APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

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Expand view Topic review: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by douglas » Fri Mar 10, 2017 12:46 pm

NGC 1961/Arp 184

http://asterisk.apod.com/viewtopic.php? ... 61#p232436

Extremely disrupted "spiral arms" with star formation at arms' extremity:
http://cseligman.com/text/atlas/ngc19a.htm#1961
"NGC 1961 is about 185 million light years away. Given that and the brighter central galaxy's apparent size of 4.1 by 2.2 arcmin, it spans about 220 thousand light years; while the 4.9 by 4.2 arcmin wide region that includes the very faint northern arms spans about 260 thousand light years."

http://sleshin.startlogic.com/stargazer ... itemId=728

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by douglas » Thu Mar 09, 2017 12:25 pm

Here you go: collisional mass accretion.

"To appreciate this galaxy, its optical-IR luminosity is nine times that of M31."

"This halo accretion rate is two orders of magnitude too low to assemble the stellar mass of this galaxy within a Hubble time.
Therefore, significant accretion must have occurred via some other mode, such as cold flows
or mergers, to produce the stellar mass seen in this galaxy today, confirming the conclusion
drew in NGC 1961 (Anderson & Bregman 2011)."

XMM-Newton Detects a Hot Gaseous Halo in the Fastest Rotating Spiral Galaxy UGC 12591
https://arxiv.org/PS_cache/arxiv/pdf/11 ... 0324v1.pdf

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by Chris Peterson » Thu Mar 09, 2017 12:09 am

john_erickson wrote:
jonas s wrote:The quoted spin rate as a linear velocity, km/sec. What is the angular rate of spin or is the quoted km/sec at baseline distance from center of rotation?
As Art pointed out in response to that question, galaxies typically have a near constant linear (tangential) velocity, independent of radius. So this is the measured velocity anywhere you look, not at any particular distance from the center. (That also means that the angular velocity varies with radius.)

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by john_erickson » Thu Mar 09, 2017 12:02 am

jonas s wrote:The quoted spin rate as a linear velocity, km/sec. What is the angular rate of spin or is the quoted km/sec at baseline distance from center of rotation?

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by neufer » Wed Mar 08, 2017 12:43 pm

MartinNi wrote:
neufer wrote:
Bopps wrote:
The orbits of earth satellites are at altitudes defined by their velocity ... higher velocity to maintain higher altitudes. As their velocity decays they eventually fall back to earth. If galaxy objects are at the same linear velocity, they would be "falling" towards the center. Does this explain arms spiraling inward towards the center black hole of galaxies?
The (~circular) orbits of earth satellites are at altitudes defined by their velocity
... higher velocities are needed to maintain lower altitudes:
Centrifugal force = mv2/r = gravitational force = GmM/r2

Hence: v2 = GM/r : or v = sqrt (GM/r)
For (~circular) orbital velocity to be constant
the gravitational force of galaxies must drop off more slowly as 1/r not 1/r2.
Centrifugal force = mv2/r = gravitational force = Cm/r (; i.e., total dark mass M grows as Cr/G)

Hence: v2 = C : or v = sqrt (C)

(; i.e., UGC 12591's dark mass density is ~4 times that of the Milky Way.)
Hi Art, isn't this simple formalism for point masses (or masses with radial symmetric distibution, when located "outsite" of them) rather inadequate (and so the estimated "dark mass density" wrong) for a much more non-spherical mass distribution, which a flat disk like UGC 12591 represents ?

What about a correct formalism for spiral galaxies ?
Hi, Martin.

I refer you to: http://physics.stackexchange.com/questi ... e-spheroid
However, to first order what I wrote still stands...
the main difference being the vertical oscillation vis-a-vis the galactic disk
(which involves the, as yet, unknown flatness of the dark matter galactic disk).

