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NGC 2041 is a Globular Cluster in the Dorado constellation. NGC 2041 is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere. Given its visual magnitude of 10.36, NGC 2041 is visible with the help of a binocular with a 80mm aperture or a small telescope.

NGC 2041 是 劍魚座 的一個 星系。

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2020年3月13日 · Historical Identification: Per Dreyer, NGC 2041 (= GC 1244 = JH 2919, (Dunlop 241), 1860 RA 05 36 36, NPD 157 04.4) is "bright, small, round, very gradually a little brighter middle". Discovery Note: Apparently now thought to be Dunlop 196 and 241, hence its being added to Dreyer's entry in parentheses. (sources?)

2024年5月30日 · The area shown in this image is a part of LMC 4 supergiant shell is located North-East of the Large Magellanic Cloud (LMC) and contains a rich collection of HII regions and supernova remnants (SNR) fitting in between the NGC 2041 globular cluster [1] and the NGC 2030 (also known as LMC N63 or LHA 120-N63) HII region [2].

R/B-band color composite image from the Second Digitized Sky Survey (DSS2), measuring 10 arcminutes across. Click and drag the chart above to pan around the sky, or use the mouse …

NGC2041是一个星系，发现者是詹姆士·丹露帕，发现日期为1826年11月6日。

Van den Bergh and Hagen ("UBV photometry of star clusters in the Magellanic Clouds", Astronomical Journal, Vol. 73, 1968) find that the integrated V magnitude through a 60'' diaphragm is 10.36. They classify it as an open cluster. The RNGC (Sulentic and Tifft 1973) notes that this is a 10.5 mag open cluster in the LMC.

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