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Quasars.

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Presentation on theme: "Quasars."— Presentation transcript:

1 Quasars

2 Distant Light Some objects in deep space are visible, small, and have large redshifts. Very distant by Hubble’s law Billions of light years away larger wavelength nearby galaxy distant object

3 Quasi-Stellar Objects
These objects were first observed as intense radio sources. Bright, but star-sized They were named quasi-stellar radio sources—quasars. Quasars emit in all parts of the electromagnetic spectrum. 100 times Andromeda Brighter flares 3C279, a quasar photographed in gamma rays

4 Distant Past Looking at a faraway object is like looking back in time.
If a quasar is 4 billion ly away, we are seeing the universe 4 billion years ago. Early life of galaxies Andromeda — 2 million years ago Earth PKS 1127 — 4 billion years ago

5 Disk and Jets Radio measurements show two giant jets of radiating gas.
Visible light and x-rays see a disk of gas, dust and stars. Most intense at center

6 Jet Formation Quasars form from a supermassive black hole.
The black hole draws stars and dust to its center. The material is accelerated to high velocity and ejected out either side.

7 Active Nuclei Some nearby galaxies show jets of radiating gas.
Start at galactic black hole Active from dust falling in Quasars fade to active galaxies as dust decreases.

8 Radio Galaxies Visible elliptical galaxies have black holes in their center. The jets are only seen with radio telescopes. Radio galaxies Active spiral galaxies are called Seyfert galaxies.

9 Colliding Black Holes The Chandra X-ray Observatory has observed two supermassive black holes in the same galaxy. NGC 6240: 400 Mly When the holes collide in a few hundred million years, the gravity waves will be felt on earth.


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