Telescope: Sky-Watcher Evostar 72ed
Mount: Sky-Watcher HEQ-5 Pro
Camera: ZWO ASI 533MC-Pro
Gain: 100
Filter: Optolong L’Pro 1.25 Inch
Totale exposure: 72 x 300 sec / 6 hours
Guide Scope: ZWO Mini Guide Scope
Guide Camera: ZWO ASI 120MM
Explore the wonders of the universe with M51, also known as the Whirlpool Galaxy. Located in the constellation Canes Venatici, M51 is a prime example of a spiral galaxy, enchanting astronomers with its majestic spiral arms and interactive companion galaxy. Join us as we delve into the fascinating features and significance of the Whirlpool Galaxy.
M51, the Whirlpool Galaxy, is a classic spiral galaxy situated about 23 million light-years from Earth. Renowned for its grand-design spiral structure, M51 serves as an archetype for spiral galaxies. The galaxy’s distinctive appearance is enhanced by its interaction with a smaller companion galaxy, NGC 5195.
Positioned in the constellation Canes Venatici near the Big Dipper’s handle, the Whirlpool Galaxy is a favorite among amateur astronomers due to its brightness and clear structure. With an apparent magnitude of 8.4, M51 is visible through binoculars in dark skies and offers a spectacular view through moderate to large telescopes.
Spiral Arms
The striking spiral arms of M51 are regions of intense star formation, filled with young, hot stars that illuminate surrounding gas and dust. These well-defined arms, featuring bright star clusters and dark dust lanes, gracefully wind around the galaxy’s core.
Galactic Core
At the heart of M51 lies a bright core housing a supermassive black hole. This black hole exerts a strong gravitational influence, playing a crucial role in the galaxy’s dynamics. The core is home to older, redder stars, contrasting with the younger, bluer stars in the spiral arms.
Companion Galaxy NGC 5195
The elliptical galaxy NGC 5195 interacts gravitationally with M51, significantly influencing its structure and enhancing its spiral arms. This cosmic dance, as NGC 5195 currently passes behind M51 from Earth’s perspective, is a subject of intense study.
Observing the Whirlpool Galaxy can be incredibly rewarding. Here are some tips:
Galactic Interaction
The interaction between M51 and NGC 5195 offers insights into galaxy collisions and mergers, crucial for understanding galactic evolution. Studying M51 helps astronomers learn how these processes trigger star formation and influence galactic structure.
Star Formation
M51’s spiral arms are hotspots for star formation. By examining these regions, astronomers gain knowledge about the conditions that lead to star birth and the lifecycle of stars.
Supermassive Black Hole
Research on the supermassive black hole at M51’s center provides understanding of the relationship between black holes and their host galaxies, including their mutual influence on growth and development.
Discovery
Charles Messier discovered the Whirlpool Galaxy in 1773, and it was later cataloged as M51. Pierre Méchain discovered its companion galaxy, NGC 5195, in 1781. M51 has since been a favorite target for astronomers and extensively studied using both ground-based and space-based telescopes.
Hubble Space Telescope
The Hubble Space Telescope has captured detailed images of M51, revealing intricate galaxy structures and star-forming regions. These observations have significantly advanced our understanding of spiral galaxies.
Capturing M51’s beauty requires planning and proper equipment:
M51, the Whirlpool Galaxy, offers a magnificent view into the complexities of galaxy formation and interaction. Its stunning spiral arms, active star-forming regions, and dynamic relationship with NGC 5195 make it a fascinating subject for observation and study. Whether you’re an amateur astronomer or a seasoned astrophotographer, the Whirlpool Galaxy provides endless opportunities for exploration and discovery. Keep looking up and marvel at the wonders of the universe!
M51 – The Whirlpool Galaxy shot through a Celestron C14
Image taken by Maurik
In the same image of M51, many more galaxies can be seen. The two most distant galaxies in this image are IC4284 and IC4285. IC 4284 and IC 4285 are two intriguing celestial objects cataloged in the Index Catalogue (IC), which is a supplement to the New General Catalogue (NGC). Both objects are galaxies located in the constellation Virgo. Here’s a closer look at each:
IC 4284 is an elliptical galaxy situated in the constellation Virgo. This galaxy is relatively faint and not easily visible without the aid of a telescope. Elliptical galaxies like IC 4284 are characterized by their smooth, featureless light distribution and lack of significant structure such as spiral arms.
IC 4284 is best observed using large telescopes due to its faintness and small size. It appears as a small, featureless blob of light, typical of elliptical galaxies, which lack the detailed structure seen in spiral or irregular galaxies.
IC 4285 is a spiral galaxy, also located in the constellation Virgo. Spiral galaxies are notable for their well-defined structures, including spiral arms that wind out from a central bulge. IC 4285, like many galaxies in Virgo, is part of the Virgo Cluster, a massive cluster of galaxies that is a key area of study in extragalactic astronomy.
In this image, you can see that with only a 3 inch refractor with a focal length of 420mm, M51 is still very small. This image only has an auto stretch, but not any further processing was done. Still you can see the details already very clear. In total the final image had a total exposure time of 72 x 300 seconds, so 6 hours of integration time. Which is a good start to try this object with a small refractor! I stacked and calibrated all sub images in Siril. Further processing was on in Adobe Photoshop.
I hope you enjoyed this blog and images about M51 – The Whirlpool Galaxy
Happy stargazing! – Jimmy Keetman