1/20
Looks like no tags are added yet.
Dark Matter and the Large-Scale Universe
• Dark matter
Matter inferred from its gravitational effects, although it does not emit or absorb light like ordinary luminous matter.
• Luminous matter
Matter that emits, reflects, or otherwise interacts with light so it can be observed electromagnetically.
Doppler Effect and Galaxy Rotation
• Doppler effect
Motion changes observed wavelength. Toward us = blueshift; away from us = redshift.
• Astronomers measure Doppler shifts of stars and gas on different sides of a galaxy to determine how quickly they orbit its center.
• Rotation curve
Graph of orbital speed of stars or gas versus distance from a galaxy’s center.
• If most mass were concentrated where visible matter is, outer objects would be expected to orbit more slowly with increasing distance.
•Evidence
Many galaxies’ outer regions rotate faster than expected; their rotation curves stay roughly flat instead of dropping.
• Conclusion
Unexpectedly fast outer motion suggests additional unseen mass spread through an extended halo
Proposed Dark Matter Explanations
• MACHOs
Massive Astrophysical Compact Halo Objects—dim or nonluminous compact objects, such as faint stars or stellar remnants, that could contribute mass in a halo.
• WIMPs
Weakly Interacting Massive Particles—hypothetical particles with mass that interact very weakly with ordinary matter and light.
• Know what WIMPs are and recognize MACHOs and WIMPs as proposed explanations.
The Cosmic Web
• Cosmic web
Large-scale structure consisting of dark matter filaments, dense intersections, and large voids.
• Filaments
Long structures where dark matter and galaxies are distributed.
• Intersections
Dense meeting points of filaments where galaxies and galaxy clusters are commonly found.
• Voids
Large, relatively empty regions between filaments.
• Gravity and galaxy formation
Dark matter’s gravity gathers ordinary matter into dense regions; galaxies form and grow preferentially in these structures.