3/31 Astro

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Last updated 3:40 AM on 3/31/26
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21 Terms

1
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Why was betelgeuse dimming

dust coming from atmosphere

2
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Where do magnetic field lines extend away from sun

coronal holes

3
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what makes the solar wind

charged particles that float away

4
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what makes tails of comets

solar wind

5
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sunspots

cooler areas in photosphere

6
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interstellar medium

gas and dust between stars

7
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interstellar extinction

dust blocks visible light from stars

8
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extinction, reddening

fainter, redder

9
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reddening

dust blocks short blue wavelengths but not red ones

10
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what produces absorbtion line spectra

intercloud gas

11
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where do stars form

molecular clouds

12
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obiect at center of disk

protostar

13
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are protostars easily observable?

no, cool and buried in dense clouds

14
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protostar is always in

hydrostatic equilibrium

15
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Molecular cloud, gravitational collapse, fragmentation into dense cores, collapsing molecular cloud core, protostar, protostar heats and contracts, hydrogen fusion begins, main-sequence star

16
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star clusters

gravitationally bound group of stars

17
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is betelgeuse on main sequence

no, red supergiant, late stage

18
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What does dust in space do to the light given off by stars

absorbs and scatters light, dimmer and redder

19
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Explain why viewing the sky through multiple different light spectra helps us understand how stars form

different wavelengths show different materials, temps, structures hidden by dust

20
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Stars are considered fully developed when they can burn what?

hydrogen

21
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do heavier more massive stars take longer to form?

yes

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