Featured Research

from universities, journals, and other organizations

New look into Whirlpool Galaxy

Date:
June 15, 2010
Source:
Calar Alto Observatory-CAHA
Summary:
The Whirlpool Galaxy (M51) is a classic, a real must that now gets into Calar Alto Documentary Photo Gallery with an impressive new photo obtained with the Zeiss 1.23 m reflector. The image displays all the features that make this galaxy an exceptional object to illustrate the nature of spiral galaxies, the processes of star formation and the dynamics of interacting stellar systems.

Left: M51 in true color. Right: M51 with H-alpha enhanced.
Credit: CAHA, Descubre, DSA, OAUV. Vicent Peris (OAUV/DSA/PixInsight), Jack Harvey (SSRO/DSA), Steven Mazlin (SSRO/DSA), Carlos Sonnenstein (Valkΰnik/DSA) and Juan Conejero (PixInsight/DSA)

The Whirlpool Galaxy (M51) is a classic, a real must that now gets into Calar Alto Documentary Photo Gallery with an impressive new photo obtained with the Zeiss 1.23 m reflector. The image displays all the features that make this galaxy an exceptional object to illustrate the nature of spiral galaxies, the processes of star formation and the dynamics of interacting stellar systems.

Related Articles


The Spanish poet Josι Hierro, when presenting his book Cuaderno de Nueva York ("New York Notebook"), said that any major poet has to write about both New York and spring, at least once in a lifetime. The same could be said about M51, the Whirlpool Galaxy, in the context of astronomical imaging. Every relevant collection of astronomical photographs has to include this object at least once, if not more times, and every new look to this magnificent object reveals different aspects of this grand-design spiral galaxy.

Galaxy M51 was discovered by Charles Messier in 1773, but its outstanding spiral structure was first perceived by William Parsons (Earl of Rosse) in 1845, using his huge reflecting telescope, the Leviathan of Parsonstown. A large telescope is needed to see its intricate shape, but even small amateur telescopes reveal that this galaxy is not isolated, but has a small companion, the dwarf irregular galaxy NGC 5195.

Now it is clear that these two stellar systems are colliding and that the outstanding spiral shape of M51 is due, mainly, to the tidal forces unleashed during this process. Just by chance, we see the disk of M51 face on from Earth, what allows studying it in detail. At a distance of 23 millions of light-years, the apparent dimensions of M51 mean that that galaxy has to be quite similar to our own, yet somewhat smaller.

M51 and its companion are performing a cosmic dance that, during the last 500 million years has made NGC 5195 pass twice through the disk of M51. Now, the small galaxy is located slightly behind the disc of the Whirlpool, and moving away from us.

The interaction of both galaxies induces a bunch of collateral effects, being the spiral structure of the main galaxy only one of them. When galaxies collide, their stars do not crash ones against the others. Instead, they suffer strong alterations in their trajectories, what usually implies that many of them are expelled into the intergalactic space. This has happened to many stars from the secondary galaxy: streams of stars stripped of from NGC 5195 extend over the left (north) part of the image as a fuzzy fog. Many of the worlds in that area are doomed to get lost into the emptiness of space, as they move far away from their parent galaxies.

The gaseous content of colliding galaxies gets compressed and this triggers violent bursts of star formation (starbursts). Star forming regions can be detected thanks to the pinkish glow of ionised hydrogen. Images taken in the so-called H-alpha colour reveal where the gas is ionised by newborn stars. For this reason, we offer the M51 image in two versions: true colour and H-alpha enhanced.

The true-colour image has been obtained gathering light through a set of three filters that mimic the chromatic sensitivity of the human eye. The final colour balance has been done in such a way that the light coming from both galaxies, put together, is considered as white. This way, the contrast among the different stellar populations in the field is more obvious. Particularly, the spiral galaxy exhibits bluish hues due to the massive, young and hot stars that populate its disk. This contrasts with the yellowish colours in the satellite galaxy, coming from lighter, older and colder stars.

M51 displays a star-forming activity much stronger than isolated galaxies like our own. This fact is highlighted in the H-alpha-enhanced image. As could be expected, star-forming activity closely follows the areas where younger and more massive stars are seen: the bluish spiral arms. But H-alpha emissions in M51 are not restricted to the spiral arms, but extend also into other areas. One of the most outstanding and intriguing features of this image is the fuzzy region of faint H-alpha emission to the north (left) of NGC 5195, a detail seldom seen before and closely related, too, to the effects of the collision on the gaseous content of these galaxies.

