+ All Categories
Home > Documents > Escape Velocity

Escape Velocity

Date post: 31-Dec-2015
Category:
Upload: lilah-schroeder
View: 126 times
Download: 1 times
Share this document with a friend
Description:
Escape Velocity. Velocity needed to escape the gravitational pull of an object. 2GM R. v esc =. Escape velocity from Earth's surface is 11 km/sec. If Earth were crushed down to 1 cm size, escape velocity would be speed of light . Then nothing, including light, could escape Earth. - PowerPoint PPT Presentation
42
Escape Velocity Velocity needed to escape the gravitational pull of an object. v esc = 2GM R Escape velocity from Earth's surface is 11 km/sec. If Earth were crushed down to 1 cm size, escape velocity would be speed of light . Then nothing, including light, could escape Earth. This special radius, for a particular object, is called the Schwarzschild Radius , R S . R S M.
Transcript

Escape Velocity

Velocity needed to escape the gravitational pull of an object.

vesc

= 2GM R

Escape velocity from Earth's surface is 11 km/sec.

If Earth were crushed down to 1 cm size, escape velocity would be speed of light. Then nothing, including light, could escape Earth.

This special radius, for a particular object, is called the Schwarzschild Radius, R

S. R

S M.

Black Holes

If core with about 3 MSun

or more collapses, not even neutron

pressure can stop it (total mass of star about 25 MSun

).

Core collapses to a point, a "singularity".

Gravity is so strong that nothing can escape, not even light => black hole.

Schwarzschild radius for Earth is 1 cm. For a 3 MSun

object, it’s 9 km.

Event horizon: imaginary sphere around object with radius equal to Schwarzschild radius.

Event horizonSchwarzschild Radius

Anything crossing over to inside the event horizon, including light, is trapped. We can know nothing more about it after it does so.

Like a rubber sheet, but in three dimensions, curvature dictates how all objects, including light, move when close to a mass.

Black hole achieves this by severely curving space. According to Einstein's General Relativity, all masses curve space. Gravity and space curvature are equivalent.

Curvature at event horizon is so great that space "folds in on itself", i.e. anything crossing it is trapped.

Approaching a Black Hole:

QuickTime™ and aYUV420 codec decompressor

are needed to see this picture.

Circling a Black Hole at the Photon Sphere:

QuickTime™ and aYUV420 codec decompressor

are needed to see this picture.

Effects around Black Holes

1) Enormous tidal forces.

2) Gravitational redshift. Example, blue light emitted just outside event horizon may appear red to distant observer.

3) Time dilation. Clock just outside event horizon appears to run slow to a distant observer. At event horizon, clock appears to stop.

Black Holes have no Hair

Properties of a black hole:- Mass- Spin (angular momentum)- Charge (tends to be zero)

Black Holes can have impact on their environments

Do Black Holes Really Exist? Good Candidate: Cygnus X-1

- Binary system: 30 MSun

star with unseen companion.

- Binary orbit => companion > 7 MSun

.

- X-rays => million degree gas falling into black hole.

Clicker Question:

The escape velocity for the Earth is normally 11 km/s, what would the escape velocity be if you launched a rocket from a platform 21000 km above the surface of the Earth (4 Earth radii):

A: 22 km/s

B: 11 km/s

C: 6 km/s

D: 3 km/s

Clicker Question:

What is the escape velocity at the Event Horizon of a 100 solar mass black hole?

A: 300,000 km/s

B: 3,000,000 km/s

C: 30,000,000 km/s

D: 300,000,000 km/s

Supermassive (3 million solar mass) Black Hole at the Galactic Center

QuickTime™ and aYUV420 codec decompressor

are needed to see this picture.

The Milky Way Galaxy

a

b c

d

Artist's Conception

Take a Giant Step Outside the Milky Way

Example (not to scale)

Artist's Conception

Take a Giant Step Outside the Milky Way

Example (not to scale)

from above ("face-on")see disk and bulge

from the side ("edge-on")

Orion arm

Perseus arm

Cygnus arm

Carina arm

Sun

Another galaxy: NGC 4414. The Milky Way roughly resembles it.

