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Test your basic knowledge |
Cosmology
Start Test
Study First
Subject
:
science
Instructions:
Answer 50 questions in 15 minutes.
If you are not ready to take this test, you can
study here
.
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 gap inthe outer portion of Saturn's A ring
Spectroscopic parallax
Geocentric
Atomic Number
Enke gap
2. Venus
Thickest atmosphere
rotation curve=winding dilemma?
mare basalt
Population 1 vs Population 2 stars
3. The rotation period of the Earth measured relative to the Sun.
Synodic Day
Most dense
open star clusters
H-are Diagram
4. 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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5. Dark areas on the sun that are cooler than the surrounding photosphere
solar nebula
Seeing
MOONS: thickest atmosphere
Sunspots
6. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
semimajor axis
Red Giant Branch Star
Energy Level
3 reasons we orbit satellites to observe universe
7. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Main Sequence
aurora
Hubble constant
300000 KM/sec
8. Extends to a distance of 50000AU. Same objects as in the Kuiper belt-when they fall in toward the sun they become comets. Debris from comets hitting the Earths atmosphere cause meteor showers.
Coldest surface
tectonics of Mars
Oort Cloud
Astronomical Unit
9. The law that predicts the possible types of spectra.
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10. A measure of the force of gravity on an object
weight
Enke gap
dark matter
contrast northern lowlands and the southern highlands of mars...
11. 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 _____.
Metals
general star population
Flat - Remain Parallel - Exactly 1
density
12. Extends to a distance of 50000AU. Same objects as in the Kuiper belt-when they fall in toward the sun they become comets. Debris from comets hitting the Earths atmosphere cause meteor showers.
Oort Cloud
Molecular Clouds
era of recombination
Continuous Spectrum
13. The measure of a variable star's apparent magnitude as it brightens and dims with time
Light Curve
accretion disk
Planck time
most moons
14. A continuous spectrum of light missing energy at a few wave lengths.
chemical differentiation
Absolute Magnitude
Kuiper belt
Absorption Spectrum
15. 30AU to 50Au from sun - consists of ancietn premordial objects made of frozen ice and dust-35000 objects or more that are larger than 100 km in diameter and many more smaller than this
accretion
Electromagnetic Radiation: Gamma Ray
Kuiper belt
Pulsar
16. A term referring to Jupiter-like planets
Pulsar
3 reasons we orbit satellites to observe universe
Molecular Clouds
jovian
17. Large bulge - tightly wound spiral arms - relatively few h2 regions and are smooth
Photon
isotropic
Sa spiral galaxy
Dark matter candidates
18. The 'edge' of the universe. Light beyond this has not reached us yet.
Rich vs poor clusters
It does not have to expand into anything. It might just be that the 3 dimensions of space are getting bigger. It may also be that our 3 spatial dimensions are expanding into higher dimensions if such things exist.
Thermal Equilibrium
partile horizon
19. The Big Bang says that the universe has not existed forever. It had a distinct beginning about 14 billion years ago called the 'Big Bang'. Therefore light from any object more than 14 billion light years away has not had time to reach us. The other p
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20. What do we think the actual fate of the universe will be and why do we think this?
Winter Solstice
Superior planets
planetesimal
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.
21. 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.
Population 1 vs Population 2 stars
Nova
Void
Halo
22. Venus (retrograde)
Halo
slowest rotation
OB Associations
nova
23. An important quality of telescopes that increases as the square of the primary mirror or objective lens
Chandrasekhar Limit
Ammonia - methane - and water
Light Gathering Power
aurora
24. Clouds of low density gas often found glowing faintly on either side of an AGN.
radio lobe
Geocentric
Differential Rotation
radiation pressure
25. The fusion process that turns three helium nuclei into a carbon nucleus
Triple Alpha rocess
rotation curve=winding dilemma?
Photon
Synchrotron Rotation
26. 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
Dwarf planets
MOONS: larger than mercury
roche limit
MOONS: roundest shape
27. Hot cells of gas that rise and fall in the hotosphere
Objective Lens
MOONS: larger than mercury
Granules
Open Cluster
28. The dark - relativley smooth areas on the moon; Latin for sea
self-propagating star formation
Maria
solar nebula
A family of radiant energy- includes light
29. Venus
synchronous rotation
Hyashi track
Halo
Thickest atmosphere
30. The apparent backward motion of a planet against the background of stars.
Occam's razor
retrograde motion
Steady State Theory (Leads to Olber's Paradox)
zone
31. Possible Fates of the Universe
conjunction
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
The Big Bang Theory resolves Olber's Paradox
Resolving Power
32. Young clusters in disk are irregularly shaped since they have no time to relax into the rounder relaxed shape of globular clusters-will constantly be torn apart and assimilated.
Most dense
open star clusters
most eccentric orbit
Kirchhoff's Law
33. Massive compact halo objects (MACHO) - weakly interacting massive particles (WIMPY's)
Ground State
Clouds of sufuric acid (very inhospitable and brightest object in the sky) - process called greenhouse affect traps radiation making it 900 degrees at times - spins with retrograde rotation (sun rises in west) and takes 58.4 days for it to set. Thick
tectonics of Mars
Dark matter candidates
34. Hydrogen and helium (mainly)
Filament
anorthosite
Make up of the jovian planets
density parameter
35. Venus
We don't know. It might be but does not have to be.
Roundest orbit
force
isotropic
36. The mirror that gathers the light in a reflector
self-propagating star formation
asteroid
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
Primary Mirror
37. Rich= dense crowded cores of galaxies - poor= few members and a looser organization of galaxies
Rich vs poor clusters
isotropic
Coldest surface
synchrotron radiation
38. The imaginary sphere centered on the Earth that hols the stars.
Celestial Sphere
Red Giant
Umbra
Roundest orbit
39. Ganymede and Titan
isotropic
Light: travels like a wave - detected like a particle
MOONS: larger than mercury
Absolute Magnitude
40. A star that is burning hydrogen to helium in a shell surrounding it's core
AGN
Red Giant Branch Star
Rich Cluster
Supernova (You can be my supernova girl)
41. The cosmological principle is the assumption that the universe is isotropic and homogeneous.The Big Bang assumes it to be a correct principle so that what we observe is exactly like What is too far away to be observed.
Seeing
Objective Lens
Proton-proton chain
Cosmological Principle
42. The relation that tells how light dims with distance.
Inverse Square Law
rotation curve=winding dilemma?
Spectroscopy
Occam's razor
43. Form honeycomb like patterns surrounding empty or nearly empty voids.
superclusters
cosmological red shift
tectonics of Earth
Umbra
44. A small chunk of rock in space
Colestial Pole
planetesimal
Cassini division
meteoriod
45. The family of radiant energy that includes light as a subset
Electromagnetic Radiation
Triple Alpha rocess
quasar
Absolute Magnitude
46. The force of attraction between any two objects having mass
radiation dominated universe
gravity
Umbra
Extrasolar Planet
47. A change in the appearance of the sun at the edge of the solar disk
Limb darkening
jovian
Void
Hyashi track
48. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
Oort cloud
Olber's paradox
disk
The Big Bang Theory
49. Is space infinitely large?
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50. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
Dark Nebula
slowest rotation
tectonics of Earth
coma
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