Review in Physical Science 11

Review in Physical Science 11

1st Grade

40 Qs

quiz-placeholder

Similar activities

Big Science Work: Physical Science

Big Science Work: Physical Science

1st - 5th Grade

40 Qs

chem

chem

1st Grade

38 Qs

UJIAN TOPIKAL FORM 3 (SCIENCE)

UJIAN TOPIKAL FORM 3 (SCIENCE)

1st - 5th Grade

40 Qs

Prashnawali grade 1&2

Prashnawali grade 1&2

1st - 2nd Grade

40 Qs

science - chemical reaction

science - chemical reaction

1st Grade

40 Qs

Force and Motion

Force and Motion

1st - 3rd Grade

40 Qs

Science Vocabulary

Science Vocabulary

1st - 5th Grade

40 Qs

Year 9 eoy revision

Year 9 eoy revision

1st - 5th Grade

40 Qs

Review in Physical Science 11

Review in Physical Science 11

Assessment

Quiz

Science

1st Grade

Hard

Created by

jefferson cristobal

Used 10+ times

FREE Resource

40 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which is the first stage of a star’s life cycle?

black hole

nebula

protostar

white dwarf

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

In main sequence star, Hydrogen fuses and converted to Helium. What element is produced from Helium gas at its core?

C

Fe

Ne

Si

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How is the energy of star produced?

combustion

decomposition

Nuclear Fusion

Nuclear Fission

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

When does a star become unstable

When it runs out of fuel.

When it contracts and expands.

When its cores is converted to Iron.

When the outer shell of star is pulled by the gravity from the center.

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

This is known as the origin and production of heavy elements.

Stellar Nucleosynthesis

Primordial Nucleosynthesis

S-Process

Supernova Nucleosynthesis

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

It was created by bombardment of molybdenum by deuterons (heavy hydrogen, H12), by Emilio Segre and Carlo Perrier in 1937.

Oxygen

Helium

Technetium

Uranium

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

In this process there’s a buildup of a VERY heavy isotope, then as beta-decays occur, you march up in atomic number and produce heavy product.

S-Process

R-Process

Nuclear Fission

Nuclear Fusion

Create a free account and access millions of resources

Create resources
Host any resource
Get auto-graded reports
or continue with
Microsoft
Apple
Others
By signing up, you agree to our Terms of Service & Privacy Policy
Already have an account?

Discover more resources for Science