CLEAN : Astronomers reveal first image of black hole at Milky Way's centre

CLEAN : Astronomers reveal first image of black hole at Milky Way's centre

Assessment

Interactive Video

Physics, Science

10th Grade - University

Hard

Created by

Quizizz Content

FREE Resource

The video discusses the process of refining images of black holes, focusing on the heart of the black hole, known as the point of no return. It highlights the significance of the Milky Way's center and the challenges faced in imaging black holes, such as magnetic fields and the evolving nature of black holes. The video also covers the importance of orientation and telescope positioning in capturing detailed images. The ultimate goal is to improve instruments and algorithms to better understand black holes, particularly Sagittarius A*.

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5 questions

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1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the 'point of no return' in a black hole?

The magnetic field

The accretion disk

The singularity

The event horizon

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How does Sagittarius A* compare to other black holes in terms of energy conversion?

It does not convert any energy into light

It is highly efficient in converting energy into light

It traps nearly all energy, converting only a small fraction into light

It converts all energy into light

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Why is the orientation of telescopes important in observing black holes?

It helps in capturing the entire galaxy

It reduces the interference from other celestial bodies

It allows for better focus on distant stars

Different angles capture different parts of the black hole

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is one major challenge in imaging Sagittarius A*?

The telescopes are not powerful enough

The black hole is too small

The black hole is too far away

The image is scattered by galactic gas

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the potential future direction for black hole imaging?

Improving instruments and algorithms

Reducing the number of observations

Using smaller telescopes

Focusing on other galaxies