Pulsars are just a kind of neutron stars so it’s essential to get a grip of these first. The...

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PULSARS : STARS WITH A PULSE

Transcript of Pulsars are just a kind of neutron stars so it’s essential to get a grip of these first. The...

Page 1: Pulsars are just a kind of neutron stars so it’s essential to get a grip of these first.  The stars that come into being at the end of a massive.

PULSARS : STARS WITH A PULSE

Page 2: Pulsars are just a kind of neutron stars so it’s essential to get a grip of these first.  The stars that come into being at the end of a massive.

OVERVIEW What are neutron stars? A day on a neutron star. Pulsars. Why do pulsars have

intense magnetic field? To what good are pulsars

to us.

Page 3: Pulsars are just a kind of neutron stars so it’s essential to get a grip of these first.  The stars that come into being at the end of a massive.

NEUTRON STARS

Pulsars are just a kind of neutron stars so it’s essential to get a grip of these first.

The stars that come into being at the end of a massive star’s lifetime are called neutron stars.

When these massive stars have finished burning their nuclear fuel, they undergo a supernova explosion.

The event of formation of neutron stars is called core-collapse supernova’.

The central region of the star collapses so much that even electron, proton combine to form neutron and hence the name neutron star.

Page 4: Pulsars are just a kind of neutron stars so it’s essential to get a grip of these first.  The stars that come into being at the end of a massive.

A DAY ON NEUTRON STAR

The size of neutron star as compared to the Earth and a White Dwarf

Page 5: Pulsars are just a kind of neutron stars so it’s essential to get a grip of these first.  The stars that come into being at the end of a massive.

+ Small diameter + High mass=Super

High Density. Density of an average neutron star

would be around 5 x 1017 kg/m3 . Rotates about 40,000 times a minute. Crust is about 1 km thick but 100 billion

times stronger than steel. Has a very tiny atmosphere(made

mostly of iron 56 and lighter elements) . The surface is about 1 million degrees

Celsius. They have an escape velocity of about

33% the speed of light.

Page 6: Pulsars are just a kind of neutron stars so it’s essential to get a grip of these first.  The stars that come into being at the end of a massive.

PULSARS Discovered by Jocelyn Bell in 1967. She observed a pulsar whose pulsations lasted for

about 0.04 seconds and were 1.3373 seconds apart, called pulsar period.

It was initially named LGM-1, for Little Green Men . Bell and her instructor assumed it as a sign of

extraterrestrial life. Later Thomas Gold recognized that pulsars were

rotating neutron stars. So pulsar is a kind of neutron star that emits beams

of radiation that sweep through Earth’s line of sight. A special phenomenon called lighthouse effect is

observed. All pulsars are neutron stars, not all neutron stars

are pulsars!

Page 7: Pulsars are just a kind of neutron stars so it’s essential to get a grip of these first.  The stars that come into being at the end of a massive.

A diagram of pulsar showing its rotation and magnetic axis

Page 8: Pulsars are just a kind of neutron stars so it’s essential to get a grip of these first.  The stars that come into being at the end of a massive.

When normal stars collapse into pulsars(neutron stars) their magnetic fields also compress and become enormously intense as much as a trillion times Earth’s magnetic field.

Pulsars spin fast for the same reason ice skaters pull in their arms to spin, following conservation of angular momentum.

The Vela Pulsar

Page 9: Pulsars are just a kind of neutron stars so it’s essential to get a grip of these first.  The stars that come into being at the end of a massive.

APPLICATIONS OF PULSARS

In Map reading.

As precise clocks.

As gravitational wave detectors.

Relative position of the Sun to the centre of the galaxy and 14

pulsars

Page 10: Pulsars are just a kind of neutron stars so it’s essential to get a grip of these first.  The stars that come into being at the end of a massive.

REFERENCES For the Love of Physics… by

Walter Lewin. Einstein for Everyone… by

Robert L. Piccioni. http://www.fromquarkstoquasa

rs.com http://imagine.gfsc.nasa.gov/do

cs/science/know_|1/pulsars.html