Editing Camelopardalis (section)

===Deep-sky objects===
Camelopardalis is in the part of the celestial sphere facing away from the [[galactic plane]]. Accordingly, many distant galaxies are visible within its borders. 
* [[NGC 2403]] is a galaxy in the [[M81 group]] of galaxies, located approximately 12 million light-years from Earth{{sfn|Wilkins|Dunn|2006}}{{sfn|Ridpath|2001|pp=92–93}} with a redshift of 0.00043. It is classified as being between an [[elliptical galaxy|elliptical]] and a [[spiral galaxy]] because it has faint arms and a large central bulge. NGC 2403 was first discovered by the 18th century astronomer [[William Herschel]], who was working in England at the time.{{sfn|Wilkins|Dunn|2006}} It has an [[integrated magnitude]] of 8.0 and is approximately 0.25° long.{{sfn|Ridpath|2001|pp=92–93}}
* [[NGC 1502]] is a magnitude 6.9 [[open cluster]] about 3,000 [[light year]]s from Earth. It has about 45 bright members, and features also a double star of magnitude 7.0 at its center.<ref>Revised NGC/IC Data 2013. Dr. Wolfgang Steinicke.</ref> NGC 1502 is also associated with [[Kemble's Cascade]], a simple but beautiful asterism appearing in the sky as a chain of stars 2.5° long that is parallel to the Milky Way and is pointed towards [[Cassiopeia (constellation)|Cassiopeia]].{{sfn|Ridpath|2001|pp=92–93}} * [[NGC 1501]] is a planetary nebula located roughly 1.4° south of NGC 1502.
* Stock 23 is an open star cluster at the southern part of the border between Camelopardalis and Cassiopeia. It is also known as ''Pazmino's Cluster''. It could be categorized as an ''asterism'' because of the small number of stars in it (a small telescopic ''constellation'').
* [[IC 342]] is one of the brightest two galaxies in the [[IC 342/Maffei Group]] of galaxies.
* The dwarf irregular galaxy [[NGC 1569]] is a magnitude 11.9 [[starburst galaxy]], about 11 million light years away.
* [[NGC 2655]] is a large [[lenticular galaxy]] with visual magnitude 10.1.
* UGC 3697 is known as the ''Integral Sign Galaxy'' (its location is 7:11:4 / +71°50').
* [[MS0735.6+7421]] is a galaxy cluster with a [[redshift]] of 0.216, located 2.6&nbsp;billion light-years from Earth. It is unique for its [[intracluster medium]], which emits [[X-ray]]s at a very high rate. This galaxy cluster features two cavities 600,000 light-years in diameter, caused by its central [[supermassive black hole]], which emits jets of matter. MS0735.6+7421 is one of the largest and most distant examples of this phenomenon.{{sfn|Wilkins|Dunn|2006}}
* Tombaugh 5 is a fairly dim open cluster in Camelopardalis. It has an overall magnitude of 8.4 and is located 5,800 light-years from Earth. It is a Shapley class c and Trumpler class III 1 r cluster, meaning that it is irregularly shaped and appears loose. Though it is detached from the star field, it is not concentrated at its center at all. It has more than 100 stars which do not vary widely in brightness,{{sfn|Levy|2005|p=89}} mostly being of the 15th and 16th magnitude.{{sfn|Levy|2005|p=91}}
* [[NGC 2146]] is an 11th magnitude barred spiral starburst galaxy conspicuously warped by interaction with a neighbour.
* [[MACS0647-JD]], one of the possible candidates for the farthest known galaxies in the universe ([[Redshift|z]]= 10.7), is also in Camelopardalis.