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Astro 101 Exam 2 Questions And Answers |Latest 2025 | Guaranteed Pass.

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©FYNDLAY 2024/2025 ALL RIGHTS RESERVED 1:25PM A+ 1 Astro 101 Exam 2 Questions And Answers |Latest 2025 | Guaranteed Pass. Revolutions in the solar system - AnswerMostly Counterclockwise- comets can be both Rotations in the solar system - AnswerMostly Counterclockwise. Clockwise=Venus Between=Uranus Milky Way rotation - Answer200 km/s Two clouds that are on adjacent circular orbits around the galaxy. What happens as they orbit? - AnswerThe inside cloud will eventually pass the outside one Molecular Clouds - AnswerCool and dense-short lived-can collapse and fragment Cloud Core - AnswerContain a protostar-small and hot Accretion disks - Answerdense, hot, short-lived Protostar - Answerdense, compressed interior. stable structure due to Hydrostatic Equilibrium: no more collapse when pressure matches weight of star Hydrostatic Equilibrium - AnswerWeight of material above pushes in an inward direction. gravity and pressure balance out Solar Nebular Theory - Answer• An enormous cloud of dust and gas collapses into multiple cores. • cores starts to form a disk around a protostar. • Material in the disk clumps. • These clumps (also called cores) draw in gas, turn into planets. • The protostar grows large enough to turn into a young star, blowing away the disk, leaving the planets. The temperature of the proto-Earth was about 600 K, thus the Earth formed out of: - AnswerAll substances that can condense at temperatures below 600 K. The composition of the solar nebula is likely similar to: - AnswerThe Sun F=ma - Answerexternal forces F on an object is equal to the mass m of that object multiplied by the acceleration ©FYNDLAY 2024/2025 ALL RIGHTS RESERVED 1:25PM A+ 2 William Herschel - AnswerDiscovered- Uranus and 4 Moons, Infrared Light • Telescopes made: >400 • Symphonies written: 24 Ole Romer - AnswerOle Romer- Measured speed of light- 131,000 mpsecond Hipparchus - AnswerFirst comprehensive star catalog, rated stars on a six point scale of brightness--which we still use. Apparent Magnitude - Answer- smaller numbers= brighter (m) Luminosity vs Brightness - Answer• Brightness is apparent—what we see. • Luminosity is energy output/second—an intrinsic (absolute) measure Absolute luminosity+magnitude - AnswerAbsolute luminosity is defined as the same as apparent Absolute magnitude (M) most negative= most luminous (brightest) Brightness = Luminosity / distance2 • BUT! Don't use magnitudes in this equation • Use solar luminosities instead - AnswerBrightness=l/d^2 Black body/thermal radiation - Answerabsorbs all incident electromagnetic radiation The color of a black body is a quick measure of its temperature. • red = ~3000 K • yellow = ~5500 K • blue = ~30,000 K Wien's displacement law - Answerstates that the black body radiation curve for different temperatures peaks at a wavelength inversely proportional to the temperature. Two stars same size and distance which is hotter - AnswerWhich peak is higher Which of these stars in Orion is most luminous? star m M distance 1 Rigel 0.18 -6.69 773 2 Betelgeuse 0.42 -6.02 643 3 Bellatrix 1.64 -2.72 242 4 Alnilam 1.69 -6.38 - Answer1. Rigel- Most negative=most luminous Two stars at the same distance, which is more luminous? - AnswerWhichever is putting out more light at all wavelengths Two stars at the same distance, which looks redder? - AnswerWhich peak is in the red section 600-700nm Two stars at the same distance, which

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Astro 101 Exam 2 Questions And Answers
|Latest 2025 | Guaranteed Pass.


Revolutions in the solar system - Answer✔Mostly Counterclockwise- comets can be both

Rotations in the solar system - Answer✔Mostly Counterclockwise. Clockwise=Venus
Between=Uranus

Milky Way rotation - Answer✔200 km/s
Two clouds that are on adjacent circular orbits around the galaxy. What happens as they orbit?
- Answer✔The inside cloud will eventually pass the outside one

Molecular Clouds - Answer✔Cool and dense-short lived-can collapse and fragment

Cloud Core - Answer✔Contain a protostar-small and hot

Accretion disks - Answer✔dense, hot, short-lived

Protostar - Answer✔dense, compressed interior. stable structure due to Hydrostatic
Equilibrium: no more collapse when pressure matches weight of star

Hydrostatic Equilibrium - Answer✔Weight of material above pushes in an inward direction.
gravity and pressure balance out

Solar Nebular Theory - Answer✔• An enormous cloud of dust and gas collapses into multiple
cores. • cores starts to form a disk around a protostar. • Material in the disk clumps. • These
clumps (also called cores) draw in gas, turn into planets. • The protostar grows large enough to
turn into a young star, blowing away the disk, leaving the planets.
The temperature of the proto-Earth was about 600 K, thus the Earth formed out of: -
Answer✔All substances that can condense at temperatures below 600 K.

The composition of the solar nebula is likely similar to: - Answer✔The Sun

F=ma - Answer✔external forces F on an object is equal to the mass m of that object multiplied
by the acceleration


1

, ©FYNDLAY 2024/2025 ALL RIGHTS RESERVED 1:25PM A+


William Herschel - Answer✔Discovered- Uranus and 4 Moons, Infrared Light • Telescopes
made: >400 • Symphonies written: 24

Ole Romer - Answer✔Ole Romer- Measured speed of light- 131,000 mpsecond

Hipparchus - Answer✔First comprehensive star catalog, rated stars on a six point scale of
brightness--which we still use.

Apparent Magnitude - Answer✔- smaller numbers= brighter (m)

Luminosity vs Brightness - Answer✔• Brightness is apparent—what we see. • Luminosity is
energy output/second—an intrinsic (absolute) measure

Absolute luminosity+magnitude - Answer✔Absolute luminosity is defined as the same as
apparent
Absolute magnitude (M) most negative= most luminous (brightest)
Brightness = Luminosity / distance2 • BUT! Don't use magnitudes in this equation • Use solar
luminosities instead - Answer✔Brightness=l/d^2

Black body/thermal radiation - Answer✔absorbs all incident electromagnetic radiation The
color of a black body is a quick measure of its temperature. • red = ~3000 K • yellow = ~5500 K
• blue = ~30,000 K

Wien's displacement law - Answer✔states that the black body radiation curve for different
temperatures peaks at a wavelength inversely proportional to the temperature.

Two stars same size and distance which is hotter - Answer✔Which peak is higher
Which of these stars in
Orion is most luminous?
star m M distance
1 Rigel 0.18 -6.69 773
2 Betelgeuse 0.42 -6.02 643
3 Bellatrix 1.64 -2.72 242

4 Alnilam 1.69 -6.38 - Answer✔1. Rigel- Most negative=most luminous
Two stars at the same distance, which is more

luminous? - Answer✔Whichever is putting out more light at all wavelengths

Two stars at the same distance, which looks redder? - Answer✔Which peak is in the red section
600-700nm
Two stars at the same distance, which emits more red

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