A galaxy is a gravitationally bound system of stars, stellar remnants, interstellar gas, dust, and dark matter. The word galaxy is derived from the Greek galaxias (γαλαξίας), literally "milky", a reference to the Milky Way. Galaxies range in size from dwarfs with just a few hundred million (108) stars to giants with one hundred trillion (1014) stars, each orbiting its galaxy's center of mass.
Galaxies are categorized according to their visual morphology as elliptical, spiral, or irregular. Many galaxies are thought to have supermassive black holes at their centers. The Milky Way's central black hole, known as Sagittarius A*, has a mass four million times greater than the Sun. As of March 2016, GN-z11 is the oldest and most distant galaxy observed. It has a comoving distance of 32 billion light-years from Earth, and is seen as it existed just 400 million years after the Big Bang.
In 2021, data from NASA's New Horizons space probe was used to revise the previous estimate of 2 trillion galaxies down to roughly 200 billion galaxies (2×1011). This followed a 2016 estimate that there were two trillion (2×1012) or more galaxies in the observable universe, overall, as many as an estimated 1×1024 stars (more stars than all the grains of sand on planet Earth). Most of the galaxies are 1,000 to 100,000 parsecs in diameter (approximately 3,000 to 300,000 light years) and are separated by distances on the order of millions of parsecs (or megaparsecs). For comparison, the Milky Way has a diameter of at least 30,000 parsecs (100,000 ly) and is separated from the Andromeda Galaxy, its nearest large neighbor, by 780,000 parsecs (2.5 million ly.)
The space between galaxies is filled with a tenuous gas (the intergalactic medium) having an average density of less than one atom per cubic meter. The majority of galaxies are gravitationally organized into groups, clusters, and superclusters. The Milky Way is part of the Local Group, which it dominates along with Andromeda Galaxy. The group is part of the Virgo Supercluster. At the largest scale, these associations are generally arranged into sheets and filaments surrounded by immense voids. Both the Local Group and the Virgo Supercluster are contained in a much larger cosmic structure named Laniakea.
When a photo of a nearly edge on galaxy, say Andromeda, is taken. Why are the stars on the far side of the galaxy so clear? The light from those stars took an additional 220,000 years to reach us. Those stars have moved quite a lot from their positions since the light from the foreground stars...
How do we know if galaxies are gravitationally bound?
I'm guessing it obviously has something to do with the mass of each galaxy in the cluster, but is there an equation that is used to determine when they are bound to each other? Is there some kind of measurement made regarding the velocity...
Because of Zwicky'f findings back in 1933 on the Coma Cluster rotational curves there is something I was wondering about with regard to this cluster. Are the galaxies orbiting in generally the same direction? (like a spiral galaxy) or in completely random directions like an Elliptical, or...
Hi all. Awesome site! Just wondering if anyone can answer my question:
If the Sextans galaxies are inside the group's zero velocity surface, why is there uncertainty over whether they're part of the group?
Homework Statement
Given that there are 10-2 Ellipticals per Mpc3 and my garden telescope can reach to 14 mag. How large an area of sky would I need to survey to find 100 Elliptical galaxies ? (assume the typical absolute magnitude for an Elliptical galaxy is -21 mag).Homework Equations...
There are galaxies that are so far away that metric expansion causes them to have a co-moving recessional velocity that exceeds the speed of light. However, those galaxies are also so far away that the time it took the light to reach us was itself billions of years in the passage of its journey...
I'm learning about imaging techniques and projection/deprojection for images of galaxies at university. The big issue there is the fact that an image is a 2D representation of a 3D object (for example a galaxy), and to learn some properties of the object you need the 3D structure. What happens...
If, as suspected, the Andromeda galaxy "colides" with our own sometime in the far future, would the gravitational forces from passing stars have effect on our solar system?
In accelerated models the interaction looks quite violent, but how would it be in our "uncharted backwaters of the...
Recently I have studied that from the rotation curve of spiral galaxies, the nearly constt. behaviour of velocity of the stars situated far away from the central core suggests mass(r) ~ r ,rather than 1/√r as expected.
