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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. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
Flat - Flat
tectonics of Earth
Negative - Diverge - Less than 1
CMB
2. A faint - remarkably uniform distribution of radiation in space
cosmic singularity
Blackbody
Olber's paradox
Cosmic Microwave Background
3. A measure of how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
dark energy
differential rotation
mass
general star population
4. The point where an inferior planet is as far away from the sun as it can be (as seen from the Earth)
greatest elongation
density waves
most eccentric orbit
Light: travels like a wave - detected like a particle
5. The rate of expansion of the universe.
Density Wave
Annular Eclipse
cosmic fireball
Hubble constant
6. Consists of old red stars in slow orbits that plunge through disk and bulge. about 1% are old - round globular clusters.
Planck time
Sunspot cycle
accretion
Halo
7. A small round distribution of gas surrounding a dying star
Planetary Nebula
Focal Plane
Asymptotic giant Branch Star
Open Cluster
8. Jupiter
critical density
Europa (Jupiters moon)
fastest rotation
Umbra
9. In a FLAT UNIVERSE(our universe) - the curvature of space-time is ________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
Spectroscopic parallax
Focal Plane
In an expanding universe all galaxies see all other galaxies that are not gravitationally bound to them receding away. This is what we see in the Hubble Law. We infer that the Hubble law also holds true for all other galaxies.
Flat - Remain Parallel - Exactly 1
10. A collection of galaxies like the one the Milky Way belongs to
White Dwarf
Poor Cluster
Inverse Square Law
Continuous Spectrum
11. A star fusing hydrogen to helium in it's core
Triple Alpha rocess
radiant
Main Sequence Stars
Open Cluster
12. Radiation (possibly left over from the big bang) that fills the universe. Perfect black body spectrum and tells us a bit aout how galaxies are formed.
Cosmic Microwave Background (CMB)
MOONS: thickest atmosphere
Penumbra
acceleration
13. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
MOONS: largest size
Most dense
blazar
critical density
14. The process that powers the sun and hydrogen bombs
density parameter
Ionization
Thermonuclear Fusion
Globular Cluster
15. A massive variable star used to find distances to the galaxies or clusters that contain them.
H-are Diagram
meteoriod
coma
Cepheid Variable
16. The mirror that determines the focus configuration of a reflector
Objective Lens
Europa (Jupiters moon)
Population 1 vs Population 2 stars
Secondary Mirror
17. The shadow behind the Earth or Moon where the Sun is partially obscured.
Void
retrograde motion
Filament
Penumbra
18. A particle of light
dark matter
Black Hole
resonance
Photon
19. 10 cm -> 1 mm
Electromagnetic Radiation: Microwave
Hubble constant
quarks
Total Eclipse
20. The powdered stone fragments that make up the lunar 'soil'
cosmological principle
Bulge
cosmology
regolith
21. A large and bright but cool star.
greehouse effects
Seeing
Kuiper belt
Red Giant
22. Arcs of increased mass concentration that slow stars and gas down as they orbit through which cause the formation of stars.
Globular Cluster
density waves
highlands
Filament
23. Flattened spherical distribution of old stars with some young stars too. 'hub' of Milky way - stars orbit with solid body speeds. Elongated into bar shape
bulge
Nucleus
most eccentric orbit
direct motion
24. Is space infinitely large?
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25. When particles are compressed to an unnatural state where their pressure is not related to their temperature
Degeneracy
Celestial Sphere
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
general star population
26. After stars form they pump light energy into surrounding gas causing it to heat up and glow (H2=ionized hydrogen - H1= neutral hydrogen in molcular couds)
Maria
The Big Bang Theory resolves Olber's Paradox
H2 Regions
Ammonia - methane - and water
27. What causes the zones and belts on jupiter and saturn?
Flat - Flat
High and low pressure which stretch into bands due to the rapid differential rotation. deeper - darker colors are in the belts and zones are lighter
Instability strip
meteoriod
28. 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.
Kirkwood gaps
Oort cloud
CMB
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
29. Electromagnetic Radiation
A family of radiant energy- includes light
planetary nebula
fastest rotation
Black Hole
30. Venus (retrograde)
slowest rotation
radiation pressure
Open - flat - and closed.
Hyashi track
31. A two-filter measure of the color - and hence temperature - of a star.
Nucleus
Color Index
3 reasons we orbit satellites to observe universe
Energy Level
32. In a CLOSED UNIVERSE - the curvature of space-time is _________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
Spectroscopy
Doppler Shift
Vernal Equinox
Positive - Converge - Greater than 1
33. What do we think the actual fate of the universe will be and why do we think this?
Spectroscopic Parallax
Total Eclipse
Steady State Theory (Leads to Olber's Paradox)
Observations of distant type Ia supernovae indicate that the expansion of the universe is speeding up with time - not slowing down! So there must be a force causing this.
34. Radiation given off by electrons accelerating in a magnetic field
CMB
Magnification
reflection star clusters
Synchrotron Rotation
35. Jupiter
density
Ground State
mass
fastest rotation
36. A bridge of material held in position above the solar surface. They can remain for hours even days
Metals
Atomic Number
Prominence
standard candle
37. All wavelengths of light emitted by a blackbody.
Globular Cluster
Nebula
Autumnal Equinox
Blackbody Curve
38. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Kirkwood gaps
Total Eclipse
Rich vs poor clusters
Summer Solstice
39. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
MOONS: roundest shape
hottest surface
Perihelion
Absolute Magnitude
40. The normal eastward movement of a planet against the background of hte distant stars.
Thermonuclear Fusion
direct motion
3 reasons we orbit satellites to observe universe
Ecliptic
41. What do we think the actual fate of the universe will be and why do we think this?
fastest rotation
Total Eclipse
Ole Roemer
Observations of distant type Ia supernovae indicate that the expansion of the universe is speeding up with time - not slowing down! So there must be a force causing this.
42. Sc galaxies
Flocculent spirals
most eccentric orbit
Celestial Sphere
gravity
43. A galaxy sending out a stream of material from its nucleus
Radio Galaxy
Parsec
Electromagnetic Radiation: Infrared
E=mc2
44. The assumption that the universe is isotropic (same in all directions) and homogeneous (Same everywhere throughout)
cosmological principle
Light Gathering Power
Olber's paradox
Gravitational Lens
45. A perfect absorber and radiator of electromagnetic radiation.
Blackbody
era of recombination
MOONS: roundest shape
Big Bang
46. The class of all objects having high energy radiation coming from their nuclei. Active Galactic Nucleus- Blazars - Quasars - Radio and Emit synchrotron radiation
Plague
Triple Alpha rocess
cosmology
AGN
47. Extremely round - lots of liquid water - ice rafts on surface ACTIVE SURFACE
Europa (Jupiters moon)
Milky way Galaxy
AGN
Turn off Point
48. A plot of star absolute magnitude verses spectral type.
least dense
density
H-are Diagram
Ionization
49. Form honeycomb like patterns surrounding empty or nearly empty voids.
Penumbra
superclusters
Shepherd satellite
Sunspots
50. First accurately measured the speed of light in a vacuum
Ammonia - methane - and water
Largest diameter
Photon
Ole Roemer
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