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Test your basic knowledge |
Cosmology
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Study First
Subject
:
science
Instructions:
Answer 50 questions in 15 minutes.
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Match each statement with the correct term.
Don't refresh. All questions and answers are randomly picked and ordered every time you load a test.
This is a study tool. The 3 wrong answers for each question are randomly chosen from answers to other questions. So, you might find at times the answers obvious, but you will see it re-enforces your understanding as you take the test each time.
1. The study of the universe as a whole.
tectonics of Mars
Gravity only pulls matter back together. Therefore - if gravity is the only force that operates on cosmic scales then the expansion of the universe should decrease with time. The critical density is the value of matter density sufficient to halt the
Absolute Magnitude
cosmology
2. The dimming of starlight by intervening dust
gravity
Total Eclipse
Interstellar Extinction
Electromagnetic Radiation: Radio
3. When the Sun is farthest north of the celestial equator (about June 22)
Summer Solstice
Electromagnetic Radiation: Infrared
protostar
fewest moons
4. The rate of expansion of the universe.
Hubble constant
Shepherd satellite
quasar
Synodic Day
5. Matter that reveals itself only through its gravitational attraction
conjunction
Dark Matter
interstellar dust
radiation pressure
6. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
Dark Nebula
Quasar
Corona
MOONS: larger than mercury
7. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Radio Galaxy
accretion disk
Prominence
Sc spiral galaxy
8. The faint glow of light left over from the Big Bang. cosmic microwave background are the photons that remain after the big bang that have not turned into matter.
evidence of water on mars
Electromagnetic Radiation: Radio
CMB
zone
9. As open clusters age - they push gas away but dust remains this can reflect light giving the cluster a blue-ish color. also called reflection nebula
Oort cloud
jovian
reflection star clusters
Synchrotron Rotation
10. The linear correlation between the rate of the expansion of the universe and distance. Says that as galaxies get farther away in space - the speed with which they recede from us increases. So we can measure the amount of recessional velocity and use
Light Curve
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Hubble law
Jupiters red spot
11. Population 1- similar to the sun and 2% of elements are metal - Population 2- formed before gas was metal- only a fraction of mass is metal.
force
Population 1 vs Population 2 stars
Grand design spirals
mass
12. A measure of the ability of a telescope to see fine detail
Degeneracy
Resolving Power
Doppler Shift
partile horizon
13. Small compact stars called white dwarfs can have material deposited on their surfaces. In time material heats up and explodes in surface nuclear reaction- star brightens - settles - repeats.
comet
Hyashi track
nova
Sidereal Day
14. Light scattered through the atmosphere that degrades astronomical images
Light Pollution
Degeneracy
difference between maria and highlands of the moon.
Synchrotron Rotation
15. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Hipparchus
The Big Bang Theory
Plague
Kirkwood gaps
16. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
Red Giant
neutrino
Heliocentric
Vernal Equinox
17. The nuclei of very distant galaxies. Likely a manifestation of supermassive black holes
Plague
Thermal Equilibrium
belt
Quasar
18. The larger bodies that formed early in teh solar nebula that were chemically differentiated
planetesimal
Supernova (You can be my supernova girl)
