Deep Sky Object in Spring
M101 (Pinwheel Galaxy in Ursa Major)


Click on image to enlarge

Date & Time: Feb 10 2024, from 23:58 to 24:53 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



M101 (NGC5457) / Galaxy, type SAB(rs)cd I
R.A.14h 03m 12.7s (2000.0)
Dec.+54° 21' 03" (2000.0)
Apparent Size28.8×26.9'
Radial Velocity+360km/s
Magnitude8.3
Distance22.5 million light yrs.
Group of GalaxiesM101 Group
Other IDsUGC8981, MCG9-23-28,
PGC50063, Arp 26
M101 (NGC5457) is a vast galaxy with open spirals, equivalent size to about two-third of the Moon and about 22 million light years away. Although seen face on, it's dim and it takes a large scope and a good sky to see this nebula at its best.
The galaxy is located 4 degrees east of zeta UMa (Mizar), the second star from the tip of the Big Dipper's handle, and the usual method given to find M101 is to the hop of several stars with fifth or sixth magnitude from Mizar.
In addition to being located at a close distance, M101 is a nearly face-on galaxy, allowing us to observe numerous Hα nebulae scattered along its arms. Some of these have catalog numbers assigned to them. You can refer their NGC numbers by clicking on a button at the upper right-hand side of the page.

Topics: Supernova 2023ixf in M101
Finding chart of M101 From Mizar to M101

  The star-hop route from Mizar to M101. You can find out M101 easily by tracing 81, 83, 84 and 86 UMa eastward.
(Taken with f=200mm telephoto lens)




Wide-field image around M101

Date & Time: May 3 2019, from 23:43 to 24:50 JST(+0900)
Composed 12 shots with 6 minutes exposed
Optical: TAKAHASHI 16cm(6.3") epsilon (f=530mm, F3.3)
with IDAS LPS-V1 Light-pollution suppression filter
Auto-guided with TAKAHASHI JP Equatorial & SBIG STV
Digital Camera: Nikon D810A
Location: Ooizumi, Hokuto city, Yamanashi pref.

Camera Settings: Recording Format...14bit CCD-RAW, converted to 16bit TIFF(7360×4912)
Device Size...FX format (36×24mm)
Sensitivity...ISO2500, White Balance...Daylight



This picture covers about 2.5 degrees in span around M101. There are several dimmed galaxies distributed around M101, and forming a small-scaled galactic group of "The M101 group". An irregular galaxy in lower of this image has a number of NGC5474.
Numbers with 4 digits represent NGC #



M94

NGC5866(M102)


Copyright(c) 2019, 2024 by Naoyuki Kurita, All rights reserved.
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