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Explain in the three to four sentences of a least 2 ways astronomers determine distances to local stars, distant galaxies, and the width of the observable universe.
parallax - the shift in stars position
standard candles - known luminosity tells us about Ia supernovae
red shift and hubble’s law - for very distant galaxies
Describe in two to four sentences about dark matter and dark energy and answering the following questions. What fraction of energy budget of the Universe is made up of visible matter, dark matter, and dark energy? For dark matter, how do we know it exists? What is dark energy doing to the Universe?
5 % visible, 27% dark matter, 68% dark energy
dark matter is inferred from galaxy rotation curves and gravitational lensing
dark energy causes the expansion of the universe
Describe in two to three sentences the three structure components of the Milky Way galaxy and the type of objects in each structure. For example what star generation, gases/dust, super massive black hole.
disk - young stars, spiral arms, ongoing star formation, gas, dust
bulge - older stars, supermassive blackhole
halo - globular clusters, large amounts of dark matter
Describe in two to three sentences the three structure components of the Milky Way galaxy and the type of objects in each structure. For example what star generation, gases/dust, super massive black hole.
disk - young stars, spiral arms, ongoing star formation, gas, dust
bulge - older stars, supermassive blackhole
halo - globular clusters, large amounts of dark matter
Describe in two to four sentences about dark matter and dark energy and answering the following questions. What fraction of energy budget of the Universe is made up of visible matter, dark matter, and dark energy? For dark matter, how do we know it exists? What is dark energy doing to the Universe?
5 % visible, 27% dark matter, 68% dark energy
dark matter is inferred from galaxy rotation curves and gravitational lensing
dark energy causes the expansion of the universe
Explain in the three to four sentences of a least 2 ways astronomers determine distances to local stars, distant galaxies, and the width of the observable universe.
parallax - the shift in stars position
standard candles - known luminosity tells us about Ia supernovae
red shift and hubble’s law - for very distant galaxies