#coma galaxy cluster
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Deep look into the past
This picture of the constellation of Coma Berenices isnt very spectacular on first glance. But within this constellation lays the Coma galaxy cluster, a group of 1000 Galaxies each with millions .... billions of own stars.
Most of those galaxies are roughly 300 Million lightyears away ... a distance hard to process for the human mind.
In the second picture each galaxy visible is marked in red or blue depending on the catalog it registered in. Who wanna count them? Who wanna guess on how many civilization we are looking at?
Bilddaten:
- RGB 63 x 300s / Gain 100
- 25 Flat Dark
- 25 Flat Darks
- 25 Darks
Setup:
- Skywatcher 150/750 PDS
- Omegon 571C
- Skywatcher EQ6R Pro
- Zwo Asi 178mm
#astronomy#universe#space#space photography#astrophotography#night sky#astrophysics#nature#coma galaxy cluster
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It occurred to me that since I was last on Tumblr, I got a new astrophotography setup. I've only used it a few times, but most nights I'd rather haul out Lyra the Dob for a quick and easy setup.
The scope part of the new rig arrived the day before I left for a week-long trip to dark skies as a mentor at an astronomy camp. I got the go-ahead to bring it; the seeing was bad all week so the stars were bloated, but I still had a great time.
From that week:
At top left is Messier 109; the bright star is the bottom-left corner of the Big Dipper's cup. I'd chosen it for first light because I'd never imaged it before and it has a beautiful barred spiral structure. In this cropped version you can see the structure and three faint satellite galaxies to the right, running in a row from above the galaxy to just below and right of it.
The one at bottom right is the Coma Galaxy Cluster. The seeing made it hard to tell, but *most* of the points of light in that image are individual galaxies and not stars. I could see a few dozen through my visual scope one night. It was glorious.
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2024 March 27
A picture filled with fuzzy yellow spots is presented. All of the yellow spots are galaxies, and most of the galaxies are members of the Coma Cluster of Galaxies. The two bright blue dots are foreground stars in our own Milky Way Galaxy.
The Coma Cluster of Galaxies
Image Credit & Copyright: Joe Hua
Explanation: Almost every object in the featured photograph is a galaxy. The Coma Cluster of Galaxies pictured here is one of the densest clusters known - it contains thousands of galaxies. Each of these galaxies houses billions of stars - just as our own Milky Way Galaxy does. Although nearby when compared to most other clusters, light from the Coma Cluster still takes hundreds of millions of years to reach us. In fact, the Coma Cluster is so big it takes light millions of years just to go from one side to the other. Most galaxies in Coma and other clusters are ellipticals, while most galaxies outside of clusters are spirals. The nature of Coma's X-ray emission is still being investigated.
#astronaut#astronomers#not astrology#star#stars#astronomy#outer space#art#space#artist#galaxy#coma#milky way#cluster#coma cluster#x ray#million years#spiral
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Lensed Seahorse
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Thousands of Coma Cluster Galaxies - September 17th, 1995.
"Almost every object in the above photograph is a galaxy. The Coma Cluster of galaxies pictured is a dense cluster containing many thousands of galaxies. Many of these galaxies contain as many stars as our own Milky Way galaxy. Although nearby when compared to most other clusters, light from the Coma Cluster still takes hundreds of millions of years to reach us. In fact, the Coma Cluster is so big it takes light millions of years just to go from one side to the other! This picture was created at the WWW site Skyview, a "virtual observatory" where it is possible to view any part of the sky in wavelengths from radio to gamma-ray."
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During the early 1930s, Fritz Zwicky, a professor of astronomy at the California Institute of Technology (a famously caustic scientist whose appreciation for symmetry led him to call his colleagues spherical bastards because, he explained, they were bastards any way you looked at them), realized that the outlying galaxies in the Coma cluster, a collection of thousands of galaxies some 370 million light-years from earth, were moving too quickly for their visible matter to muster an adequate gravitational force to keep them tethered to the group.
