC 6015 is a Spiral Galaxy in the Draco constellation. NGC 6015 is situated close to the northern celestial pole and, as such, it is visible for most part of the year from the northern hemisphere. Given its visual magnitude of 11.14, NGC 6015 is visible with the help of a telescope having an aperture of 6 inches (150mm) or more.

2023年6月24日 · NGC 6015 at 40 million light years distance is an isolated and warped type Sc-r galaxy. Recent studies indicate a discontinuity in the formation of the spiral arms and different rotation rates between the inner and outer arms.

NGC 6015 is a Spiral Galaxy located in the constellation of Draco in the northern hemisphere. NGC 6015's distance from Earth is 48,147,204.48 light years. NGC 6015 is called NGC 6015 in the New General Catalogue (NGC). This catalogue is a list of deep space objects compiled by John Louis Emil Dreyer in 1888 to update John Herschel's earlier work.

Spiral Galaxy NGC 6015 This is a 10 minute exposure with an ST-6 CCD camera thru Kopernik's 20-inch Ritchey Chretien Cassegrain telescope, working at F/4.9. The field of view is about 9x12.5 arc minutes.

NGC 6015 at 40 million light years distance is an isolated and warped type Sc-r galaxy. Recent studies indicate a discontinuity in the formation of the spiral arms and different rotation rates between the inner and outer arms.

From Redmond , NGC6015 is visible all night because it is circumpolar. It will be highest in the sky shortly before dawn, when it will be lost to twilight at around 06:23, 71° above your north-eastern horizon. At dusk, it will become visible at around …

NGC 6015 is a spiral galaxy located in the constellation Draco, near the north pole. It is an area with many faint background galaxies.

2023年8月2日 · NGC 6015は、りゅう座にあり、およそ4千万光年の距離の棒構造を持たない渦状銀河です。今回の画像からはわかりにくいのですが、後期型の渦状銀河には珍しい、渦状腕と繫がる見かけの大きさ約5.2′ x 1.8′の淡い疑似リング構造が外周に見えています。

NGC 6015 in Draco. Higher resolved image / höher aufgelöstes Bild (2000 x 1534)

NGC 6015 is an isolated and warped type Sc-r galaxy. Recent studies indicate a discontinuity in the formation of the spiral arms and different rotation rates between the inner and outer arms. There is no indication of bar formation.