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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 'edge' of the universe. Light beyond this has not reached us yet.
planetary nebula
scarp
Blackbody
partile horizon
2. The part of the Milky way that has on-going star formation
Sunspot cycle
tectonics of Mars
Disk
radio lobe
3. Sulfurous volcanoes - pools of liquid sulfur - surface resembles cheese pizza ACTIVE SURFACE
H2 Regions
Nucleus
Io (jupiters moon)
Cosmic Microwave Background (CMB)
4. A long-lived high-pressure bulge in Jupiter's southern hemisphere
Jovian Planets
great red spot
Trojan asteroids
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
5. Hot cells of gas that rise and fall in the hotosphere
Yes - frozen at the poles- remains protected from the suns rays
Meridian
difference between maria and highlands of the moon.
Granules
6. A star that is in the process of forming. It glows from gravitational contraction
protostar
The Big Bang Theory
Big Crunch
Precession
7. What do we think the actual fate of the universe will be and why do we think this?
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.
Pulsar
radio galaxy
weight
8. The layer of the sun just above the photosphere
Cosmological Principle
Coldest surface
Chromosphere
accretion disk
9. Earth
Secondary Mirror
Thickest atmosphere
CMB
Most dense
10. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
Hipparchus
accretion disk
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
If it is in a denser medium - such as glass - it will move slower
11. The particle horizon is the farthest we can see. It exists because the universe had a beginning and thus a definite age. Light from distances farther away from the particle horizon have not had time to reach us yet.
force
Particle Horizon
meteor
solar nebula
12. A spectrum of light with energy at only a few wavelengths.
Parallax
Parallax
Dwarf planets
Emission Spectrum
13. Wave- only waves cause an interference pattern when passing through a double slit - particle- only particles deposit energy at specific locations (the way an image builds up on digital camera)
Pulsar
Light: travels like a wave - detected like a particle
MOONS: largest size
meteorite
14. 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 _____.
OB Associations
Flat - Remain Parallel - Exactly 1
Terrestrial Planets
Sunspot cycle
15. The process that powers the sun and hydrogen bombs
Thermonuclear Fusion
bulge
We don't know. It might be but does not have to be.
Cassini division
16. What Ole Roemer used to measure the speed of light in a vacuum
Instability strip
Autumnal Equinox
Eclipses of the Moons of Jupiter
fastest rotation
17. Hot cells of gas that rise and fall in the hotosphere
Granules
Geocentric
scarp
Celestial Sphere
18. Centered on the sun.
radiation dominated universe
Astronomical Unit
Heliocentric
Ionization
19. A quantity measuring the stability of the Earth's atmosphere
Seeing
contrast northern lowlands and the southern highlands of mars...
Colestial Pole
Globular Cluster
20. The process of acquiring material
most moons
supermassive black hole
radio lobe
accretion
21. The family of radiant energy that includes light as a subset
zone
Electromagnetic Radiation
homogeneous
Electromagnetic Radiation: X-Ray
22. The location of a supermassive black hole
Largest diameter
Nucleus
Refractor
Big Bang
23. The era when the ratio of matter to energy greatly favored matter. (verses radiation dominated universe where it was opaque. Matter is now dominated by gravity not photons)
Cosmological Principle
matter dominated universe
Jupiters red spot
Corona
24. A location on an H-are Diagram where evolving stars pulsate
AGN
Rich Cluster
Instability strip
Ole Roemer
25. The process similar to conduction by which energy moves from the solar core to the convective layer
Radiative Diffusion
highlands
Apparent Magnitude
Doppler Shift
26. The dark - relativley smooth areas on the moon; Latin for sea
Metals
Precession
Hyashi track
Maria
27. The process responsible for creating the arms of flocculent spiral galaxies
Light Gathering Power
difference between maria and highlands of the moon.
Self-Propogating Star Formation
great dark spots
28. Sa - Sb galaxies where two magnificent arms wind their way from nucleus out in a symmetrical manner.
We don't know. It might be but does not have to be.
Grand design spirals
Refractor
Photosphere
29. 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
reflection star clusters
Flat - Remain Parallel - Exactly 1
Kirchhoff's Law
Kuiper belt
30. A high-pressure bulge in Neptune's southern hemisphere
Self-Propogating Star Formation
great dark spots
Light Pollution
Zenith
31. Venus
Thickest atmosphere
most moons
Spectral Lines
tectonics of Venus
32. A star that erratically and explosively brightens and dims
Cosmic Microwave Background (CMB)
widmanstatten pattern
Nova
terrestrial planet
33. The mass of an object divided by its volume
Supernova (You can be my supernova girl)
density
most moons
H2 Regions
34. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
CNO Cycle
Europa (Jupiters moon)
Absolute Magnitude
Differential Rotation
35. 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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36. A small spherical dark nebula
Quasar
Bok Globule
Interstellar Extinction
Brown dwarf
37. A rock or iron specimen that has fallen from space
meteorite
MOONS: largest size
hottest surface
Light Gathering Power
38. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
Emission Spectrum
Coldest surface
Olber's paradox
epicycle
39. Light-flaky crust - convective currents cause it to wrinkle and bunch (1/5 of surface). uniform cratering suggests lack of weathering and tectonics. volcanoes are flat due to atmospheric pressure.
tectonics of Venus
Disk
Open Cluster
neutrino
40. A planet orbiting about a distant star
Extrasolar Planet
Molecular Clouds
aphelion
Bulge
41. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
dark energy
Photometry
Astronomical Unit
Extrasolar Planet
42. The process that powers the sun and hydrogen bombs
highlands
slowest rotation
Thermonuclear Fusion
Hipparchus
43. The average distance between the Earth and the Sun (=1.5 x10^8km)
Seeing
300000 KM/sec
Sunspots
Astronomical Unit
44. A spread of light with an uninterrupted wavelength distribution of energy.
Seyfert galaxy
MOONS: largest size
Hyashi track
Continuous Spectrum
45. What are the three possible geometries of the universe?
Superior planets
Open - flat - and closed.
Light Gathering Power
neutrino
46. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Corona
mare basalt
Kirkwood gaps
Seeing
47. We can infer the absolute magnitude of pulsating variable stars by measuring their pulsation periods. The longer the pulsations - the greater their luminosities. We then again measure their apparent magnitudes - compare it with their absolute magnitu
Cepheid variables
Light Curve
High Velocity Stars
Red Giant
48. A small chunk of rock in space
Stephen-Boltzman Law
meteoriod
Annular Eclipse
Umbra
49. A planet that is farther from the sun than the Earth is
Cepheid variables
Superior planets
Galilean satellite
Molecular Clouds
50. A distance measure determined by the shifting of a star against the background sky every 6 months.
Umbra
Cassini division
Bok Globule
Parsec
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