"The Fabric of the Cosmos" - Brian Greene
#book quotes#the fabric of the cosmos#brian greene#nonfiction#30s#1930s#20th century#fritz zwicky#astronomy#california institute of technology#caustic#bastard#galaxy#coma cluster#gravity
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*M99
NGC 4254 by NASA's James Webb Space Telescope
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An image captured by the Dark Energy Camera (DECam) depicts the Coma Cluster, also known as Abell 1656, so named because it's part of the constellation Coma Berenices. DECam was designed to conduct a long-term investigation of dark energy but is also useful for other types of astronomical studies. The Coma Cluster is linked to the study of dark matter since the inconsistency between the estimate of its overall mass and the measurement of its gravitational effects stimulated the research that led to today's dark matter models.
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2024 May 2
M100: A Grand Design Spiral Galaxy Image Credit & Copyright: Drew Evans
Explanation: Majestic on a truly cosmic scale, M100 is appropriately known as a grand design spiral galaxy. The large galaxy of over 100 billion stars has well-defined spiral arms, similar to our own Milky Way. One of the brightest members of the Virgo Cluster of galaxies, M100, also known as NGC 4321 is 56 million light-years distant toward the well-groomed constellation Coma Berenices. In this telescopic image, the face-on grand design spiral shares a nearly 1 degree wide field-of-view with slightly less conspicuous edge-on spiral NGC 4312 (at upper right). The 21 hour long equivalent exposure from a dark sky site near Flagstaff, Arizona, planet Earth, reveals M100's bright blue star clusters and intricate winding dust lanes which are hallmarks of this class of galaxies. Measurements of variable stars in M100 have played an important role in determining the size and age of the Universe.
â Source: apod.nasa.gov/apod/ap240502.html
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Why Does the Ortolan Sing?
A human AU Good Omens fanfic
(View uncensored art on AO3)
Chapter 20: So Much For Stardust
Rating: Explicit
Summary:
Following his motherâs death, Azira sets out to prepare his familyâs bookshop for reopening. While appreciating the shopâs new sign, he hears the beckon of a sirenâs song sounding from the coffee shop over the road. He succumbs to temptation to find the source of the hypnotic voice is an auburn-haired songbird. Intrigued by the singerâs beauty and haunted by his apparent loneliness, Azira is determined to introduce himself. Thereâs only one problem: the musicianâs menacing, jealous, and possessive partner.
CW: Domestic abuse, loss of a loved one, adultery, toxic relationship, murder, blood, organized crime
Excerpt from chapter 20:
âSpace is incredible, you know?â Crowleyâs smile broadened as he stared up at Godâs canvas. âItâs true eternity. So vast and limitless, weâre constantly finding something new. Even when Earth is long gone, the space we used to occupy will receive the light from star systems weâve never known, never named, and the light from Earth will do the same. Weâre fleeting, but space isnât.â
âThatâs beautifulâŠâ Azira sighed. âAnd slightly tragic. Nothing lasts forever, I suppose.â
âSome things do.â Crowley took a deep breath of the fresh, country air. âHumans give names and stories to the stars, and I wonder who else out there, seeing the same stars from a different angle, have done the same. Like over there,â Crowley motioned to a cluster of stars Azira couldnât differentiate from any others. âComa Berenices. Humans looked at those stars and saw the hair of an Egyptian queen, sacrificed to Aphrodite to ensure her husbandâs return from battle. Something so human. Or the Andromeda Galaxy⊠one of our neighbors. Named for a beauty whose parents angered the Gods, causing her to be sacrificed to a monster. The stories we assign them wonât last for eternity, but their light always reaches somewhere, even once theyâre gone. And thereâs an infinite number of them to do just that.â
âWhen you put it like that, eternity is⊠a hard concept to grasp.â Azira pondered for a moment. Heâd had philosophical conversations with his parents, but eternity was never a topic they touched on. âI admit, my mind usually stays grounded in the stories in books; I donât tend to consider just how insignificant that all is.â
Crowley eyed Azira at askance, then rolled onto his side, propping his head up on his hand and smiling. âEternity is a mountain made of diamonds.â
âA what?â Azira grinned.
