Galaxy

A galaxy is a group of many stars, with gas, dust, and dark matter.^[1]^[2]^[3]^[4] The name 'galaxy' is taken from the Greek word galaxia meaning milky, a reference to our own galaxy, the Milky Way.

Gravity holds galaxies together against the general expansion of the universe.^[3] In effect, the expansion of the universe takes place between groups of galaxies, not inside those groups. Gravity holds the galaxy together. The same applies to groups and clusters of galaxies, such as our Local Group where the Milky Way is, and the Virgo Cluster, a collection of more than 1,000 (might even be 2,000) galaxies. The gravitation is produced by the matter and energy in a galaxy or group of galaxies. Everything in a galaxy moves around a centre of mass, which is also an effect of gravity.

There are various types of galaxies: elliptical, spiral and lenticular galaxies, which can all be with or without bars. There are also irregular galaxies.

All galaxies exist inside the universe. The observable Universe contains more than 2 trillion (10¹²) galaxies^[5] and, overall, as many as an estimated 1×10²⁴ stars^[6]^[7] (more stars than all the grains of sand on planet Earth).^[8]

Description

There are galaxies of different sizes and type. Typical galaxies range from dwarfs with as few as ten million^[3]^[9] (10⁷) stars up to giants with a hundred trillion^[3]^[10] (10¹⁴) stars, all orbiting the galaxy's center of mass. Galaxies may contain many multiple star systems, star clusters, and various interstellar clouds. The Sun is one of the stars in the Milky Way galaxy; the Solar System includes the Earth and all the other objects that orbit the Sun.

Star clusters are not galaxies, they are inside galaxies. Globular clusters are spherical-shaped star clusters which are part of the outer halo of the Milky Way. One of the largest (and oldest) known star clusters, Messier 15, has several million stars, packed closely together, with a black hole at its centre. The stars are too closely packed to get an accurate count, but it certainly has more stars than some of the smaller galaxies.

Within galaxy clusters, galaxies move relative to other galaxies. They can and do collide. When this happens, the stars generally move past each other, but gas clouds and dust interact, and can form a burst of new stars. Gravity pulls both galaxies into somewhat new shapes, forming bars, rings or tail-like structures.

NGC 2997, a spiral galaxy in the constellation Antila, produces new stars at a rate of 1 or 2 stars per year.

Many galaxies continue to form new generations of stars. The Milky Way, and all spiral shaped galaxies like it (see right side image of NGC 2997), produce new stars at a rate of one or two stars per year. This star formation happens in the vast interstellar clouds that account for about 1% to 10% of the mass of these galaxies. Globular star clusters, on the other hand, are not currently forming stars because this activity happened billions of years ago and then stopped once all of the gas and dust clouds were used up.

In the astronomical literature, the word 'Galaxy' with a capital G is used for our galaxy, the Milky Way. The billions of other galaxies are written as 'galaxy' with a lowercase g. The term Milky Way first came out in the English language in a poem by Chaucer.

"See yonder, lo, the Galaxyë
Which men clepeth the Milky Wey,
For hit is whyt".^[3]^[11]

When William Herschel wrote his catalogue of deep sky objects, he used the name spiral nebula for objects like the Andromeda Galaxy. 200 years later astronomers discovered that they are made of stars as the Milky Way is, so the term 'nebula' is now only used for diffuse structures in a galaxy.

Types

There are two main kinds of galaxies, spiral galaxy and elliptical galaxy. They are classified according to the Hubble Sequence.

Spiral galaxy

A spiral galaxy is a galaxy that has a spiral shape. Most of the galaxies in the universe observed by astronomers are spiral galaxies (about 77%).^[12]

They are divided into two :

Barred spiral galaxy (classified as "SB")
Unbarred spiral galaxy (classified as "SA")

NGC 1300 and NGC 1672 are examples of barred spiral galaxies. The Whirlpool galaxy and Messier 81 are examples of unbarred spiral galaxies.

The identifying characteristics of a spiral galaxy are disk-shaped rotating, spiral arms, and a bulge in the galactic core. The spiral arms are where new hot stars are born. "Bulge" in the galactic core has old stars. This feature is common to the most spiral galaxies.

Elliptical galaxy

An elliptical galaxy is a galaxy that has a ellipsoid (3D of ellipse) shape. This type of galaxy are dominant in universe, especially in galaxy clusters. The shape ranges from circle, ellipse, and cigar-shaped. In Hubble Sequence, this shape can be represented as class :

E0 (circle-shape)
E53 (ellipse-shape)
E7 (cigar-shaped)

Elliptical galaxies have a large range in size. The giant elliptical galaxy can be over a more 1 million light years and the smallest (know as "dwarf elliptical galaxy") are less than one-tenth the size of Milky Way^[13] The effective radius defines the area from which half its light comes. The mass of elliptical galaxy is also large. A giant elliptical galaxy can have mass of 10¹³ (many trillions) of solar masses.^[14]

Other kinds of galaxies

A lenticular galaxy is a galaxy seen as a disc shape. The shape of a lenticular galaxy is between spiral galaxy and elliptical galaxy. The shape can be known by looking at the bulge of the galactic center. If the bulge is very bright, it is a spiral galaxy.^[15]

Related pages

List of galaxies
List of nearest galaxies
Most distant things
Local Group
IC 1101: the largest known galaxy, with about 100 trillion stars.^[16]^[17]
Milky Way
Andromeda galaxy