Summer Solstice
zone
19. 10^2 nm 10^7 nm
Electromagnetic Radiation: Visible Light
radio galaxy
planetary nebula
Electromagnetic Radiation: Gamma Ray
20. The family of radiant energy that includes light as a subset
cosmic singularity
Electromagnetic Radiation
Refractor
Umbra
21. Matter so dense that even light cannot escape its gravity
Nebula
Cosmological Principle
anorthosite
Black Hole
22. The average distance between the Earth and the Sun (=1.5 x10^8km)
Asymptotic giant Branch Star
Thickest atmosphere
Coronal Loop
Astronomical Unit
23. A galaxy emitting large amounts of energy at long wavelengths.
Drake equation
radio galaxy
Horizontal Branch Star
Light Pollution
24. A telescope that uses lenses to focus light
Energy Level
Refractor
Ecliptic
H2 Regions
25. A huge sphere of tenuous gas surrounding the nucleus of a comet
coma
inferior planets
radio lobe
fusion crust
26. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
synchrotron radiation
tectonics of Earth
Secondary Mirror
Brown dwarf
27. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
roche limit
Neutron Star
tectonics of Venus
Thickest atmosphere
28. The mass of an object divided by its volume
chondrite
Electromagnetic Radiation: Visible Light
density
Grand design spirals
29. A star that has become a red giant for the second and final time. It is burning helium to carbon in a shell surrounding the core
Asymptotic giant Branch Star
Proton-proton chain
Thermal Equilibrium
hottest surface
30. Radiation given off by electrons accelerating in a magnetic field
Oort Cloud
Synchrotron Rotation
Galilean satellite
Electromagnetic Radiation: Gamma Ray
31. A distance measure determined by the shifting of a star against the background sky every 6 months.
Planetary Nebula
Turn off Point
Electromagnetic Radiation: X-Ray
Parsec
32. 1-orbit aroudn the sun 2- are in hydrostatic equilibrium and 'mostly round' 3- have not cleared debris around its orbit 4- are not satellites
Electromagnetic Radiation: Radio
Dwarf planets
Coldest surface
acceleration
33. A crystalline patter found in iron meteorites
Heliocentric
Jovian Planets
Apparent Magnitude
widmanstatten pattern
34. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
Halo
Triple Alpha rocess
If it is in a denser medium - such as glass - it will move slower
Coronal Loop
35. The wavelengths where a specific element can absorb or emit light.
synchrotron radiation
Gamma-ray Burst
Spectral Lines
accretion disk
36. Radiation emitted when charged particles spiral rapidly in a magnetic field. come off of jets from black holes.
Primary Mirror
Largest diameter
synchrotron radiation
Big Bang
37. A subatomic particle with a negative charge. It creates light.
Electron
Thermonuclear Fusion
Total Eclipse
Winter Solstice
38. The larger bodies that formed early in teh solar nebula that were chemically differentiated
Trojan asteroids
The Big Bang Theory
planetesimal
Stephen-Boltzman Law
39. Large nebula consisting of very cold gas and dust
How is winding dilemma solved?
critical density
Brown dwarf
Molecular Clouds
40. Matter that reveals itself only through its gravitational attraction
Light Gathering Power
Dark Matter
Secondary Mirror
highlands
41. The organization of clusters of galaxies into sheets and strings
Supercluster
Plague
homogeneous
solar nebula
42. Dark areas on the sun that are cooler than the surrounding photosphere
asteroid
Big Bang
Horizontal Branch Star
Sunspots
43. Jupiter
aurora
Electromagnetic Radiation: Infrared
most moons
highlands
44. Saying that the sky should not get dark at night because all lines of sight end on a star meaning that the night sky should be ablaze BUT the big bang - because the universe had a beginning - says that the sky gets dark because out in space - galaxie
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45. A plot of star absolute magnitude verses spectral type.
Electromagnetic Radiation: Microwave
Electromagnetic Radiation: Infrared
tectonics of Venus
H-are Diagram
46. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
Primary Mirror
Thermonuclear Fusion
highlands
Absolute Magnitude
47. The source of the force that is accelerating the expansion rate of the universe.
dark energy
radiation dominated universe
Neutron Star
comet
48. Sc galaxies where star formation and destruction is so rapid that supernova explosions are mainly responsible for compressing gas to create new stars.
self-propagating star formation
solar nebula
Parallax
conjunction
49. The 11 or 22 period on the sun durin which sunspots increase - decrease - change polarity - increase and decrease again.
self-propagating star formation
Sunspot cycle
Focal Plane
mass
50. A small round distribution of gas surrounding a dying star
Meridian
Maria
Planetary Nebula
Apparent Magnitude
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