Light and stars Flashcards

(50 cards)

1
Q

includes gamma rays, X-rays, ultraviolet light, visible light, infrared
radiation, microwaves, and radio waves.

A

Electromagnetic radiation

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2
Q

the arrangement of electromagnetic radiation according to wavelength.

A

electromagnetic spectrum

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3
Q

a small packet of light energy.

A

photon

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4
Q

the study of the properties of light that
depend on wavelength.

A

spectroscopy

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5
Q

an uninterrupted band
of light emitted by an incandescent solid, liquid, or gas under pressure.

A

continuous spectrum

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6
Q

a continuous spectrum produced when white light passes through a cool gas under low pressure. The gas absorbs selected wavelengths of light, and the
spectrum looks like it has dark lines
superimposed.

A

Absorption spectrum

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7
Q

s a series of bright lines
of particular wavelengths produced by a hot gas under low pressure.

A

emission spectrum

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8
Q

“FINGERPRINTS” lines
identify the elements present and thus the star’s chemical composition.

A

SPECTRAL LINES

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9
Q

the apparent change in
frequency of electromagnetic or sound waves caused by the relative motions of the source and
the observer.

A

Doppler effect

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10
Q

used to determine whether a star or other body in space is moving away from or toward Earth.

A

Doppler effect

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11
Q

a telescope that uses a
lens to bend or refract light

A

refracting telescope

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12
Q

produces an image
by bending light from a distant object so that the light converges at an area

A

focus

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13
Q

a telescope that reflects
light off a concave mirror, focusing the image in front of the mirror

A

reflecting telescope

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14
Q

a telescope designed to
make observations in radio wavelengths.

A

radio telescope

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15
Q

orbit above Earth’s atmosphere and thus
produce clearer images than Earth-based
telescopes.

A

space telescope

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16
Q

first space telescope, built by NASA

A

HUBBLE space telescope

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17
Q

telescope that study X-rays

A

Chandra X-Ray Observatory

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18
Q

used to study both visible light and gamma rays.

A

Compton Gamma- Ray Observatory

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19
Q

study infrared radiation.

A

James Webb Space Telescope

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20
Q

the region of the sun that
radiates energy to space, or the visible surface of the sun.

A

Photosphere

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21
Q

the first layer of the solar
atmosphere found directly above the
photosphere.

22
Q

the outer, weak layer of the solar
atmosphere

23
Q

a stream of protons and electrons
ejected at high speed from the solar corona.

24
Q

a dark spot on the sun that is cool

25
huge cloudlike structures consisting of chromospheric gases
prominences
26
ionized gases trapped by magnetic fields that extend from regions of intense solar activity.
prominences
27
brief outbursts that normally last about an hour and appear as a sudden brightening of the region above a sunspot cluster.
solar flares
28
are bright displays of ever-changing light caused by solar radiation interacting with the upper atmosphere in the region of the poles.
Auroras
29
the way that the sun produces energy. This reaction converts four hydrogen nuclei into the nucleus of a helium atom, releasing a tremendous amount of energy
nuclear fussion
30
is 74% hydrogen
Sun
31
large region in the corona which is less dense and is cooler than its surroundings. Through these holes, streams of solar wind escape at high speeds.
corona hole
32
A pattern that we recognize in the night sky
asterism
33
An apparent group of stars originally named after mythical characters
constellations
34
a constellation that is very prominent and easily recognizable; close to the equator and visible everywhere.
Orion
35
Brightest star
Alpha star
36
how many constellation in present day?
88
37
what path does stars move?
westward
38
is our north star, directly above the earth's axis at the North Pole.
Polaris
39
disappear or lose brightness.
eclipses/ecliptic
40
a unit of distance; It is the distance that light travels in one year.
light year
41
A nearby star can be viewed from earth and is seen in a position among other stars.
stellar paralax
42
A nearby star can be viewed from earth and is seen in a position among other stars.
stellar parallax
43
The study of the aspects and properties of the spectrum
spectroscopy
44
he total energy radiated by the star every second in all its forms and wavelengths.
Luminosity
45
Hottest star
O
46
The bluer a star appears=
the hotter the star
47
Coolest star
M
48
The wavelengths become smaller and the perceived color will shift toward O blue
blue shift
49
As the wavelengths gets larger, the color shifts toward red.
red shift
50
A very large mass of gas and dust in space
Nebula