Many of the tiny points in the image are stars belonging to our own Galaxy. But a detailed inspection reveals that most of the small spots are other background galaxies. Small and remote extragalactic systems, of many shapes and colours, can be seen down to the edge of infinity in this photo. The two most outstanding background galaxies are the bright edge-on spiral galaxy IC 4277 seen close to the lower left (north-east) corner of the frame, and the small irregular galaxy IC 4278, to the right of the previous one, below (east) from the bridge of stars that seems to link M51 with NGC 5195.

This image has been obtained with the Zeiss 1.23 m reflector of Calar Alto Observatory (CAHA) as a part of the Public Outreach Project conducted by Foundation Descubre with this instrument. The observations have been planned and carried out by the Documentary School of Astrophotography (DSA), and the data have been processed by this organisation with the collaboration of the Astronomical Observatory of the University of Valencia (OAUV), using the software package PixInsight.


Story Source:

The above story is based on materials provided by Calar Alto Observatory-CAHA. Note: Materials may be edited for content and length.


Cite This Page:

Calar Alto Observatory-CAHA. "New look into Whirlpool Galaxy." ScienceDaily. ScienceDaily, 15 June 2010. <www.sciencedaily.com/releases/2010/06/100611085351.htm>.
Calar Alto Observatory-CAHA. (2010, June 15). New look into Whirlpool Galaxy. ScienceDaily. Retrieved October 26, 2014 from www.sciencedaily.com/releases/2010/06/100611085351.htm
Calar Alto Observatory-CAHA. "New look into Whirlpool Galaxy." ScienceDaily. www.sciencedaily.com/releases/2010/06/100611085351.htm (accessed October 26, 2014).

Share This



More Space & Time News

Sunday, October 26, 2014

Featured Research

from universities, journals, and other organizations


Featured Videos

from AP, Reuters, AFP, and other news services

Raw: China Launches Moon Orbiter

Raw: China Launches Moon Orbiter

AP (Oct. 24, 2014) — China launched an experimental spacecraft Friday to fly around the moon and back to Earth in preparation for the country's first unmanned return trip to the lunar surface. (Oct. 24) Video provided by AP
Powered by NewsLook.com
China Prepares Unmanned Mission To Lunar Orbit

China Prepares Unmanned Mission To Lunar Orbit

Newsy (Oct. 23, 2014) — The mission is China's next step toward automated sample-return missions and eventual manned missions to the moon. Video provided by Newsy
Powered by NewsLook.com
Russian Cosmonauts Kick Off Final Spacewalk of 2014

Russian Cosmonauts Kick Off Final Spacewalk of 2014

Reuters - US Online Video (Oct. 22, 2014) — Russian cosmonauts Maxim Suraev and Alexander Samokutyaev step outside the International Space Station to perform work on the exterior of the station's Russian module. Rough Cut (no reporter narration) Video provided by Reuters
Powered by NewsLook.com
Comet Siding Spring Grazes Mars' Atmosphere

Comet Siding Spring Grazes Mars' Atmosphere

Newsy (Oct. 19, 2014) — A comet from the farthest reaches of the solar system passed extremely close to Mars this weekend, giving astronomers a rare opportunity to study it. Video provided by Newsy
Powered by NewsLook.com

Search ScienceDaily

Number of stories in archives: 140,361

Find with keyword(s):
 
Enter a keyword or phrase to search ScienceDaily for related topics and research stories.

Save/Print:
Share:  

Breaking News:

Strange & Offbeat Stories

 

Space & Time

Matter & Energy

Computers & Math

In Other News

... from NewsDaily.com

Science News

Health News

Environment News

Technology News



Save/Print:
Share:  

Free Subscriptions


Get the latest science news with ScienceDaily's free email newsletters, updated daily and weekly. Or view hourly updated newsfeeds in your RSS reader:

Get Social & Mobile


Keep up to date with the latest news from ScienceDaily via social networks and mobile apps:

Have Feedback?


Tell us what you think of ScienceDaily -- we welcome both positive and negative comments. Have any problems using the site? Questions?
Mobile iPhone Android Web
Follow Facebook Twitter Google+
Subscribe RSS Feeds Email Newsletters
Latest Headlines Health & Medicine Mind & Brain Space & Time Matter & Energy Computers & Math Plants & Animals Earth & Climate Fossils & Ruins