Are there any other theory which proves the existence of dark energy ??
Ive been lying in bed this morning wondering about the unusual motion of stars in galaxies.The whole disc rotating like a record at the same speed.Does it mean that the effects of gravity are simply altered by speed?Much like a wonder-wall.So the faster the speed of the object,or stars,the less...
I am trying to estimate the distance of closest galaxy neighbor knowing the expression of number of neighbors into a volume ##\text{d}V##, the mean density ##n_\text{gal}## and the correlation function, i.e with this expression :
##\text{d}N=n_{\text{gal}}\,\text{d}V\,(1+\xi(r))##
with...
Hello,
I am asked to give the formal expression of the total number density of galaxies and explain why is this expression problematic in practice?
From what I saw from my research and into my lectures, I have found the follwing relation which gives the number of galaxies ##N## with mass ##(m...
https://Earth'sky.org/space/new-map-confirms-four-milky-way-arms
...four spiral arms. The arms are where most stars in the galaxy are born. They contain most of the galaxy’s gas and dust, the raw ingredients for new stars.
Two of the arms, called Perseus and Scutum-Centaurus, seem to be more...
Homework Statement
I have the following questions as homeworks and I would like to get help.
Here's some informations given to help us to answer :
Photometry :
U=11.60
B=11.16
V=10.20
Redshift : z= 0.00780
Central velocity dispersion : ##\sigma_{v}## = 210 km/s
Introduction :
The...
Homework Statement
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I have the following questions as homeworks and I would like to get help.
Question 1) Give the formal expression of the total number density of galaxies. Why is this expressoin problematic in practice?
Question 2) In practice one uses a numerical value for the number...
1. Homework Statement
The Initial Mass Function (IMF) defines the distribution of stellar masses created in a star-forming event. The probability P(m)dm of forming a star with a mass between m and m + dm is given by
P(m)dm = km−α dm
where α is the exponent of the power law and k is a constant...
Sorry for a basic question but I keep reading conflicting information on this.
So, I know that there are distant galaxies that are being carried by the expansion of space faster than the speed of light relative to us. But were these objects actually receding >c when the light we are seeing was...
If I am given the variable of time (observed), and diameter is it possible to measure the distance of a galaxy? Or do I need more variables?
Just trying to figure out the most simple way to go about doing something like that.
I'm not sure where to post this, so I figured Academic Guidance is the best fit for the question.
Here is their main page:
http://www.mdpi.com/journal/galaxiesHere is a paper published in it on the Sagnac effect in the context of relativity...
Could it be imagined that due to a particular stars' distribution in a galaxy the gravitational force felt would be like $$f(\vec{e}_r)/r^{\alpha}$$ where $$\alpha\neq 2$$ but near 2 and f a non spherically symmetric function (like a comet around a flat galaxy) ?
I'm trying to understand the Schechter function, I read on Wikipedia that the L star term in the function is the 'characteristic galaxy luminosity where the power-law form of the function cuts off'. What does this mean exactly?
I've been doing some spectrum extractions in IRAF, stellar and galactic, and I was wondering if anyone here had any ideas on how to tell if the extraction/calibration/etc went well? I have a bunch of finished projects but I'm not sure about how to tell if they're any good or not. Let me know if...
Hello, I'm new at the forum. I'm a science-fiction writer. My question then concerns an imaginary, fictional situation. I'll try to be brief but it's not easy to explain:
Let's imagine that a character who lives on Earth is strongly attracted by the gravitational force of some other celestial...
Is I understand it Hubble's law states that V = Hd = dx/dt
Solving this differential equation, I got d = kexp(HT) where k is an arbitrary constant.
This implies d²x/dt² = Hv = H²d and dⁿx/dtⁿ = Hⁿd.
However (at least for me), finding the value of k is a problem, for 1, it must vary from galaxy...
Spiral galaxies of course rotate around one axis perpendicular to the plane, but has anyone measured if any spiral galaxies are also rotating about an axis through the plane or about any other axis?