References

↑ Sparke L.S. & Gallagher III J.S. 2000. Galaxies in the Universe: an introduction. Cambridge: Cambridge University Press. ISBN 0521671868.
↑ Hupp E; Roy S. & Watzke M. 2006.[1] Archived 2020-03-28 at the Wayback Machine
↑ ^3.0 ^3.1 ^3.2 ^3.3 ^3.4 Cox, Brian; Cohen, Andrew (2011). Wonders of the Universe. HarperCollins. p. 24. ISBN 9780007395828.
↑ "What is a Galaxy? | NASA Space Place – NASA Science for Kids".
↑ Fountain, Henry (17 October 2016). "Two Trillion Galaxies, at the Very Least". The New York Times. Retrieved 17 October 2016.
↑ "How many stars are there in the Universe?". European Space Agency. 2019. Retrieved 21 September 2019.
↑ Marov, Mikhail Ya. (2015). "The Structure of the Universe". The Fundamentals of Modern Astrophysics. pp. 279–294. doi:10.1007/978-1-4614-8730-2_10. ISBN 978-1-4614-8729-6.
↑ Mackie, Glen (1 February 2002). "To see the Universe in a Grain of Taranaki Sand". w:Centre for Astrophysics and Supercomputing. Retrieved 28 January 2017.
↑ ESO 2000: [2] Archived 2012-07-29^{[Timestamp length]} at Archive.today
↑ Wilford, John Noble 1990. "Sighting of largest galaxy hints at clues on the clustering of matter". New York Times. Retrieved 2010-05-06^{[permanent dead link]}
↑ Geoffrey Chaucer. The House of Fame, ~1380."Online Etymology Dictionary". Retrieved 2007-01-03.
↑ "Spiral Galaxy Facts & Definition". Space.com. Retrieved 2018-01-28.
↑ "Elliptical Galaxies". cas.sdss.org. Retrieved 2018-01-28.
↑ "Elliptical Galaxy | COSMOS". astronomy.swin.edu.au. Retrieved 2018-01-28.
↑ "Lenticular Galaxies". cas.sdss.org. Retrieved 2018-01-30.
↑ https://arxiv.org/PS_cache/astro-ph/pdf/0209/0209205v2.pdf
↑ Uson, Juan M. (October 1990). "The central galaxy in Abell 2029 – an old supergiant". Science. 250 (4980): 539–540. Bibcode:1990Sci...250..539U. doi:10.1126/science.250.4980.539. ISSN 0036-8075. PMID 17751483. S2CID 23362384.

Other websites

Galaxies, SEDS Messier pages Archived 2011-08-12 at the Wayback Machine
An Atlas of The Universe
Galaxies — Information and amateur observations
The oldest galaxy yet found Archived 2006-04-11 at the Wayback Machine
Galaxies — discussed on BBC Radio 4's "In Our Time" programme
Galaxy classification project, harnessing the power of the internet and the human brain
How many galaxies are in our universe? Archived 2015-08-21 at the Wayback Machine

[sparke-1] Sparke L.S. & Gallagher III J.S. 2000. Galaxies in the Universe: an introduction. Cambridge: Cambridge University Press. ISBN 0521671868.

[nasa-2] Hupp E; Roy S. & Watzke M. 2006.[1] Archived 2020-03-28 at the Wayback Machine

[cox1-3] 3.0 ^3.1 ^3.2 ^3.3 ^3.4 Cox, Brian; Cohen, Andrew (2011). Wonders of the Universe. HarperCollins. p. 24. ISBN 9780007395828.

[4] "What is a Galaxy? | NASA Space Place – NASA Science for Kids".

[NYT-20161017-5] Fountain, Henry (17 October 2016). "Two Trillion Galaxies, at the Very Least". The New York Times. Retrieved 17 October 2016.

[ESA-2019-6] "How many stars are there in the Universe?". European Space Agency. 2019. Retrieved 21 September 2019.

[7] Marov, Mikhail Ya. (2015). "The Structure of the Universe". The Fundamentals of Modern Astrophysics. pp. 279–294. doi:10.1007/978-1-4614-8730-2_10. ISBN 978-1-4614-8729-6.

[SU-20020201-8] Mackie, Glen (1 February 2002). "To see the Universe in a Grain of Taranaki Sand". w:Centre for Astrophysics and Supercomputing. Retrieved 28 January 2017.

[eso-9] ESO 2000: [2] Archived 2012-07-29^{[Timestamp length]} at Archive.today

[Wilford-10] Wilford, John Noble 1990. "Sighting of largest galaxy hints at clues on the clustering of matter". New York Times. Retrieved 2010-05-06^{[permanent dead link]}

[11] Geoffrey Chaucer. The House of Fame, ~1380."Online Etymology Dictionary". Retrieved 2007-01-03.

[12] "Spiral Galaxy Facts & Definition". Space.com. Retrieved 2018-01-28.

[13] "Elliptical Galaxies". cas.sdss.org. Retrieved 2018-01-28.

[14] "Elliptical Galaxy | COSMOS". astronomy.swin.edu.au. Retrieved 2018-01-28.

[15] "Lenticular Galaxies". cas.sdss.org. Retrieved 2018-01-30.

[16] ttps://arxiv.org/PS_cache/astro-ph/pdf/0209/0209205v2.pdf

[science250_4980_539-17] Uson, Juan M. (October 1990). "The central galaxy in Abell 2029 – an old supergiant". Science. 250 (4980): 539–540. Bibcode:1990Sci...250..539U. doi:10.1126/science.250.4980.539. ISSN 0036-8075. PMID 17751483. S2CID 23362384.

[1]

[2]

[3]

[4]

[5]

[6]

[7]

[8]

[9]

[10]

[11]

[12]

[13]

[14]

[15]

[16]

[17]