Galactic evolution
Sponsored Links
This presentation is the property of its rightful owner.
1 / 48

Galactic Evolution PowerPoint PPT Presentation


  • 101 Views
  • Uploaded on
  • Presentation posted in: General

Galactic Evolution. AST 112. Four Types of Galaxies. Spiral Elliptical Lenticular Irregular Why?. Hubble Sequence. The Hubble Sequence suggests a path of evolution for galaxies. The Hubble Sequence is ABSOLUTELY WRONG! (But good first try.). Formation of Galaxies.

Download Presentation

Galactic Evolution

An Image/Link below is provided (as is) to download presentation

Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author.While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server.


- - - - - - - - - - - - - - - - - - - - - - - - - - E N D - - - - - - - - - - - - - - - - - - - - - - - - - -

Presentation Transcript


Galactic Evolution

AST 112


Four Types of Galaxies

  • Spiral

  • Elliptical

  • Lenticular

  • Irregular

    Why?


Hubble Sequence

The Hubble Sequence suggests a path of evolution for galaxies.


The Hubble Sequence isABSOLUTELY WRONG!(But good first try.)


Formation of Galaxies

  • Galaxies begin as a protogalactic cloud

  • We will assume a “top-down” theory of galaxy formation

    • Large, simultaneous collapse


Elliptical vs. Spiral

What determines whether a galaxy willbecome a spiral or an elliptical?


Spiral or Elliptical?

  • Does it form as a spiral or elliptical?

    • Depends on protogalactic cloud conditions

  • Does it ever transform from one to the other?

    • Depends on interactions with other galaxies


Formation of Galaxies

  • Keep this in mind:

    • Spiral galaxies have gas-rich disks

    • Ellipticals do not


Protogalactic Conditions

  • Protogalactic spin:

    • If it’s spinning, it will flatten

  • Protogalactic density:

    • Higher density: more rapid star formation, most stars formed during collapse

      • Less material left over

    • Lower density: fewer stars created during collapse

      • More material left over


Spirals: Halo, Bulge and Disk

  • Protogalactic cloud contracted

    • Formed massive 1st generation stars

  • Spin increases as cloud collapses

  • Protogalaxy flattens as spin increases

  • Gas contracts faster than the stars

    • Spirals start with low density

    • Lower rate of star formation during collapse

  • First generation stars exploded in a few million years as the protogalaxy was collapsing

    • Slowed collapse


Spirals: Halo, Bulge and Disk

  • What do we have?

    • A spherical distribution of stars left over from initial collapse and star formation

      • Bulge and Halo

    • A disk of gas and dust that was “preserved” due to lower rates of star formation


Spirals: Halo, Bulge and Disk

  • What causes star formation to ramp up in the disk?

  • Why is the bulge yellow?


Ellipticals

  • Giant ellipticals across the Universe:

    • Nearly devoid of blue and white stars

    • Very red; entire galaxy is old

  • Suggests all stars formed at once

    • Nothing left to make a disk out of

    • Star formation ceased shortly after the galaxy formed


Lenticulars: “Anemic Spirals”?

  • Lenticular galaxies could be former spirals that have lost their cold gas

    • Used up

    • Lost via collision


Globular Clusters

  • Globular clusters live in the halos of large galaxies

    • Milky Way: 150+

    • Andromeda: 500+

    • M87: 13,000+

  • Some may have intermediate-sized black holes at their center


Globular Clusters

  • Two possible origins for globular clusters:

    • As the protogalactic disk collapsed, larger fragments formed globular clusters

      OR

    • These are the bulges of much smaller galaxies that were absorbed into larger galaxies


Galactic Collisions / Mergers

  • If the approaching galaxies are moving fast, they may collide and keep going

  • Otherwise, they may collide repeatedly and merge


Galactic Collisions

  • The Whirlpool Galaxy (Messier 51) is a classic example of colliding galaxies


A Galactic Merger


Another galacticmerger.


