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Gamma-Ray
Bursts
Salwa Shaglel
Outline
2
first
What Are Gamma-Ray
Bursts ?
- Gamma-Rays
- How Can We Detect
Gamma Rays ?
GRBs Energy
second
GRBs Types
third
Effects of GRBs on Earth
- Are They Going to Kill us ?
- Did Any GRBs Hit the Earth ?
last
August 17th,2017 GRB
and Gravitational
Wave Detection
last
1- What Are Gamma-Ray Bursts ?
3
● The brightest electromagnetic
events in the universe.
● Extremely energetic explosions
observed in distant galaxies.
● Lasts from ten milliseconds to
several hours.
● Followed by slowly fading
emission at longer wavelengths
created by collisions between
the burst ejecta and interstellar
gas ( Afterglow ).
4
1.1 - Gamma-Rays
● Electromagnetic radiation
● Carry very high energy.
● A single gamma-ray photon is more
energetic than a million visible photons
combined !
● DANGEROUS ??
Form of Ionizing
Radiation, it can
break apart atomic
bonds.
5
E=hf
1.2 - How Can We Detect
Gamma-Rays ?
● Our Atmosphere (Ozone Layer O3
) blocks
𝛾-rays.
● 𝛾-rays should be detected by spacecrafts.
● The discovery of 𝛾-ray bursts was during
the cold war, when the USA sent up spy
satellites to detect 𝛾-rays from soviet
nuclear tests!.
6
7
Distribution is
isotropic.
2- Gamma-Ray Bursts Energy
● The source of GRBs are distant galaxies.
● Incredibly energetic.
8
☀
● Releasing more energy in a
second than the sun will, in its
entire ten billion years lifetime!
● Unlike other cosmic
explosions, which spread out
and fade, GRBs stay focused.
9
GRB 080319B :
- Detected by swift satellite at
March 19, 2008.
- Peak apparent magnitude of 5.3.
- Remained visible to human eyes
for 30 seconds.
- Occurred about 7.5 billion years
ago.
“
10
3- Types of Gamma-Ray Bursts
Short 𝛾-Ray Bursts Long 𝛾-Ray Bursts
Ultra-Long 𝛾-Ray
Bursts
Last for a few
seconds
Last for a minute
Last more than
10,000 seconds
Source : merge of 2
neutron stars in a binary.
30% of GRBs
Associated with
kilonovae.
Source : star
formation/core-collapse
supernova/deaths of massive
stars.
More than 50%
Source : collapse of a blue
supergiant stars/new-born
magnetar.
So rare
11
4- Effects of GRBs on Earth
● One GRB per day is
detected.
● Most of these GRBs
are harmless.
● Originated outside
the milky way.
● A nearby GRB could be disastrous! It would totally cook the
surface of the earth.
● A distant GRB are also dangerous. It wouldn’t need to be directly
pointing to us, because it would be a hundred light years wide
by the time it reaches us washing over the solar system.
12
13
● A GRB would overwhelm the ozone
layer.
● Exposed to deadly solar radiation.
● Our sattelites and power grids would
all be fried.
● Because of GRBs, only 10% of all
galaxies might be hospitable to life.
4.1 - Are GRBs
Going to Kill
Us?
14
N0
NO
No
No
No
No
No
● In a galaxy like the milky
way, there may only be one
GRB per million years.
● 𝛾-rays travel at the speed of
light, we won’t know when
it’s headed to us until it
arrives!!
15
4.2 -Did Any GRB Hit The
Earth ?
● A GRB may have hit the
earth about 1200 years ago.
● In 2012, scientists
discovered unusually high
levels of 2 particular
isotopes :
C Be
14
6
10
4
16
1- Ancient Trees.
Tree rings of old Japanese
cedars.
2- Ancient Ice.
Layers of Antarctic Ice.
17
18
5- August 17th, 2017
Gamma-Ray Burst and Gravitational Waves Detection.
● on Aug. 17, 2017: Scientists from U.S. and European
collaborations detected a GRB that coincided with
a burst of gravitational waves, followed by
kilonova.
● LIGO, and Virgo team, detected gravitational
waves produced by the coalescence of two
neutron stars.
● Two seconds later: NASA's Fermi Gamma-ray
Space Telescope detected a short flash of X-rays
and gamma rays from the same location in the sky.
19
● The gamma rays allow for a
precise localization of where the
gravitational waves are coming
from.
● The combined information from
gravitational and
electromagnetic radiation allows
scientists to probe the binary
neutron star system.
Credits
Special thanks to :
● ScienceDaily website.
● 2-days Gamma-Ray Bursts workshop at AUS
(2016)
20
21
Thanks!
Any questions?