âThereâs a mountain made of diamonds, a hundred miles wide and a hundred miles high, and every thousand years a bird comes and sharpens its beak on the mountain.â
âThe same bird?â
Crowley waved his hand dismissively. âWeâre talking diamond mountains; you want to harp on the age of the bird?â
âRight,â Azira chuckled. âCarry on.â
âSo this bird sharpens its beak on the mountain, scraping away a tiny piece every time. Once that mountain has completely worn away, one second of eternity has passed.â
Azira stared up at Crowley, his face framed in the falling stars and glittering diamonds of eternity, sending their light to Earth. His lips parted, a soft gasp leaving him as he took in the eternal beauty, incomparable in his mind to the fleeting beauty that was Crowley. Crowleyâs soft smile and gentle eyes were gazing at him with the kind of love actors attempt to portray in movies. It was so believable, as he watched the old black-and-whites with his mother, until he witnessed it himself.
âMake love to me under the stars,â Azira whispered. âEternally.â
Continue from chapter 20 here.
Thank you so much to everyone at @goodomensafterdark for your help and putting up with my millions of questions! đ„°
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*M99.
Itâs oh-so-easy to be mesmerized by this spiral galaxy known as NGC 4254. Follow its clearly defined arms, which are brimming with stars, to its center, where there may be old star clusters and, sometimes, active supermassive black holes. NASAâs James Webb Space Telescope delivered highly detailed scenes of this spiral galaxy in a combination of near- and mid-infrared light.
Image Credit & Copyright: NASA, ESA, CSA, STScI, Janice Lee (STScI), Thomas Williams (Oxford), and the PHANGS team
#reblog#astronomy#m99#spiral galaxy#virgo cluster#coma berenices#infrared#james webb space telescope
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The Coma Cluster of Galaxies
Credits: U. Toronto, Kitt Peak National Obs.
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went out with my telescope tonight and got pictures of the black eye galaxy and the ring nebula :3
the black eye galaxy is a spiral galaxy about 17 million light years away, with an inner disk dense with dark dust that gives it its name
the ring nebula is a planetary nebula about 2500 light years away. planetary nebulae form when a red giant star at the end of its life sheds its outer layers into space, leaving a roughly spherical nebula with the star's remnant core as a tiny white dwarf in the center. our sun will share a similar fate billions of years from now
these two pictures kinda illustrate an interesting thing - the density of stars in them are drastically different. the black eye galaxy is located near the north galactic pole in the constellation coma berenices, so when you look towards it, you're looking "up" out of our galaxy. there's not too many stars in the way. this gives us a clear view of distant galaxies, and is why coma berenices and other nearby constellations (like canes venatici, ursa major, leo, and virgo) have soooooo many visible galaxies. the ring nebula on the other hand is located close to the galactic plane, which is very dense with stars. that plus the vast dust clouds in the galactic disk obscure our view of distant galaxies. instead we see things like star clusters and nebulae
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Hubble takes a look at tangled galaxies MCG+05-31-045
This NASA/ESA Hubble Space Telescope image depicts the cosmic tangle that is MCG+05-31-045, a pair of interacting galaxies located 390 million light-years away and a part of the Coma galaxy cluster.
The Coma Cluster is a particularly rich cluster that contains more than a thousand known galaxies. Amateur astronomers can easily spot several of these in a backyard telescope (such as Caldwell 35).
Most of them are elliptical galaxies, and that's typical of a dense galaxy cluster like the Coma Cluster: many elliptical galaxies form through close encounters between galaxies that stir them up, or even collisions that rip them apart.
While the stars in interacting galaxies can stay together, their gas is twisted and compressed by gravitational forces and rapidly used up to form new stars. When the hot, massive, blue stars die, there is little gas left to form new generations of young stars to replace them.
As spiral galaxies interact, gravity disrupts the regular orbits that produce their striking spiral arms. Whether through mergers or simple near misses, the result is a galaxy almost devoid of gas, with aging stars orbiting in uncoordinated circles: an elliptical galaxy.
It's very likely that a similar fate will befall MCG+05-31-045. As the smaller spiral galaxy is torn up and integrated into the larger galaxy, many new stars will form, and the hot, blue ones will quickly burn out, leaving cooler, redder stars behind in an elliptical galaxy, much like others in the Coma Cluster. But this process won't be complete for many millions of years.
IMAGE: This Hubble image features a pair of interacting spiral galaxies called MCG+05-31-045. Credit: ESA/Hubble & NASA, R. J. Foley (UC Santa Cruz)
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Even galaxies get tangled !
