NGC 4565

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NGC 4565
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NGC 4565
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascensionTemplate:RA[1]
DeclinationTemplate:DEC[1]
Redshift0.004276[1]
Heliocentric radial velocity1282 ± 1 km/s[1]
Distance38.16 ± 2.27 Mly (11.700 ± 0.697 Mpc)[2]
53 ± 4 Mly (16.2 ± 1.3 Mpc)[3]
Apparent magnitude (V)10.42[1]
Characteristics
TypeSA(s)b?[1]
Size~176,000 ly (53.94 kpc) (diameter; D25 isophote)[1]
Apparent size (V)15.90′ × 1.85′[1]
Other designations
Template:Odlist[1]

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.[2] 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, and is a prominent example of an edge-on spiral galaxy.[4][5] It was discovered by German-British astronomer William Herschel on 6 April 1785.[6]

Characteristics

NGC 4565 is a giant spiral galaxy more luminous than the Andromeda Galaxy.[7] 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.[8] 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.[9]

File:Needle Wide.png
This is a wide field view of the Needle Galaxy captured in March 2025.

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. GALEX images show the slight warp at the edge of the disc more clearly than other surveys.

Using the LOw-Frequency ARray (LOFAR), astronomers of the University of Hamburg discovered a diffuse radio halo around NGC 4565. During the observations, a warp was detected in the radio continuum of NGC 4565 that is reminiscent of a neutral hydrogen line (HI) warp and identifying a slight flaring of the galaxy's radio halo. It is assumed that this flaring is caused by the warp as the vertical intensity profiles are asymmetric, which is in agreement with the warp. According to the study, a minimum age for the warp was estimated at approximately 130 million years. This is the spectral age of the galaxy's cosmic ray electrons, during which they are transported into the warp. This indicates that NGC 4565 may be in the aftermath of a period with more intense star formation.

Galaxy Groups

NGC 4565, along with NGC 4562, IC 3543, and IC 3546, are listed together as Holm 426 in Erik Holmberg's A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems, published in 1937.[10]

NGC 4565 has at least two satellite galaxies, one of which is interacting with it.[11] It has a population of roughly 240 globular clusters, more than the Milky Way.[7]

NGC 4565 is one of the brightest[12] member galaxies of the Coma I Group.[13][12]

References

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  1. ^ a b c d e f g h i Page Module:Citation/CS1/styles.css has no content."Results for NGC 4565". NASA/IPAC Extragalactic Database. Retrieved 2026-03-27.
  2. ^ a b Page Module:Citation/CS1/styles.css has no content."Distance Results for NGC 4565". NASA/IPAC Extragalactic Database. Retrieved 2026-03-27.
  3. ^ Page Module:Citation/CS1/styles.css has no content.Jensen, Joseph B.; Tonry, John L.; Barris, Brian J.; Thompson, Rodger I.; et al. (February 2003). "Measuring Distances and Probing the Unresolved Stellar Populations of Galaxies Using Infrared Surface Brightness Fluctuations". Astrophysical Journal. 583 (2): 712–726. arXiv:astro-ph/0210129. Bibcode:2003ApJ...583..712J. doi:10.1086/345430. S2CID 551714.
  4. ^ Page Module:Citation/CS1/styles.css has no content."NGC4565 at". apod.nasa.gov.
  5. ^ Spiral Galaxy NGC 4565 at http://www.eso.org/public/images/eso0525a/
  6. ^ Page Module:Citation/CS1/styles.css has no content.Seligman, Courtney. "New General Catalogue Objects: NGC 4565". Celestial Atlas. Retrieved 18 August 2025.
  7. ^ a b Page Module:Citation/CS1/styles.css has no content.Harris, William E. (1991). "Globular cluster systems in galaxies beyond the Local Group". Annual Review of Astronomy and Astrophysics. 29: 543. Bibcode:1991ARA&A..29..543H. doi:10.1146/annurev.aa.29.090191.002551.
  8. ^ Page Module:Citation/CS1/styles.css has no content.Wu, Hong; et al. (2002). "Intermediate-band surface photometry of the edge-on galaxy NGC 4565". The Astronomical Journal. 123 (3): 1364–1380. arXiv:astro-ph/0111433. Bibcode:2002AJ....123.1364W. doi:10.1086/338849.
  9. ^ Detection of a Distinct Pseudobulge Hidden Inside the Box-Shaped Bulge of NGC 4565
  10. ^ Page Module:Citation/CS1/styles.css has no content.Holmberg, Erik (1937). "A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems". Annals of the Observatory of Lund. 6: 1. Bibcode:1937AnLun...6....1H.
  11. ^ HALOGAS: H I Observations and Modeling of the Nearby Edge-on Spiral Galaxy NGC 4565
  12. ^ a b Page Module:Citation/CS1/styles.css has no content."Webb Deep-Sky Society: Galaxy of the Month: NGC4565". www.webbdeepsky.com. Retrieved 2018-05-20.
  13. ^ Page Module:Citation/CS1/styles.css has no content.Gregory, Stephen A.; Thompson, Laird A. (April 1977). "The Coma i Galaxy Cloud". The Astrophysical Journal. 213: 345–350. Bibcode:1977ApJ...213..345G. doi:10.1086/155160. ISSN 0004-637X.
  14. ^ Page Module:Citation/CS1/styles.css has no content."NGC 4565 - Needle Galaxy".


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