AS101 LESSON 6

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

1/37

encourage image

There's no tags or description

Looks like no tags are added yet.

Last updated 12:50 AM on 4/21/26
Name
Mastery
Learn
Test
Matching
Spaced
Call with Kai

No analytics yet

Send a link to your students to track their progress

38 Terms

1
New cards

Light

Electromagnetic transverse wave and main tool of astronomy

2
New cards

Why light is important in astronomy

Most information about universe comes from analyzing light

3
New cards

Electromagnetic spectrum

All forms of light including radio, infrared, visible, ultraviolet, X-ray, gamma ray

4
New cards

Visible light

Small part of full electromagnetic spectrum

5
New cards

Wave properties of light

Wavelength, frequency, speed

6
New cards

Light wave formula

Frequency × wavelength

7
New cards

Speed of light

3 × 10^8 m/s (300,000 km/s)

8
New cards

Wavelength measured in

Nanometres (nm)

9
New cards

Frequency measured in

Hertz (Hz)

10
New cards

Long wavelength means

Lower frequency and lower energy

11
New cards

Short wavelength means

Higher frequency and higher energy

12
New cards

Photon

Packet of light energy

13
New cards

Photon energy

Directly proportional to frequency

14
New cards

Light interactions with matter

Absorbed, reflected, transmitted, refracted, emitted

15
New cards

Refraction

Bending of light when entering new medium

16
New cards

Prism effect

Separates white light into spectrum

17
New cards

Source of light

Atomic or molecular energy transitions

18
New cards

Emission spectrum

Unique set of spectral lines for each element

19
New cards

Use of spectra in astronomy

Determine composition, temperature, motion

20
New cards

Doppler Effect

Change in observed wavelength/frequency due to motion

21
New cards

Redshift

Object moving away; wavelengths stretched longer

22
New cards

Blueshift

Object moving toward; wavelengths shortened

23
New cards

Use of Doppler Effect in astronomy

Measure radial motion of stars/galaxies

24
New cards

Optical device common features

Collect light, focus light, detect light

25
New cards

Human eye parts

Pupil, lens, retina

26
New cards

Camera parts

Lens, aperture, shutter, detector/film

27
New cards

CCD

Electronic light detector with high efficiency used in astronomy

28
New cards

Quantum efficiency highest

CCD (better than eye or film)

29
New cards

Two basic visible-light telescopes

Refracting and reflecting

30
New cards

Refracting telescope

Uses lens to focus light

31
New cards

Reflecting telescope

Uses mirror to focus light

32
New cards

Main telescope properties

Light-gathering power and resolving power

33
New cards

Light-gathering power

Ability to collect faint light; larger aperture is better

34
New cards

Resolving power

Ability to distinguish close objects

35
New cards

Magnification

Not most important telescope property

36
New cards

Ground telescopes problems

Atmosphere, weather, light pollution

37
New cards

Hubble Space Telescope significance

Above atmosphere gives clearer images and major discoveries

38
New cards

Space telescope advantage

Can observe wavelengths blocked/distorted by atmosphe