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Multi-messenger Astronomy

Total questions: 30

Worksheet time: 23mins

Name
Class
Date
1.

Which of these is not a messenger for astronomy?

a)

Electromagnetic waves

b)

Cosmic rays

c)

Neutrons

d)

Gravitational waves

2.

Identify the telescope which is about to launch in the near future.

a)
b)
c)
d)
3.

Supernova is known to emit what of the following (more than 1 option is correct)

a)

Cosmic rays

b)

Neutrino

c)

Electromagnetic waves

d)

Gravitational waves

4.

DUNE is an experiment to detect which of the following Messenger?

a)

Cosmic ray particles

b)

Photons

c)

Gravitational waves

d)

None of the above

5.

Which messenger of astronomy played an important role in getting this image?

a)

Gravitational waves

b)

Neutrinos

c)

Electromagnetic waves

d)

Cosmic rays

6.

Identify this

a)

Microwave telescope

b)

UV telescope

c)

IR telescope

d)

Radio telescope

7.

Which could be the hottest star among the following?

a)
b)
c)
d)
e)
8.

What does this image depict?

a)

Absorption Spectral lines

b)

Emission spectral lines

c)

Continuous spectral lines

d)

None of the above

9.

Which messenger of astronomy is not a fundamental particle?

a)

Neutrinos

b)

Electromagnetic waves

c)

Cosmic rays

d)

Gravitational waves

10.

What types of waves are gravitational waves?

a)

Transverse - Dipolar

b)

Longitudinal - Dipolar

c)

Transverse - Quadrupolar

d)

Longitudinal - Quadrupolar

11.

What is the principle behind this detector? (more than 1 option is correct)

a)

Superposition

b)

Interference

c)

Diffraction

d)

Refraction

12.

Arrange the phases of Gravitational wave production through Inspiral mechanism

a)

Spiralling - Merger - Ringdown

b)

Merger - Spiralling - Ringdown

c)

Ringdown - Spiralling - Merger

d)

Spiralling - Ringdown - Merger

13.

Which type of Gravitational wave is hard to detect? (more than 1 option is correct)

a)

Compact binary inspiral

b)

Continuous

c)

Stochastic

d)

Burst

14.

Core collapse supernova emits this messenger abundantly

a)

Gravitational waves

b)

Gamma rays

c)

Neutrinos

d)

Cosmic rays

15.

Which of the following has its charge and its anti-particle's charge both to be equal to zero? (more than 1 option is correct)

a)

Muon neutrino

b)

electron neutrino

c)

tau neutrino

d)

cosmic ray particles

16.

Which is the main nuclear reaction that occurs in a core-collapse supernova?

a)
b)
c)
d)
17.

The detector of ICE-CUBE Neutrino Observatory is most sensitive to the following:-

a)
b)
c)
d)

All of the above

18.

The main reasons why neutrinos are least interactive are (more than 1 option is correct)

a)

The rest mass of the neutrino is much smaller than that of the other known elementary particles.

b)

Neutrinos participate only through weak interactions which are very short-ranged.

c)

Because of Neutrino oscillations.

d)

Neutrinos don't have an electric charge

19.

What does this Feynman diagram represent? (more than 1 option is correct)

a)

Beta minus decay

b)

Proton decay

c)

Neutron decay

d)
20.

Identify this detector

a)

Super-Kamiokande

b)

ICE-CUBE

c)

ALBORZ

d)

TRACER

21.

What is the phenomenon observed when the speed of a particle in a medium is more than the speed of light in that particular medium?

a)

Photonic boom

b)

Sonic boom

c)

Cherenkov effect

d)

Anomalous dispersion

22.

Cosmic ray particles are primarily (mostly) made of?

a)

Positrons and electrons

b)

Helium nuclei

c)

Protium nuclei

d)

Neutrinos

23.

Which of the following protects us from cosmic rays. (more than 1 option is correct)

a)

Earth's magnetic field

b)

Atmosphere

c)

Ozone layer

d)

All of the above

24.

What was the method used to find the void in the Great Pyramids of Giza in Egypt?

a)

Electron tomography

b)

Muon tomography

c)

Tau tomography

d)

None of the above

25.

What is the highest possible total collision energy of LHC till date?

a)

14 Tev

b)

10 Tev

c)

8 Tev

d)

13 Tev

26.

What is the limit that dictates how far can cosmic rays come from?

a)

Greisen–Zatsepin–Kuzmin limit

b)

Planck limit

c)

Victor Hesses limit

d)

Speed limit

27.

What is the occurrence rate of Gamma ray Bursts?

a)

About a 100 per solar system

b)

Proportional to the number of stars in a galaxy

c)

A few per galaxy cluster per year

d)

A few per galaxy per million years

28.

What were the Vela satellites originally designed for?

a)

Detection of Gamma Ray Bursts

b)

Detection of radio signals from outer space

c)

Detection of the covert nuclear weapons test

d)

Communication

29.

The distribution of Gamma Ray Bursts is :-

a)

Prominent near the Large Magellanic Cloud

b)

Isotropic (uniformly distributed)

c)

Prominent near Sagittarius A*

d)

None of the above

30.

Which satellite first detected the X-ray afterglow of a Gamma ray Burst?

a)

BeppoSAX

b)

Castel-Gauss

c)

Vela

d)

Chandra X-ray