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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. Highlands: rocks are made of lighter anorthosite (similar to old earth rocks) Maria: rocks made of heavy mare basalt (volcanic rock) everywhere else is loose regolith created by meteoric impact.
Kirchhoff's Law
Light Gathering Power
difference between maria and highlands of the moon.
Horizontal Branch Star
2. Comglomerates of ice and rock that orbit the sun in highly elliptical paths
aurora
Electromagnetic Radiation: Infrared
weight
comet
3. In Ptolemy's geocentric solar system - the large circle on which a planet's epicycle moved around the Earth.
Resolving Power
Secondary Mirror
Sunspots
deferent
4. The apparent backward motion of a planet against the background of stars.
Electromagnetic Radiation: Microwave
retrograde motion
Spectroscopy
Neutron Star
5. The imaginary sphere centered on the Earth that hols the stars.
Celestial Sphere
H2 Regions
radiant
supermassive black hole
6. All possible types of energy that can be emitted and absorbed by atoms.
Oort cloud
Electromagnetic Radiation
mare basalt
Celestial Equator
7. When the Sun is farthest north of the celestial equator (about June 22)
aurora
Quasar
Summer Solstice
Main Sequence Stars
8. The rotation of a star or planet at different speeds at its equator and poles
Jupiters red spot
Resolving Power
gravity
differential rotation
9. Galaxies whose nuclei emit jets of materil at high speeds. material comes from supermassive black holes
radio galaxy
Oort Cloud
Photometry
Gamma-ray Burst
10. When massive objects bend space and time enough to create multiple images of an object located behind them
Gravitational Lens
Dark Matter
Kirkwood gaps
Poor Cluster
11. Saturn
planetary nebula
least dense
MOONS: most geologically active
shape and color of SPIRAL galaxies
12. A phenomenon seen when the Earth passes through the orbit of a burned out comet
Radio Galaxy
meteor shower
Kuiper belt
Parsec
13. How did Earth come to have an oxygen rich atmosphere?
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.
Red Giant Branch Star
zone
Flat - Remain Parallel - Exactly 1
14. A volume of space where few - if any - galaxies are located
Sidereal Day
Void
Halo
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
15. What Ole Roemer used to measure the speed of light in a vacuum
isotropic
tectonics of Earth
Dwarf planets
Eclipses of the Moons of Jupiter
16. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
Open Cluster
Supercluster
Limb darkening
rotation curve=winding dilemma?
17. The fusion process that turns three helium nuclei into a carbon nucleus
Sunspots
Triple Alpha rocess
planetary nebula
Extrasolar Planet
18. Old - pock marked - icy surface - interior is not differentiated - geologically dead - NOT ACTIVE SURFACE
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Radio Galaxy
Callisto (Jupiter)
least dense
19. 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.
MOONS: larger than mercury
CMB
scarp
Winter Solstice
20. 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
bulge
chemical differentiation
radio lobe
Cepheid variables
21. Electromagnetic Radiation
A family of radiant energy- includes light
Gamma ray bursts
coma
Most dense
22. A quantity measuring the stability of the Earth's atmosphere
homogeneous
Planck time
Red Giant Branch Star
Seeing
23. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
Supercluster
Neutron Star
condensation temperature
H-are Diagram
24. 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
tectonics of Earth
Thermal Equilibrium
Cepheid variables
superclusters
25. The amount an image is enlarged by a telescope
force
Light Pollution
Open - flat - and closed.
Magnification
26. A location on an H-are Diagram where evolving stars pulsate
Instability strip
Yes - frozen at the poles- remains protected from the suns rays
Cepheid Variable
disk
27. The distance a moon can be from a planet before shattering from tidal forces
matter dominated universe
roche limit
meteoriod
regolith
28. A faint - remarkably uniform distribution of radiation in space
CNO Cycle
Hyashi track
Cosmic Microwave Background
Europa (Jupiters moon)
29. 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.
neutrino
meteoriod
Population 1 vs Population 2 stars
weight
30. Is there water on the moon?
most moons
Terrestrial Planets
Yes - frozen at the poles- remains protected from the suns rays
great red spot
31. An evolved star - past the helium flash that is burning helium to carbon in it's cores
Sa spiral galaxy
Apparent Magnitude
Radiative Diffusion
Horizontal Branch Star
32. An entity that is likely in the nucleus of most - if not all - galaxies.
Electron
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.
supermassive black hole
Electromagnetic Radiation: Infrared
33. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
The Big Bang Theory resolves Olber's Paradox
Electromagnetic Radiation: Radio
Secondary Mirror
CCD
34. A point in the sky where meteors appear to come from during a shower
Winter Solstice
synchronous rotation
Roundest orbit
radiant
35. When a planet lines up with the sun inthe sky
conjunction
Void
Electron
bulge
36. A bright area of higher temperature that often proceeds the formation of sunspots.
Enke gap
Electromagnetic Radiation: Radio
Neutron Star
Plague
37. A collection of galaxies like the one the Milky Way belongs to
Halo
radio lobe
Maria
Poor Cluster
38. The distance between a lens and its focal plane
Hipparchus
Blackbody Curve
CNO Cycle
Focal Length
39. A particle of light.
Sa spiral galaxy
Halo
Photon
300000 KM/sec
40. Venus
Roundest orbit
fusion crust
OB Associations
fastest rotation
41. The trapping of heat by carbon dioxide or other gases in the Earth's atmosphere.
direct motion
Open - flat - and closed.
Cassini division
greehouse effects
42. Is space infinitely large?
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43. Elliptical orbits that come inside orbit of the Earth.
open star clusters
Heliocentric
Apollo asteroids
radiant
44. When the Sun is farthest north of the celestial equator (about June 22)
radio galaxy
Summer Solstice
Electromagnetic Radiation
Celestial Equator
45. The process responsible for creating the arms of flocculent spiral galaxies
Radiative Diffusion
mare basalt
Self-Propogating Star Formation
Asymptotic giant Branch Star
46. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
The Local Group
Cosmological Principle
Big Bang
force
47. Consists of old red stars in slow orbits that plunge through disk and bulge. about 1% are old - round globular clusters.
Hubble constant
fusion crust
Halo
MOONS: largest size
48. Formed from slow rotating clouds - collapsed quicker - initial star formation rate is high but died out - older - little rotation - look redder
Open Cluster
Yes - frozen at the poles- remains protected from the suns rays
radio galaxy
shape and color of ELLIPTICAL galaxies
49. IO
Black Hole
Metals
Vernal Equinox
MOONS: most geologically active
50. A technique using computer-controlled mirrors to sharpen images distorted by the atmosphere
meteorite
Absolute Magnitude
Active Optics
Flat - Flat