You can find me at U14220199@sharjah.ac.ae

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Gamma-Ray Bursts (GRBs)

  • 2. Outline 2 first What Are Gamma-Ray Bursts ? - Gamma-Rays - How Can We Detect Gamma Rays ? GRBs Energy second GRBs Types third Effects of GRBs on Earth - Are They Going to Kill us ? - Did Any GRBs Hit the Earth ? last August 17th,2017 GRB and Gravitational Wave Detection last
  • 3. 1- What Are Gamma-Ray Bursts ? 3 ● The brightest electromagnetic events in the universe. ● Extremely energetic explosions observed in distant galaxies. ● Lasts from ten milliseconds to several hours. ● Followed by slowly fading emission at longer wavelengths created by collisions between the burst ejecta and interstellar gas ( Afterglow ).
  • 4. 4
  • 5. 1.1 - Gamma-Rays ● Electromagnetic radiation ● Carry very high energy. ● A single gamma-ray photon is more energetic than a million visible photons combined ! ● DANGEROUS ?? Form of Ionizing Radiation, it can break apart atomic bonds. 5 E=hf
  • 6. 1.2 - How Can We Detect Gamma-Rays ? ● Our Atmosphere (Ozone Layer O3 ) blocks 𝛾-rays. ● 𝛾-rays should be detected by spacecrafts. ● The discovery of 𝛾-ray bursts was during the cold war, when the USA sent up spy satellites to detect 𝛾-rays from soviet nuclear tests!. 6
  • 8. 2- Gamma-Ray Bursts Energy ● The source of GRBs are distant galaxies. ● Incredibly energetic. 8 ☀ ● Releasing more energy in a second than the sun will, in its entire ten billion years lifetime! ● Unlike other cosmic explosions, which spread out and fade, GRBs stay focused.
  • 9. 9 GRB 080319B : - Detected by swift satellite at March 19, 2008. - Peak apparent magnitude of 5.3. - Remained visible to human eyes for 30 seconds. - Occurred about 7.5 billion years ago.
  • 10. “ 10 3- Types of Gamma-Ray Bursts Short 𝛾-Ray Bursts Long 𝛾-Ray Bursts Ultra-Long 𝛾-Ray Bursts Last for a few seconds Last for a minute Last more than 10,000 seconds Source : merge of 2 neutron stars in a binary. 30% of GRBs Associated with kilonovae. Source : star formation/core-collapse supernova/deaths of massive stars. More than 50% Source : collapse of a blue supergiant stars/new-born magnetar. So rare
  • 11. 11 4- Effects of GRBs on Earth ● One GRB per day is detected. ● Most of these GRBs are harmless. ● Originated outside the milky way.
  • 12. ● A nearby GRB could be disastrous! It would totally cook the surface of the earth. ● A distant GRB are also dangerous. It wouldn’t need to be directly pointing to us, because it would be a hundred light years wide by the time it reaches us washing over the solar system. 12
  • 13. 13 ● A GRB would overwhelm the ozone layer. ● Exposed to deadly solar radiation. ● Our sattelites and power grids would all be fried. ● Because of GRBs, only 10% of all galaxies might be hospitable to life.
  • 14. 4.1 - Are GRBs Going to Kill Us? 14 N0 NO No No No No No ● In a galaxy like the milky way, there may only be one GRB per million years. ● 𝛾-rays travel at the speed of light, we won’t know when it’s headed to us until it arrives!!
  • 15. 15 4.2 -Did Any GRB Hit The Earth ? ● A GRB may have hit the earth about 1200 years ago. ● In 2012, scientists discovered unusually high levels of 2 particular isotopes : C Be 14 6 10 4
  • 16. 16 1- Ancient Trees. Tree rings of old Japanese cedars. 2- Ancient Ice. Layers of Antarctic Ice.
  • 17. 17
  • 18. 18 5- August 17th, 2017 Gamma-Ray Burst and Gravitational Waves Detection. ● on Aug. 17, 2017: Scientists from U.S. and European collaborations detected a GRB that coincided with a burst of gravitational waves, followed by kilonova. ● LIGO, and Virgo team, detected gravitational waves produced by the coalescence of two neutron stars. ● Two seconds later: NASA's Fermi Gamma-ray Space Telescope detected a short flash of X-rays and gamma rays from the same location in the sky.
  • 19. 19 ● The gamma rays allow for a precise localization of where the gravitational waves are coming from. ● The combined information from gravitational and electromagnetic radiation allows scientists to probe the binary neutron star system.
  • 20. Credits Special thanks to : ● ScienceDaily website. ● 2-days Gamma-Ray Bursts workshop at AUS (2016) 20
  • 21. 21 Thanks! Any questions? You can find me at U14220199@sharjah.ac.ae