M31

The Three Main Structural Components of the Milky Way

1. Disk

- 30,000 pc diameter (or 30 kpc)

- contains young and old stars, gas, dust. Has spiral structure

- vertical thickness roughly 100 pc - 2 kpc (depending on component. Most gas and dust in thinner layer, most stars in thicker layer)

2. Halo

- at least 30 kpc across

- contains globular clusters, old stars, little gas and dust, much "dark matter"

- roughly spherical

3. Bulge

- About 4 kpc across

- old stars, some gas, dust

- central black hole of 3 x 106 solar masses

- spherical

Shapley (1917) found that Sun was not at center of Milky Way

Shapley used distances to variable “RR Lyrae” stars (a kind of Horizontal Branch star) in Globular Clusters to determine that Sun was 16 kpc from center of Milky Way. Modern value 8 kpc.

Stellar Orbits

Halo: stars and globular clusters swarm around center of Milky Way. Very elliptical orbits with random orientations. They also cross the disk.

Bulge: similar to halo.

Disk: rotates.

Precise Distance to Galactic Center

QuickTime™ and aTIFF (Uncompressed) decompressor

are needed to see this picture.

Distance = 7.94 +/- 0.42 kpc

Eisenhauer et al. 2003Orbital motion 6.37 mas/yr

SgrA*

Clicker Question:

Where is our solar system located?

A: near the center of the Milky Way Galaxy in the bulge.

B: 4 kpc from the center of the Milky Way in the halo.

C: 8 kpc from the center of the Milky Way in the disk.

D: 20 kpc from the center of the Milky Way in the disk.

Clicker Question:

What lurks at the center of our galaxy?

A: A 3 million solar mass black hole.

B: A giant star cluster.

C: A 30 solar mass black hole.

D: Darth Vader

Rotation of the Disk

Sun moves at 225 km/sec around center. An orbit takes 240 million years.

Stars closer to center take less time to orbit. Stars further from center take longer.

The "rotation curve" of the Milky Way

=> rotation not rigid like a phonograph record or a merry-go-round. Rather, "differential rotation".

Over most of disk, rotation velocity is roughly constant.

Spiral Structure of Disk

Spiral arms best traced by:

Young stars and clustersEmission NebulaeHIMolecular Clouds(old stars to a lesser extent)

Disk not empty between arms, just less material there.

Problem: How do spiral arms survive?

Given differential rotation, arms should be stretched and smeared out after a few revolutions (Sun has made 20 already):

The Winding Dilemma

The spiral should end up like this:

Real structure of Milky Way (and other spiral galaxies) is more loosely wrapped.

Proposed solution:

Arms are not material moving together, but mark peak of a compressional wave circling the disk:

A Spiral Density Wave

Traffic-jam analogy:

Now replace cars by stars and gas clouds. The traffic jams are actually due to the stars' collective gravity. The higher gravity of the jams keeps stars in them for longer. Calculations and computer simulations show this situation can be maintained for a long time.

Traffic jam on a loop caused by merging

Molecular gas clouds pushed together in arms too => high density of clouds => high concentration of dust => dust lanes.

Also, squeezing of clouds initiates collapse within them => star formation. Bright young massive stars live and die in spiral arms. Emission nebulae mostly in spiral arms.

So arms always contain same types of objects, but individual objects come and go.

90% of Matter in Milky Way is Dark Matter

Gives off no detectable radiation. Evidence is from rotation curve:

RotationVelocity (AU/yr)

Solar System Rotation Curve: when almost all mass at center, velocity decreases with radius ("Keplerian")

R (AU)

10

5

1

1 10 20 30

Curve if Milky Way ended where visible matter pretty much runs out.

observed curve

Milky Way Rotation Curve

Not enough radiating matter at large R to explain rotation curve => "dark" matter!

Dark matter must be about 90% of the mass!

Mass of Milky Way

6 x 1011 solar masses within 40 kpc of center.

Composition unknown. Probably mostly exotic particles that don't interact with ordinary matter at all (except gravity). Some may be brown dwarfs, dead white dwarfs …

Most likely it's a dark halo surrounding the Milky Way.

Clicker Question:

How long does it take our solar system to orbit once around the Milky Way?

A: 1 year

B: 2 million years

C: 250 million years

D: 250 billion years (longer than the age of the universe)

Clicker Question:

What makes up most of the mass (90%) of the Milky Way Galaxy?

A: hydrogen gas

B: stars

C: dead stars (white dwarfs, neutron stars, and black holes)

D: we don’t know

Seeing into the center of the Milky Way

Seeing into the center of the Milky Way


Recommended