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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. 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 _____.
Flat - Remain Parallel - Exactly 1
rotation curve = dark matter?
Black Hole
inferior planets
2. Centered on the Earth
protostar
Parallax
Geocentric
Rich vs poor clusters
3. A word meaning 'the same in all directions.'
Autumnal Equinox
Active Optics
radio lobe
isotropic
4. A prominence seen against the disk of the sun
We don't know. It might be but does not have to be.
Roundest orbit
standard candle
Filament
5. How did Earth come to have an oxygen rich atmosphere?
inferior planets
Corona
cosmic singularity
Biologicla life created the recycling of nitrogen - co2 - and the production of oxygen. Oxygen is heavier so the atmosphere held onto it easier than hydrogen and helium.
6. A spectrum of light with energy at only a few wavelengths.
quasar
Red Giant Branch Star
Cepheid Variable
Emission Spectrum
7. A force exerted by reflecting sunlight
radiation pressure
Radio Galaxy
Roundest orbit
Radiative Diffusion
8. A force exerted by reflecting sunlight
Largest diameter
radiation pressure
terrestrial planet
Sb spiral galaxy
9. 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.
hottest surface
least dense
self-propagating star formation
Cosmic Microwave Background (CMB)
10. The location in an H-are diagram of a star cluster - where stars have just left the main sequence. Used to estimate the cluster age.
If it is in a denser medium - such as glass - it will move slower
Molecular Clouds
Black Hole
Turn off Point
11. The nuclei of very distant galaxies. Likely a manifestation of supermassive black holes
Prominence
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Quasar
dark energy
12. 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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13. The lens in a telescope used to determine the magnification
Cassini division
Wein's Law
fewest moons
Eyepiece Lens
14. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
Callisto (Jupiter)
Spectroscopic Parallax
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
accretion disk
15. A term referring to the orbital character of stars near the Sun
Terrestrial Planets
meteor
Differential Rotation
Dark matter candidates
16. Jupiter
fastest rotation
planetesimal
solar nebula
hottest surface
17. When massive objects bend space and time enough to create multiple images of an object located behind them
Light: travels like a wave - detected like a particle
Electromagnetic Radiation: X-Ray
Ground State
Gravitational Lens
18. A spectrum of light with energy at only a few wavelengths.
terrestrial planet
fewest moons
Emission Spectrum
Positive - Converge - Greater than 1
19. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Sc spiral galaxy
Winter Solstice
synchrotron radiation
regolith
20. The amount an image is enlarged by a telescope
Magnification
Turn off Point
Electromagnetic Radiation
dark energy
21. A planet that is closer to the sun than the earth
Eyepiece Lens
inferior planets
Instability strip
protostar
22. The universe is isotropic - homogeneous - and without beginning or end in time and space. If the universe is truly homogeneous then every line of sight will eventually end on a galaxy. If it has existed forever then there has been enough time for lig
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23. Light scattered through the atmosphere that degrades astronomical images
Light Pollution
Gravitational Lens
Convection
Secondary Mirror
24. The oldest terrain on the moon
Poor Cluster
Ionization
highlands
Make up of the jovian planets
25. The location in the Milky Way where stars orbit like a solid wheel
Convection
fusion crust
Bulge
Cepheid Variable
26. A faint - remarkably uniform distribution of radiation in space
Cosmic Microwave Background
Photon
Primary Mirror
Particle Horizon
27. A spread of light with an uninterrupted wavelength distribution of energy.
highlands
Continuous Spectrum
Olber's paradox
Coronal Loop
28. The elementary building blocks from which protons and neutrons are formed.
quarks
Light: travels like a wave - detected like a particle
difference between maria and highlands of the moon.
Lagrangian Razor
29. 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.
highlands
nova
Callisto (Jupiter)
Ganymede (Jupiter)
30. 1μm 100 nm
Sa spiral galaxy
Main Sequence Stars
Electromagnetic Radiation: Visible Light
Jupiters red spot
31. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
Spectroscopy
gravity
Absolute Magnitude
Jovian Planets
32. The source of the force that is accelerating the expansion rate of the universe.
Meridian
Largest diameter
Gamma ray bursts
dark energy
33. How is the Hubble Law consistent with an expanding universe?
nova
Photometry
Gamma ray bursts
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.
34. What Ole Roemer used to measure the speed of light in a vacuum
Eclipses of the Moons of Jupiter
Oort Cloud
Terrestrial Planets
rotation curve = dark matter?
35. The process similar to conduction by which energy moves from the solar core to the convective layer
Radiative Diffusion
Self-Propogating Star Formation
Supernova (You can be my supernova girl)
deferent
36. Population 1 with higher metals and contain many young stars in star clusters. Distribution of stars is everywhere in disk (arms only have 5% more stars)
Geocentric
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.
general star population
superclusters
37. 10 nm 10^2 nm
Electromagnetic Radiation: X-Ray
hottest surface
Eclipses of the Moons of Jupiter
Flat - Flat
38. The location of a supermassive black hole
Proton-proton chain
High Velocity Stars
Nucleus
Focal Length
39. A change in the appearance of the sun at the edge of the solar disk
Occam's razor
Celestial Equator
nucleus
Limb darkening
40. A star that blows itself apart
rotation curve = dark matter?
H2 Regions
Supernova (You can be my supernova girl)
Objective Lens
41. Venus (retrograde)
Flat - Flat
slowest rotation
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
The Big Bang Theory
42. The displacement of spectral lines to redder colors caused by the expansion of the universe.
cosmological red shift
coma
Supernova (You can be my supernova girl)
Nucleus
43. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
Total Eclipse
Photometry
mapping the structure of Milky Way disk
Celestial Equator
44. The 11 or 22 period on the sun durin which sunspots increase - decrease - change polarity - increase and decrease again.
Celestial Sphere
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Apollo asteroids
Sunspot cycle
45. The assumption that the universe is isotropic (same in all directions) and homogeneous (Same everywhere throughout)
cosmological principle
reflection star clusters
Neutron Star
Flat - Flat
46. When a planet lines up with the sun inthe sky
HII Region
Terrestrial Planets
Color Index
conjunction
47. Sulfurous volcanoes - pools of liquid sulfur - surface resembles cheese pizza ACTIVE SURFACE
conjunction
OB Associations
Io (jupiters moon)
If it is in a denser medium - such as glass - it will move slower
48. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
opposition
Roundest orbit
Doppler Shift
meteorite
49. That which is responsible for Jupiter's magnetic field
Supercluster
reflection star clusters
Liquid metallic hydrogen
Light Gathering Power
50. The point where an inferior planet is as far away from the sun as it can be (as seen from the Earth)
Granules
Globular Cluster
greatest elongation
Neutron Star