A Galactic Collision


Cartwheel Galaxy


Galactic Collisions

  • Galactic collisions play a major role in galactic evolution

  • “Rarely evolve in perfect isolation”

  • From the book:

    • If our galaxy is a grapefruit, Andromeda is another grapefruit 3 meters away (and several are closer)


Galactic Collisions

  • Collisions occur over hundreds of millions of years

  • Stars don’t collide much

  • Gas and dust DO collide

  • Triggers LOTS of star formation (100/yr)


Galactic Collisions

  • Tidal forces tear the disks apart

  • Orbits get randomized

  • Trails of stars form after collisions

  • Supernovae and winds blow gas away


Galactic Collisions

Collisions tend to disrupt orbits and destroy disks in spiral galaxies.Regardless of what type of galaxy you start with,what type of galaxy likely results from multiplelarge-scale collisions?


Galactic Collisions

What’s goingon here?


Galactic Collisions

  • M81 / M82 have been duking it out for millions of years

  • M82 is undergoing starburst because of this


Sagittarius Dwarf Galaxy

  • The Milky Way is colliding with the Sagittarius Dwarf Galaxy!

  • 80,000 LY away (behind the bulge)


Sagittarius Dwarf Galaxy


Collision With Andromeda

  • The Milky Way will merge with Andromeda in 3 to 5 billion years

    • Star collisions won’t hurt us… gas collision could

    • We could get flung out of the galaxy


Galactic Collisions: Simulation


Observing Galaxies Through Time

  • Galaxies take billions of years to evolve…

    • So how can we hope to study it?

  • Recall that light takes time to travel from one location to another

    • It’s fast. But the distances involved are HUGE.

  • We are able to study galactic evolution because our large telescopes can look far away

    • And therefore into the distant past

    • We can see back to 13 billion years

    • Almost back to the beginning of the universe (13.7 billion years old)


Observing Galaxies Through Time

  • The circled galaxy is seen when it was 800 million years old


Observing Galaxies Through Time


Observing Galaxies Through Time

  • Due to the expansion of the Universe, collisions between galaxies used to be more frequent


Observing Galaxies Through Time

  • Newly formed galaxies show huge starburst activity

  • They are warped, bright, chaotic

    • Little to no structure


Quasars

  • Distant, luminous objects that look like stars

  • These are galaxies that have an active galactic nucleus

    • An SMBH that is actively devouring material

    • Forms a very hot accretion disk

  • Most of them more than halfway to cosmological horizon


Late Bloomer

  • Zwicky 18 resembles newly formed galaxies that we observe with Hubble

  • A “late bloomer”?


Life in the Cluster

  • What kind of galaxy results from a merger?

  • Rich clusters: few or lots of mergers?

  • So what kind of galaxy do we find many of in large clusters?


Life in the Cluster

  • Messier 87: The showpiece of dense-cluster evolution!

  • Gigantic.

  • Elliptical.


Life in the Cluster

Clusters (50-1000 galaxies) do contain spirals but they tend to live on the edges.

Galaxy Groups(5-50 galaxies)are often dominated by spirals.


Life in the Cluster

  • Central Dominant Galaxy of a cluster is usually a Giant Elliptical

  • IT ATE THE OTHER GALAXIES.

  • Most massive galaxies in the universe.

M87


Life in the Cluster

  • Another way for a spiral to become an elliptical:

    • Clusters have lots of hot gas

    • Spiral can pass through it. Stars keep going, gas gets left behind

    • Becomes elliptical if disk hasn’t formed

    • Could become lenticular if disk has formed


Summary

  • A galaxy will likely become elliptical if:

    • It had no rotation as it formed

    • It is dense (uses up all of the star stuff on initial collapse)

    • It undergoes numerous large collisions

  • A galaxy will likely become a spiral if:

    • It is rotating

    • It is less dense (so that it doesn’t use up all of the star stuff during the initial collapse)

    • It doesn’t suffer too many large collisions


Summary

  • Young galaxies are usually irregular starburst galaxies

  • Earlier, quasars (galaxies with AGN) were more common


Summary

  • Galaxy groups tend to be dominated by spiral galaxies

  • Galaxy clusters tend to be dominated by elliptical galaxies

  • Galaxies at the center of large clusters are giant ellipticals

    • Because of many, many collisions


Down to Earth

Here we are in a large spiral galaxy onthe outer edge of the Virgo Supercluster.We orbit a stable, long-lived star.Make sense?


  • Login