I'd just like to comment if I may - The virial thereom is not applicable to clusters of galaxies as the numbers of member galaxies in the majority of clusters (as opposed to superclusters) are too small for the virial thereom to effectively calculate the cluster mass. There is a short article to...
I recently looked at
https://www.physicsforums.com/threads/will-temperature-go-down.104791/
and then looked at the link
http://math.ucr.edu/home/baez/end.html .
My question is related to a quote from this link.
(It may seem odd that first the galaxies form by gravitational attraction of matter...
From deep galaxy counts, it is estimated that there are about 40 billion galaxies in the observable universe (not including probable multitudes of dwarf galaxies too faint to observe). Assuming that the mean age of these galaxies is 10 Gyr, and that each one goes through an AGN episode once...
When discussing about galactic 'collisions' and mergers, such as the predicted future encounter between the Milky Way and Andromeda, it is often said that actual collisions among stars are extremely unlikely, it's just that the mutual gravitational influence of both galaxies on each other will...
The planets rotate around our sun faster and faster the closer they are.The Suns rotate around a black hole in a galaxy as if they were a record on a record player.Gravitational laws as we understand them don't seem to apply.Is it possible that a black holes gravitational pull not only freezes...
https://www.sciencedaily.com/releases/2017/10/171026103110.htm
Astronomers have discovered that the brightest galaxies within galaxy clusters 'wobble' relative to the cluster's center of mass. This unexpected result is inconsistent with predictions made by the current standard model of dark...
This may sound like a noob question, even more if it's asked by a undergraduate physics student, but here it's:
How do we know about the existence of 100 billion galaxies out there (even that it's an average value)? I mean, how do we know about these exact number? Why not, say, 200 billion or...
I have as advised done some catching up on basic cosmology, looking at various discussion and lectures on the nature of the universe.
Something that has always played on my mind, is that i remember reading and watching a documentary about the potential to achieve the velocity of light.
It was...
Hi all,my second question is this.Why don't galaxies obey gravity? In our solar system the closer to our sun the planet is the faster it rotates.So the outer planet takes much longer for a solar year.
When we look at galaxies this gravitational law doesn't apply.The outside stars spin at the...
Can someone point me to a resource that describes, or describe, how the orbital speed of stars within galaxies are observed and measured?
I'm struggling with how these values can be attained with any confidence in their accuracy.
Thanks :)
How far are we from being capable of estimating the number of planets in other galaxies? At least, in any of the nearby galaxies that are already known to us?
Would this require state-of-art equipments?
I’m joining this forum just to see if someone can answer this question in a way that I can understand, because it’s driving me nuts.
I read about galaxies observed by the Hubble Space Telescope that were formed “shortly” after the Big Bang. For example, the article may say that they are 12...
I thought that z= 7.5 was the maximum for galaxies to form after re ionization but this paper puts it at z=8.38,
can galaxies have formed this early?
arXiv:1703.02039 [pdf, other]
Dust in the reionization era: ALMA observations of a z=8.38 Galaxy
Nicolas Laporte, Richard S. Ellis, Frederic...
Reading this article it states that ram pressure can kill off star formation, can you tell me please what ram pressure is?
https://www.sciencedaily.com/releases/2017/01/170116160620.htm
Hi
I have a question which is about the lyman break drop-out technique for identifying high red shift galaxies. I am basically trying to understand how the technique works.
My current understanding is that the drop-out technique makes use of the fact that very high red shift galaxies...
My question is following:
Is there another Galaxy in the Universe that has a relative speed to the Milky Way of 0.999c (near of light speed)? The implication of that is that our life 'observed' by extraterrestrial beings in that Galaxy might be millions of years, an eternity! This is because of...
The observed galaxy rotation curve does not match the theoretical curve derived from the model that galaxies are in steady state circular motion (SSCM). The presence of dark matter would bring the SSCM curve up to the observed curve. But what observation demonstrates that galaxies are in SSCM in...