This new #HubbleFriday view captures a pair of interacting galaxies located 390 million light-years away. They go by MCG+05-31-045... it really rolls off the tongue.
This cosmic tangle will likely eventually result in a galaxy merger. As the smaller spiral galaxy is integrated into the larger galaxy, many new stars will form, and the hot, blue ones will quickly burn out, leaving cooler, redder stars behind to form what's known as an elliptical galaxy.
MCG+05-31-045 is part of the Coma galaxy cluster, which contains over a thousand known galaxies, many of which are ellipticals.
For more information, visit the link in our bio!
Image description: In the center is a large, oval-shaped galaxy, with a shining, ringed core. Left of its center is a second, smaller galaxy with two spiral arms. The galaxy pair is so close that they appear to be merging: a tail of material with a few glowing spots connects from one of the smaller galaxyâs spiral arms to the larger galaxy. A faint halo surrounds both galaxies. Several stars are visible around the pair.
Image credit: ESA/Hubble & NASA, R. J. Foley (UC Santa Cruz)
#space#nasa#universe#art#astronomy#science#galaxy#moon#stars#cosmos#spacex#scifi#astrophotography#photography#earth#astronaut#love#alien#nature#mars#spaceart#sky#spaceexploration#planets#aliens#spaceship#spacetravel#rocket#digitalart#design
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The search for dark matter
Post #6 on Physics and Astronomy, 06/10/23
Welcome back.Â
This time, Iâm going to be talking about how astronomers and physicists have made an effort to detect and provide evidence for the existence of dark matter.Â
To recap from my first issue, itâs worth talking about what dark matter actually is. Itâs a type of matter estimated to make up about 80% of the Universeâs matter. To date, it hasnât been detected. Light passes straight through, it is assumed, however we infer the existence of such a substance due to its gravitational influence.Â
We can take an example from the Bullet Cluster. This is a pair of galaxy clusters that collided head-on a while ago. That pink mist you see in the photo is hot gas, and within it most of the regular matter. The blue mist, on the other hand, is dark matter, and where most of the mass of these two galaxies were in this photo.Â
Vera Rubin and Kent Ford
Vera Rubin and Kent Ford were two astronomers who had worked together to observe the Andromeda Galaxy, more specifically the rotational velocities of concentric regions from the center. The prediction was that, the further you looked from the center, the less the velocity of the stars within that region, since a greater centripetal force would be required to maintain a high-velocity orbit. This, however, was not the case.Â
It was observed that the velocity remained nearly constant the further you went out. Wait a minute, though, this didnât make senseâthat velocity was high enough, in theory, to make the stars fly off into space. But they werenât.
These findings matched those of Fritz Zwicky. He was a Swiss astronomer who had studied the Coma galaxy cluster. He made the same observationâthe speeds were so high that the stars should just have been flung off into space. His findings, however, were ignored.
Experiments to detect dark matter
So far, experiments to detect dark matter have been largely unsuccessful. Some of these include PICASSO, LUX-ZEPLIN, EURECA, FUNK, KIMS, DarkSide, Edelweiss, DARWIN, and DAMA/LIBRA, which is what Iâm exploring next.Â
This detector in particular, introduced promising results which ended up the subject of dispute. DAMA/LIBRA, which hoped to capture activity from WIMPs (Weakly Interacting Massive Particles), returned a signal with a period of one year. This looked to be one step closer to affirming dark matterâs existenceâhowever, COSINE-100, an experiment set up to mirror that of DAMA/LIBRA, could not reach those same results, which led to the belief that the signal detected could be from some other factor.
The search for dark matter is one that interests me very much. Itâs like telling someone in the Stone Age that metal exists, and they should go find it. Except, dark matter is seemingly even more impossible to find, since we canât perceive it, with the human eye or the best of our current technology. Which, I guess you could argue, would be exactly how the Stone Age person would have felt, but you understand my point.
That said, itâs something Iâm eagerly watching. The day we find something promising? Youâll hear it first from me.
#physics#studyblr#astronomy#engineering#astrophysics#stem#sixth form#alevels#dark matter#dark energy#mathematics#physicsblr#mathsblr
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