NGC 4565 the Needle Galaxy
NGC 4565 the Needle Galaxy
NGC 4565 (also known as the Needle Galaxy or Caldwell 38) is an edge-on spiral galaxy about 30 to 50 million light-years away in the constellation Coma Berenices. It lies close to the North Galactic Pole and has a visual magnitude of approximately 10. It is known as the Needle Galaxy for its narrow profile. First recorded in 1785 by William Herschel, it is a prominent example of an edge-on spiral galaxy.
NGC 4565 is a giant spiral galaxy more luminous than the Andromeda Galaxy. Much speculation exists in literature as to the nature of the central bulge. In the absence of clear-cut dynamical data on the motions of stars in the bulge, the photometric data alone cannot adjudge among various options put forth. However, its exponential shape suggested that it is a barred spiral galaxy. Studies with the help of the Spitzer Space Telescope not only confirmed the presence of a central bar but also showed a pseudobulge within it as well as an inner ring.
NGC 4565 has at least two satellite galaxies, one of which is interacting with it. It has a population of roughly 240 globular clusters, more than the Milky Way.
This edge-on galaxy exhibits a slightly warped and extended disk under deep optical surveys- likely due to ongoing interactions with neighboring satellite galaxies or other galaxies in the Coma I group. (Wikipedia.org)
Technical Information for Image
Telescope: William Optics Zenithstar 81 Refractor
Mount: iOptron CEM25P
Imaging Camera: ZWO ASI294MC Pro Gain 120 -5C
Filter: Optolong L-Pro
Guiding: William Optics 50mm, 200mm FL, ASI290MC camera
Exposures: 42 x 180s each Bin 1x1
Capture: ASIAIR Pro
Guiding: ASIAIR Pro through ASI290MC camera
Polar Alignment: ASIAIR Pro
Site: Pinyon Pines, CA USA, Bortle 4
Processing: Pixinsight with Touch up in Corel PaintShop Pro.
NGC 4565 the Needle Galaxy
NGC 4565 the Needle Galaxy
NGC 4565 (also known as the Needle Galaxy or Caldwell 38) is an edge-on spiral galaxy about 30 to 50 million light-years away in the constellation Coma Berenices. It lies close to the North Galactic Pole and has a visual magnitude of approximately 10. It is known as the Needle Galaxy for its narrow profile. First recorded in 1785 by William Herschel, it is a prominent example of an edge-on spiral galaxy.
NGC 4565 is a giant spiral galaxy more luminous than the Andromeda Galaxy. Much speculation exists in literature as to the nature of the central bulge. In the absence of clear-cut dynamical data on the motions of stars in the bulge, the photometric data alone cannot adjudge among various options put forth. However, its exponential shape suggested that it is a barred spiral galaxy. Studies with the help of the Spitzer Space Telescope not only confirmed the presence of a central bar but also showed a pseudobulge within it as well as an inner ring.
NGC 4565 has at least two satellite galaxies, one of which is interacting with it. It has a population of roughly 240 globular clusters, more than the Milky Way.
This edge-on galaxy exhibits a slightly warped and extended disk under deep optical surveys- likely due to ongoing interactions with neighboring satellite galaxies or other galaxies in the Coma I group. (Wikipedia.org)
Technical Information for Image
Telescope: William Optics Zenithstar 81 Refractor
Mount: iOptron CEM25P
Imaging Camera: ZWO ASI294MC Pro Gain 120 -5C
Filter: Optolong L-Pro
Guiding: William Optics 50mm, 200mm FL, ASI290MC camera
Exposures: 42 x 180s each Bin 1x1
Capture: ASIAIR Pro
Guiding: ASIAIR Pro through ASI290MC camera
Polar Alignment: ASIAIR Pro
Site: Pinyon Pines, CA USA, Bortle 4
Processing: Pixinsight with Touch up in Corel PaintShop Pro.