1.7, 1.8, 1.9 Flashcards

1
Q

Albedo

A

The reflective property of a nonluminous object.

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2
Q

Photosphere

A

The visible surface of the sun. just below the chromosphere.

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3
Q

Chromosphere

A

A layer in the sun’s atmosphere. between the photosphere and coronas.

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4
Q

Corona

A

The outermost atmosphere of a star.

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5
Q

Ozone

A

A molecule made up of three oxygen atoms.

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6
Q

Electromagnetic Spectrum

A

The range of frequencies of electromagnetic radiation. Includes: radio, microwave, infrared, visible, light, UV, x-rays, and gamma rays.

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7
Q

Spectrum

A

a chart of the entire range of wavelengths of light from an object.

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8
Q

Luminosity

A

The total amount of energy radiated by an object every second.

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9
Q

Main-sequence star

A

star formed when the temperature in the center of a cloud reaches 15 million k.

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10
Q

Radiation

A

Emission of energy in the form of rays or waves.

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11
Q

wavelength

A

The horizontal distance between two successive crests of a wave.

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12
Q

supernova

A

the death explosion of a massive star whose core has completely burned out.

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13
Q

Radiative zone

A

carries energy from the core outward by using protons.

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14
Q

Convective Zone

A

convective currents carry the energy outward to the surface. hot materials rise and cool materials fall.

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15
Q

Core

A

The core creates nuclear fusion reactions fusing hydrogen atoms to create helium.

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16
Q

HR diagram

A

Position represents the color of an absolute magnitude of the star at various stages in its evolution.

17
Q

Apparent Magnitude

A

How bright the star appears to us from our point of view.

18
Q

Absolute Magnitude

A

the magnitude the star would have if it was placed at a distance of 10 parsecs from earth.

19
Q

Black hole

A

supernova remnants from a star 3x more massive than our sun.

20
Q

Spectral class

A

depends on color/temperature and a few more factors. OBAFGKM

21
Q

Solar Radii

A

The radius of the sun= 695,800 km

22
Q

What is meant by earth’s energy budget?

A

The amount of energy that is absorbed from the sun by earth changes in the amount of energy can cool us down or heat us up.

23
Q

what is the difference between apparent magnitude and absolute magnitude?

A

Apparent= what it appears to be. Absolute= what it really is

24
Q

How do we measure wavelength?

A

Like point to point.

25
Q

What part of a stars life is a white dwarf.

A

Final stage, will slowly begin to cool and become a deaf black dwarf.

26
Q

What type of storm could interfere with our electromagnetic power grid system.

A

Solar flares.

27
Q

How long is the sunspot cycle?

28
Q

How would the earths albedo be affected if it were covered by ice?

A

The albedo would increase and the earth would become colder.

29
Q

What layer are solar storms produced in

A

photosphere

30
Q

What type of land would reflect the most incoming radiation and what type would absorb the most?

A

Reflect= ice/white snow; Absorb= dark colors (forest, dark rock/land)

31
Q

The order of colors observed in the visible light are determined by what?

A

Wavelength

32
Q

What part of the EM spectrum has the longest wave.

A

Radiowaves

33
Q

What is the order of the EM spectrum as it increases from the largest wavelength to the smallest?

A

Radio. microwave, infrared, visible, UV, x-ray, and gamma ray

34
Q

What is the relationship between wavelength and frequency on the EM spectrum.

A

As the wavelength decreases the frequency increases

35
Q

How has the EM spectrum helped us study objects in space?

A

Different telescopes help us see objects in space we could not otherwise see.

36
Q

What determines a stars color?

A

temperature.

37
Q

What determines the life-cycle path of a star?

38
Q

What did our sun form from?