Ch.2 Naked Eye Universe

0.0(0)
Studied by 0 people
call kaiCall Kai
learnLearn
examPractice Test
spaced repetitionSpaced Repetition
heart puzzleMatch
flashcardsFlashcards
GameKnowt Play
Card Sorting

1/32

encourage image

There's no tags or description

Looks like no tags are added yet.

Last updated 6:31 PM on 10/8/26
Name
Mastery
Learn
Test
Matching
Spaced
Call with Kai
Chat

No analytics yet

Send a link to your students to track their progress

33 Terms

1
New cards

Celestial sphere

Imaginary sphere used to map positions of objects in the sky.

2
New cards

Constellation

Recognizable pattern or defined region of stars in the sky.

3
New cards

Why are constellations useful?

They provide a reference background for tracking sky motions.

4
New cards

Daily apparent sky motion

Sun, Moon, and stars generally rise east and set west because Earth rotates eastward.

5
New cards

Celestial poles

Points in the sky aligned with Earth's rotation axis.

6
New cards

Circumpolar stars

Stars that never set at a given observing latitude.

7
New cards

Ecliptic

Apparent yearly path of the Sun against background stars.

8
New cards

Why does the Sun drift eastward against stars?

Earth revolves around the Sun.

9
New cards

Moon's motion against stars

Moon gradually moves eastward relative to background stars.

10
New cards

Moon phases

Changing appearance of Moon's sunlit half as seen from Earth.

11
New cards

Cause of Moon phases

Changing Sun–Earth–Moon viewing geometry, not Earth's shadow.

12
New cards

New Moon

Moon lies roughly toward the Sun; illuminated half faces away from Earth.

13
New cards

Full Moon

Earth-facing lunar hemisphere appears illuminated.

14
New cards

First-quarter Moon

Half of the visible Moon is lit while waxing.

15
New cards

Third-quarter Moon

Half of the visible Moon is lit while waning.

16
New cards

Waxing

Illuminated fraction of the Moon appears to increase.

17
New cards

Waning

Illuminated fraction of the Moon appears to decrease.

18
New cards

Solar eclipse

Moon passes between Earth and Sun and casts a shadow on Earth.

19
New cards

Lunar eclipse

Earth passes between Sun and Moon, shadowing the Moon.

20
New cards

Umbra

Region of complete shadow.

21
New cards

Penumbra

Region of partial shadow.

22
New cards

Why not an eclipse every month?

Moon's orbital plane is tilted relative to Earth's orbit.

23
New cards

Why can the Moon cover the Sun?

Their apparent angular sizes are nearly equal.

24
New cards

Annular solar eclipse

Moon appears too small to cover Sun fully, leaving a bright ring.

25
New cards

Cause of seasons

Earth's tilted axis changes daylight duration and Sun angle.

26
New cards

Why is summer warmer?

Longer days and more direct sunlight deliver more energy.

27
New cards

Are seasons caused by Earth–Sun distance?

No; axial tilt is the main cause.

28
New cards

June solstice in Northern Hemisphere

Sun follows its highest yearly path; longest daylight.

29
New cards

December solstice in Northern Hemisphere

Sun follows its lowest yearly path; shortest daylight.

30
New cards

Equinox

Sun rises due east and sets due west; day and night nearly equal.

31
New cards

Why do seasonal changes grow at high latitudes?

Tilt produces larger differences in daylight and solar angle.

32
New cards

At midnight where are meridian stars relative to Sun?

On the opposite side of the sky from the Sun.

33
New cards

Why are some constellations not visible at night in a season?

They lie near the Sun in the daytime sky.