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by MartinNi » Wed Mar 08, 2017 11:02 am

neufer wrote:
Bopps wrote:
The orbits of earth satellites are at altitudes defined by their velocity ... higher velocity to maintain higher altitudes. As their velocity decays they eventually fall back to earth. If galaxy objects are at the same linear velocity, they would be "falling" towards the center. Does this explain arms spiraling inward towards the center black hole of galaxies?
The (~circular) orbits of earth satellites are at altitudes defined by their velocity
... higher velocities are needed to maintain lower altitudes:
Centrifugal force = mv2/r = gravitational force = GmM/r2

Hence: v2 = GM/r : or v = sqrt (GM/r)
For (~circular) orbital velocity to be constant
the gravitational force of galaxies must drop off more slowly as 1/r not 1/r2.
Centrifugal force = mv2/r = gravitational force = Cm/r (; i.e., total dark mass M grows as Cr/G)

Hence: v2 = C : or v = sqrt (C)

(; i.e., UGC 12591's dark mass density is ~4 times that of the Milky Way.)
Hi Art,
isn't this simple formalism for point masses (or masses with radial symmetric distibution, when located "outsite" of them) rather inadequate (and so the estimated "dark mass density" wrong) for a much more non-spherical mass distribution, which a flat disk like UGC 12591 represents ?
What about a correct formalism for spiral galaxies ?

Kind regards
Martin

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by douglas » Wed Mar 08, 2017 5:49 am

"Classified as an S0/Sa galaxy, UGC 12591 sits somewhere between a lenticular and a spiral galaxy.

Also known as LEDA 71392 and 2MASX J23252175+2829425, UGC 12591 lies just under 400 million light-years away from us in the westernmost region of the Pisces-Perseus Supercluster, a chain of galaxy clusters that stretches out for hundreds of millions of light-years — one of the largest known structures in the cosmos."

http://www.sci-news.com/astronomy/hubbl ... 04653.html

http://space.wikia.com/wiki/Lenticular_galaxy

I'm going to go with the collision growth scenario. Those spiral arms look disconnected from the core, and circularized.

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by sillyworm » Tue Mar 07, 2017 9:58 pm

All these wondrous beautiful elusive mysterious mind-bending exotic Galaxies....and we may never even get to explore Andromeda.Imagining WHY & HOW are two of the most exiting mind journeys.

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by Ann » Tue Mar 07, 2017 8:24 pm

To return to fast-rotating galaxy UGC 12591, other galaxies rotate fast, too. NGC 488 is a particularly whirligig-like specimen.
[c]NGC 488. Photo: Adam Block/Caelum Observatory.[/c]
Charles J. Peterson (a relative, Chris?) wrote in Astronomical Journal, vol. 85, Mar. 1980, p. 226-229:

The rotation curve of NGC 488 has been measured out to a radius of 20 kpc, at which point the velocity is 363 km−1 and continuing to increase with radius. This rotational velocity is the largest known for an Sb galaxy. For a mass model based on the thin-disk approximation of Kuzmin [Publ. Tartu Astron. Obs. 32, 211 (1952)], we find the mass and mass-luminosity interior to 20 kpc are M ⪆ 4.0 X 1011 M and <M/L>B ⪆ 3.6. Exterior to the nuclear region, the mass-luminosity relation shows only a gentle increase with radius.
Phew! I couldn't copy that from the page, so I had to write it all in by hand, including all those pesky mathematical symbols and signs!

Ann

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by neufer » Tue Mar 07, 2017 5:56 pm

Chris Peterson wrote:
pipejazz wrote:
Numerous galaxies, is this gravational lensing or reality? :D
Gravitational lensing is reality! But I don't see any obvious lensing in this image. (And the object in this image is much too close to be an effective lens.)
If the brightest object below UGC 12591 is, in fact, a distant galaxy then I calculate that gravitational lensing is probably making it appear to be ~34" away (off towards the bottom) when it should otherwise have appeared to be just ~32" away (off towards the bottom). This qualifies as significant though not "obvious lensing." In fact, all those distant galaxies appear ~2" (i.e., 4,000 light years) further away from the center of UGC 12591 than they would otherwise. And if there had been a distant galaxy or quasar sitting directly behind UGC 12591 it would probably have formed a noticeable ring (or Einstein cross) with a diameter of ~2-3" (i.e., 4 to 6 thousand light years)...but there isn't.

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by MrE » Tue Mar 07, 2017 5:52 pm

Not visible in the cropped image but in the enlargement when fully sized, in the upper right corner is a very nice bright galaxy. to the left of it is a very red (faint) galaxy with what appears to be a brightly shining supernova

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by Ann » Tue Mar 07, 2017 5:24 pm

RJN wrote:
Rajesh Kalmady wrote:The light from the galaxy left 400 million years ago, not 400 million light years ago.
Oops! Yes. Fixed it on the main NASA APOD. Thanks!

