DIFFICULT LEVEL

DIFFICULT LEVEL

12th Grade

15 Qs

quiz-placeholder

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DIFFICULT LEVEL

DIFFICULT LEVEL

Assessment

Quiz

Science

12th Grade

Practice Problem

Hard

Created by

Jhuly-An Villanueva

Used 2+ times

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15 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which of the following best describes the shape of the universe according to current cosmological models?

Perfectly spherical

Flat with possible curvature

Hyperbolic

Cylindrical

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the Chandrasekhar limit, and why is it significant in stellar evolution?

The minimum mass a star needs to become a supernova

The maximum mass a white dwarf can have before collapsing into a neutron star or black hole

The temperature required for nuclear fusion to begin in a star

The distance a planet must be from its star to have liquid water

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which of these methods is used to detect exoplanets?

Transit method

Doppler shift (radial velocity)

Direct imaging

All of the above

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the primary force counteracting gravity inside a main-sequence star?

Magnetic pressure

Nuclear fusion pressure

Radiation pressure

Electron degeneracy pressure

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the Roche limit, and why is it important?

The distance where a planet's gravity is too weak to hold a moon

The minimum distance a satellite must maintain before being torn apart by tidal forces

The maximum radius of a black hole's event horizon

The point at which a star stops nuclear fusion

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the significance of the Schwarzschild radius of a black hole?

It marks the distance where the gravitational force is strongest

It defines the event horizon beyond which nothing can escape

It is the radius of the singularity inside a black hole

It measures the spin rate of a black hole

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

A planet orbits a star at a distance of 5 AU. Using Kepler’s Third Law, determine its orbital period. (Assume the mass of the star is equal to the Sun's.)

5 years

11.2 years

25 years

7.5 years

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