Caty Pilachowski IU Astronomy Mini-University 2014

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Caty Pilachowski IU Astronomy Mini-University 2014 Monster Black Holes

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Monster Black Holes. Caty Pilachowski IU Astronomy Mini-University 2014. What is a black h ole , anyway?. A black hole is…. …an object whose gravity is so intense that light cannot escape. How Big Are Black Holes?. A black hole’s size depends on its mass…. - PowerPoint PPT Presentation

Transcript of Caty Pilachowski IU Astronomy Mini-University 2014

Caty PilachowskiIU AstronomyMini-University 2014

Monster Black Holes

What is a black hole, anyway?

Black holes are not intuitive!

from xkcd (www.xkcd.com)

Black Hole

Historya

Escape Velocity

Isaac Newton, 1728A Treatise of the System of the World

A cannonball fired with enough velocity will orbit the EarthWith a high enough velocity, it will escape Earth entirely

Gravity Distance x Distance

Mass~

Dark Stars

• What happens if a star’s gravity is so strong that its escape velocity is faster than the speed of light?

• From the speed of light, Michell calculated that light could not escape from a star 500 x the Sun’s radius and the same density (125,000,000 solar masses!)

• The star would be dark!

John Michell, 18th century British scientist, Fellow of the Royal Society

Black Holes!

In the 1930s – Chandrasekhar, Oppenheimer, Snyder predict that massive stars can collapse into something denser – a black hole

J.A. Wheeler popularized the term “black hole”

Cygnus X-1: The FIRST Black Hole

Discovered in 1972A blue supergiant star orbits an invisible companionBright in x-raysHDE 226868, near Eta Cygni in Cygnus

Evidence for Black Holes

Effect of gravity on nearby objects – Mass!Accretion disks

Accretion disks emit x-rays as matter falls in But it’s hard to tell the difference between a black hole and a neutron star

Stellar Mass BHs

About 20 candidates known in the Milky Way Masses 4-12 times the mass of the Sun A few thousand light years away The galaxy contains many more yet to be discovered

The Monsters!

Sagittarius A*

1974 – A strong radio source was discovered in a radio- wavelength survey of the Galactic Center region

Sgr A* in X-rays

Strong X-ray emission from Sgr A* X-ray flares!

Sgr A* is not visible in visible or infrared light

But many stars surround Sgr A*

Stars Orbit Sgr A*

The orbits of stars around Sgr A* tell us the mass of the central object

The mass of Sgr A* is 4,000,000 times the mass of the Sun

Other galaxies have black holes, too!

The giant elliptical galaxy M87 contains a massive black hole 3.5 BILLION solar masses!

All large galaxies contain central black holes Hubble has

examined many large galaxies and found super-massive black holes at their centers

How do Monster black holes form?

Does the galaxy make the

black hole?

-or-Does the black

hole make the galaxy?

Black Hole First

Dense clump of primordial gas

becomes a black hole

The black hole’s gravity attracts more

gas into a disk

The gas forms stars to make a galaxy

Galaxies First: IA single massive

star forms

The star collapses to form a few hundred

solar mass black hole

The black hole eats gas, stars, and other black holes to grow

A cluster of massive stars forms in a baby galaxy

The cluster collapses under gravity to form a massive black hole

The black hole grows

Galaxies First: II

Black Holes Grow with Galaxies

Black holes accrete gasBlack holes eat starsWhen galaxies merge, their central black holes also merge

NGC 5033 hosts TWO super-massive black holes!

The black holes will eventually merge into one

Black holes in the center of galaxies will eventually merge together

Merging Black Holes

Black Hole Eats

a Star• A star in the galaxy

RX J1242-11 came too close to its black hole

• The star was tidally shredded

• Strong x-ray flare

Artist’s Conception

BH Mass ~ 100 million suns

Accreting Gas

The Doomed CloudSmall gas cloud discovered in 2011Moving almost directly toward Sgr A* black hole (yellow )Velocity ~ several million km/hour!About 3 Earth-masses of gas (but is a star inside?)

The Cloud in 2013Closest approach to Sgr A* in early 2014, about 2200 x the black hole’s radiusAs the cloud approaches Sgr A*, gravity “spagettifies” the cloud

2014 Observations The leading edge of the cloud has whipped

around Sgr A* at 10,000,000 km/hour!Computer Simulation

We’re still not sure what it is…– An isolated cloud– A “wind bubble”

around a star

The Cloud’s Future… Current observations suggest the cloud

contains a star… Computer Simulation

Black Holes Affect Galaxy Evolution

High energy jets from feeding black holes may regulate star formation, gas accretion, and

galaxy growth!

Only a fraction of accreted material ends up in the black hole – most is shot back out in a jet!

Courtesy A. Feild / STScI / NASA

Summary

The End