Mars Orbit and Retrograde Motion

Mars Orbit and Retrograde Motion

Assessment

Interactive Video

Physics, Science, Geography

9th - 10th Grade

Hard

Created by

Patricia Brown

FREE Resource

The video explains the apparent retrograde motion of Mars, which is an illusion caused by the different orbital speeds and distances of Mars and Earth. Mars appears to slow down, stop, and move backward in the sky due to Earth's faster orbit. This phenomenon is also applicable to other planets like Mercury and Venus, although their retrograde motions are harder to observe due to their proximity to the Sun.

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7 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the observed motion of Mars in the sky over a two-year period?

It remains stationary.

It speeds up continuously.

It appears to slow down, stop, and move backward.

It moves in a straight line.

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What causes the apparent retrograde motion of Mars?

Mars actually moves backward in its orbit.

Earth's orbit is slower than Mars'.

The different orbital speeds and distances of Mars and Earth.

Mars orbits the Sun in the opposite direction.

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How often does Earth catch up and pass Mars in their orbits?

Every five years

Every two years

Every six months

Every year

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What visual effect is created when Earth passes Mars?

Mars' path looks like a loop.

Mars appears to disappear.

Mars becomes brighter.

Mars changes color.

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How long does it take Mars to complete one orbit around the Sun?

730 days

365 days

687 days

500 days

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which planets also exhibit apparent retrograde motion?

Mercury and Venus

All planets except Earth

Only the outer planets

Only Mars

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Why is it difficult to observe the retrograde motion of Mercury and Venus?

They are too far from Earth.

They do not exhibit retrograde motion.

They are always visible during the night.

They pass Earth during the daytime.