Whale Galaxy
Polish version is here |
NGC 4631, known as the Whale Galaxy, is an impressive barred spiral galaxy located in the constellation Canes Venatici. Its shape, resembling a whale swimming in the cosmic ocean, has earned it its name. Discovered on March 20, 1787, by William Herschel, it lies approximately 25–30 million light-years from Earth and spans about 140,000 light-years, making it slightly larger than the Milky Way. The galaxy is viewed almost exactly edge-on from Earth, which allows for detailed studies of its structure and properties.
At the core of NGC 4631 lies a prominent starburst region, an area of intense star formation. This vigorous stellar activity is evident in the emission of ionized hydrogen and interstellar dust heated by the newly formed stars. The most massive stars in these regions undergo rapid hydrogen fusion, quickly exhausting their fuel before ultimately exploding as supernovae.
Although no supernovae have been directly observed in NGC 4631, on January 29, 2021, a luminous red nova (LRN) designated AT 2021biy was discovered, with an apparent magnitude of 18.1m. LRNe are rare astronomical events thought to result from a stellar merger in a binary system. AT 2021biy was monitored photometrically and spectroscopically, revealing spectral evolution characteristic of this class of objects.
Observations
March 6, 2025, around 9:00 PM - Katowice (Poland)
urban environment, extremely high level of light pollution
That night, the sky was exceptionally clear, providing excellent conditions for astronomical observations. Despite the high level of light pollution, good atmospheric transparency allowed for deep-sky observations, and proper imaging techniques facilitated successful astrophotography.
During the observation, the elongated shape of the Whale Galaxy was clearly visible. The galaxy’s structure, including its dust lanes and active star-forming regions, was discernible as subtle variations in brightness along the edge of the disk. Nearby, the satellite galaxy NGC 4627 was also detected, although its smaller size and lower luminosity required greater observational effort.
NGC 4627 is a small elliptical galaxy gravitationally bound to its larger companion. Together, the Whale Galaxy and its satellite are cataloged as Arp 281 in Halton Arp’s Atlas of Peculiar Galaxies. Nearby, the distorted galaxy NGC 4656 suggests past gravitational interactions among all three, leading to structural deformations, the formation of tidal bridges, and enhanced star formation activity.
2MASX J12420645+3245390 is a small galaxy that has not yet been included in any widely known catalogs.
Photo 2 Parameters:
- Total exposure time: 25 minutes (stack of 50 RAW frames at 30s each, using an appropriate number of dark, bias, and flat frames)
- Canon EOS 60D
- ISO: 1500
- Maksutov-Cassegrain telescope (100/1400), prime focus exposure
- A filter was used to reduce the effects of artificial light pollution and atmospheric glow
- Mount: equatorial mount with tracking, aligned using the drift method and controlled by a custom-built system.
Further readings:
- Binney J., Merrifield M., Galactic Astronomy, Princeton University Press, 1998
- Freeman K., Bland-Hawthorn J., Galaxies and their Masks, Springer, 2011
- Sparke L.S., Gallagher J.S., Galaxies in the Universe: An Introduction, Cambridge University Press, 2007
Marek Ples