- RJN
Good! We don't want Starship Asterisk* to sound like Han Solo.
Click to play embedded YouTube video.
Ann

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by Fred the Cat » Tue Mar 07, 2017 4:42 pm

Perhaps dark matter is more akin to the grooves on a record album. It keeps the tonearm on track despite its rotational speed. :wink:

How does that sound :?: It's a gas. :ssmile:

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by neufer » Tue Mar 07, 2017 4:29 pm

https://en.wikipedia.org/wiki/ISOHDFS_27 wrote:

<<ISOHDFS 27 is the most massive spiral galaxy in the Hubble Deep Field South known so far which is 130,000 light-years in diameter. It is approximately 6 billion light years from Earth. It has a mass of 1.04×1012 solar masses (M), about four times as massive as the Milky Way.

The preceding most massive spiral was UGC 12591.>>
https://en.wikipedia.org/wiki/Segue_2 wrote: <<Segue 2 is a dwarf spheroidal galaxy situated in the constellation Aries and discovered in 2009 in the data obtained by Sloan Digital Sky Survey. The galaxy is located at the distance of about 35 kpc (110,000 ly) from the Sun and moves towards the Sun with the speed of 40 km/s. It is classified as a dwarf spheroidal galaxy (dSph) meaning that it has an approximately round shape with the half-light radius of about 34 pc. Segue 2 is located near the edge of Sagittarius Stream and at the same distance. It may once have been a satellite of Sagittarius Dwarf Elliptical Galaxy or its star cluster.

Segue 2 is one of the smallest and faintest satellites of the Milky Way—its integrated luminosity is about 800 times that of the Sun (absolute visible magnitude of about −2.5), which is much lower than the luminosity of the majority of globular clusters. Circa 1,000 stars are supposed to exist within the galaxy. However, the mass of the galaxy—about 550,000 solar masses—is substantial, corresponding to the mass to light ratio of about 650. In June 2013 the The Astrophysical Journal reported that Segue 2 was bound together with dark matter.

The stellar population of Segue 2 consists mainly of old stars formed more than 12 billion years ago. The metallicity of these old stars is also very low at [Fe/H] < −2, which means that they contain at least 100 times less heavy elements than the Sun. The stars of Segue 2 were probably among the first stars to form in the Universe. Currently, there is no star formation in Segue 2.>>

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by rstevenson » Tue Mar 07, 2017 3:42 pm

Wow! What a view!

I wonder how many of those small round blueish-white spots near the galaxy are its globular clusters? There look to be many dozens of them.

Rob

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by neufer » Tue Mar 07, 2017 3:25 pm

RJN wrote:
Rajesh Kalmady wrote:
The light from the galaxy left 400 million years ago, not 400 million light years ago.
Oops! Yes. Fixed it on the main NASA APOD. Thanks!
https://en.wikipedia.org/wiki/Tree#Evolutionary_history wrote: <<The earliest tree-like organisms were tree ferns, horsetails and lycophytes, which grew in forests in the Carboniferous period. The first tree may have been Wattieza, fossils of which have been found in New York State in 2007 dating back to the Middle Devonian (about 385 million years ago). Prior to this discovery, Archaeopteris was the earliest known tree. Both of these reproduced by spores rather than seeds and are considered to be links between ferns and the gymnosperms which evolved in the Triassic period. The gymnosperms include conifers, cycads, gnetales and ginkgos and these may have appeared as a result of a whole genome duplication event which took place about 319 million years ago. Ginkgophyta was once a widespread diverse group of which the only survivor is the maidenhair tree Ginkgo biloba. This is considered to be a living fossil because it is virtually unchanged from the fossilised specimens found in Triassic deposits.

During the Mesozoic (245 to 66 million years ago) the conifers flourished and became adapted to live in all the major terrestrial habitats. Subsequently, the tree forms of flowering plants evolved during the Cretaceous period. These began to dominate the conifers during the Tertiary era (66 to 2 million years ago) when forests covered the globe. When the climate cooled 1.5 million years ago and the first of four ice ages occurred, the forests retreated as the ice advanced. In the interglacials, trees recolonised the land that had been covered by ice, only to be driven back again in the next ice age.>>

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by RJN » Tue Mar 07, 2017 3:08 pm

Rajesh Kalmady wrote:The light from the galaxy left 400 million years ago, not 400 million light years ago.
Oops! Yes. Fixed it on the main NASA APOD. Thanks!

- RJN

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by gadieid » Tue Mar 07, 2017 3:05 pm

Great photo! I've counted at least 40 other galaxies and that without looking at the high resolution picture.

