1 / 10

ASTRONOMY

ASTRONOMY. Chapter 30 Pulsars and Neutron Stars. Formation of a Neutron Star. In the iron core of a high-mass star: Iron nuclei break into He nuclei, protons, and neutrons Energy is carried out and the pressure drops The core collapses.

spence
Download Presentation

ASTRONOMY

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. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. ASTRONOMY Chapter 30 Pulsars and Neutron Stars

  2. Formation of a Neutron Star • In the iron core of a high-mass star: • Iron nuclei break into He nuclei, protons, and neutrons • Energy is carried out and the pressure drops • The core collapses. • Electrons are squeezed into the nucleus where they react with protons • Neutrons and neutrinos are formed • Neutrinos escape taking more energy

  3. Formation of a Neutron Star • After the explosion, the remaining mass can be from a few tenths M˳ to 3 M˳ • Core collapses until neutron degeneracy balances the gravity and the star becomes stable. • 1 teaspoon would weigh 1 billion tons on earth

  4. Comparison • A white dwarf packs the mass of the sun into the size of Earth. • A neutron star packs the mass of 2 suns into a 20 km diameter.

  5. Pulsars • Discovered in 1967 • Search has found that they are located in our galaxy • Periods range from thousandths of a second to four seconds. • Questions: • What are they? • What makes them tick”?

  6. The Lighthouse Model

  7. Crab Nebula “Proof” • A pulsar was discovered at the center of the Crab Nebula • Its period was found to be 0.033s • It is rotating at 30 revolutions per second • This speed would tear apart a white dwarf. • This pulsar radiates in all parts of the spectrum • Fastest known pulsar – the millisecond pulsar – spins at 642 rev/s

  8. Crab Nebula “Proof”

  9. Binary Pulsars • A pulsar in a binary system can exhibit a Doppler shift as it orbits its companion. • Relativity predicts gravitational waves from binary pulsars. • None have been detected so far.

  10. X-ray Binaries • Orbiting X-ray telescopes have detected some stars that pulse in x-rays • This is probably due to mass from the companion star being funneled to an accretion disk around the neutron star. • This gas heats up and emits x-rays.

More Related