Deep Sky Object in Spring
NGC4605(Galaxy in Ursa Major)



Date & Time: Jan 16 2026, from 26:44 to 27:39 JST(+0900)
Composed 10 shots with 6 minutes exposed
Optical: Meade 25cm(10") Schmidt-Cassegrain with conversion lens (f=1600mm, F6.3)
with IDAS LPS-P1 Light-pollution suppression filter
Auto-guided with Meade LX200 Equatorial & Lacerta M-GEN
Digital Camera: Nikon D810A
Location: Ooizumi, Hokuto city, Yamanashi pref.

Camera Settings: Recording Format...14bit CCD-RAW, converted to 16bit TIFF(4080×4080)
Device Size...20×20mm
Sensitivity...ISO4000, White Balance...Daylight



NGC3917 / Galaxy, type SB(s)c pec III-IV
R.A.12h 40m 00.3s (2000.0)
Dec.+61°36' 39" (2000.0)
Apparent Size5.7×2.1'
Radial Velocity+149km/s
Magnitude10.9
Distance18 million light yrs.
Group of GalaxiesM81 Group
Other IDsUGC 7831, CGCG 293-31
MCG +10-18-74, PGC 42408
IRAS 12378+6152
NGC4605 is a peculiarly shaped barred spiral galaxy seen in the northern part of Ursa Major, located 5.6 degrees northeast of δ Ursae Majoris, one of the stars forming the Big Dipper. It has a cigar-like appearance with a major-axis length of 5.7 arcminutes, and no well-defined spiral structure is visible. Although faint, asymmetric dust lanes can be seen distributed within the galaxy. It lies at a distance of about 18 million light-years and, despite being separated by as much as 18 degrees on the sky, is thought to belong to the same galaxy group as M81 and M82 in Ursa Major.




NGC4565

NGC4631, NGC4656


Copyright(c) 2026 by Naoyuki Kurita, All rights reserved.
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