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by Chris Peterson » Tue Mar 07, 2017 2:45 pm

pipejazz wrote:Numerous galaxies, is this gravational lensing or reality? :D
Gravitational lensing is reality! But I don't see any obvious lensing in this image. (And the object in this image is much too close to be an effective lens.)

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by Chris Peterson » Tue Mar 07, 2017 2:43 pm

De58te wrote:In the expanded view next to the galaxy pointed out by Coil Smoke, there are two neat blue galaxies really close to each other. I wonder if they are colliding?
Also look at the neat all red galaxy just above the ESA letters. I wonder why the galaxy is all red. Could it be due to the expansion of the universe and all the distant galaxies are red shifted because they are moving away from us? There are about 2 or 3 other red galaxies along the bottom, but through the rest of the photograph the galaxies are either white or blue. There are a lot of blue distant galaxies visible. Would those galaxies be blue shifted because they are all moving towards us? That would be at odds with the distant galaxies being red shifted.
You have to be careful comparing color and redshift. First of all, this isn't a natural color image- the entire visual range is mapped to cyan, and a non-overlapping near IR range is mapped to orange. Second, when you redshift you move otherwise invisible short wavelengths into the visible, and you move otherwise visible longer wavelengths into the IR. The effect that has on perceived color isn't always obvious.

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by leats » Tue Mar 07, 2017 2:30 pm

Thank you for providing a reference point relative to earth's evolution for the time the light left this galaxy. I'd like to see this done for all photos of interstellar objects. Staggering numbers like 5 million light years or 1 billion light years... have more meaning (to me) if I can associate them with a period in earth's history.

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by pipejazz » Tue Mar 07, 2017 2:17 pm

Numerous galaxies, is this gravational lensing or reality? :D

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by Ann » Tue Mar 07, 2017 2:03 pm

De58te wrote:In the expanded view next to the galaxy pointed out by Coil Smoke, there are two neat blue galaxies really close to each other. I wonder if they are colliding?
Also look at the neat all red galaxy just above the ESA letters. I wonder why the galaxy is all red. Could it be due to the expansion of the universe and all the distant galaxies are red shifted because they are moving away from us? There are about 2 or 3 other red galaxies along the bottom, but through the rest of the photograph the galaxies are either white or blue. There are a lot of blue distant galaxies visible. Would those galaxies be blue shifted because they are all moving towards us? That would be at odds with the distant galaxies being red shifted.
Well, the two most obvious galaxies that I can see, that are definitely interacting and close to the "pale bright ghost galaxy" at upper right - I like that desciption :D - aren't blue, but yes, they really seem to be interacting. So yes, they should collide in a few (hundred) million years from now. (And of course, if we could see what these galaxies have evolved into hundreds of millions of years after the light that we can see actually left them - which we can't - we would probably see that they have already collided.)

The very red background galaxies do indeed owe their color to redshift reddening, although it is quite possible that dust reddening also contributes to their color.

The very blue galaxies, by the way, were forming hot bright stars at a furious rate at the time when the light that has reached us left them. At that time they emitted copious amounts of ultraviolet light, which has since been redshiftet into the blue light that we now can see.

Ann

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by neufer » Tue Mar 07, 2017 1:05 pm

Bopps wrote:
The orbits of earth satellites are at altitudes defined by their velocity ... higher velocity to maintain higher altitudes. As their velocity decays they eventually fall back to earth. If galaxy objects are at the same linear velocity, they would be "falling" towards the center. Does this explain arms spiraling inward towards the center black hole of galaxies?
The (~circular) orbits of earth satellites are at altitudes defined by their velocity
... higher velocities are needed to maintain lower altitudes:
Centrifugal force = mv2/r = gravitational force = GmM/r2

Hence: v2 = GM/r : or v = sqrt (GM/r)
For (~circular) orbital velocity to be constant
the gravitational force of galaxies must drop off more slowly as 1/r not 1/r2.
Centrifugal force = mv2/r = gravitational force = Cm/r (; i.e., total dark mass M grows as Cr/G)

Hence: v2 = C : or v = sqrt (C)

(; i.e., UGC 12591's dark mass density is ~4 times that of the Milky Way.)

Re: APOD: UGC 12591: The Fastest Rotating... (2017 Mar 07)

by orin stepanek » Tue Mar 07, 2017 12:22 pm

I name this Galaxy (Zip)! :D

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