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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. 1μm 100 nm
Sidereal Day
Electromagnetic Radiation: Visible Light
Photosphere
Electromagnetic Radiation
2. The powdered stone fragments that make up the lunar 'soil'
Make up of the terrestrial planets
deferent
regolith
scarp
3. What do we think the actual fate of the universe will be and why do we think this?
force
Nova
Doppler Shift
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.
4. 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)
A family of radiant energy- includes light
general star population
planetesimal
Turn off Point
5. The north-south line passing directly overhead through the zenith.
Photometry
weight
Meridian
interstellar dust
6. A large - irregularly shaped rocky object orbiting the sun mostly between mars and jupiter. Left-over planetesimals
meteor shower
Electromagnetic Radiation: Gamma Ray
Ole Roemer
asteroid
7. 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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8. Orbit in Jupiters orbit
Parsec
contrast northern lowlands and the southern highlands of mars...
Trojan asteroids
Hubble law
9. A spectrum of light with energy at only a few wavelengths.
Metals
Emission Spectrum
Molecular Clouds
Apparent Magnitude
10. Infinitely long -> 10 cm
Electromagnetic Radiation: Radio
Liquid metallic hydrogen
Electromagnetic Radiation: Visible Light
Plank's Law
11. The organized effort to find life elsewhere in the universe. (Search for Extra-Terrestrial Intelligence)
Wein's Law
SETI
Light Curve
Titus-Bode Law
12. The rock that makes up the lunar highlands
anorthosite
Cepheid Variable
Hyashi track
Stephen-Boltzman Law
13. When the Sun is farthest south of the celestial equator (About December 22)
Winter Solstice
Electromagnetic Radiation
era of recombination
Supercluster
14. Electromagnetic Radiation
Astronomical Unit
Parsec
A family of radiant energy- includes light
mass
15. An element of a highly efficient - two-dimensional electronic light detector
planetary nebula
Pixel
Electromagnetic Radiation: Gamma Ray
Spectroscopic parallax
16. Dying large-mass stars lose their outer layers in a violent explosion creating large - chaotic remnants. these brighten like nova but are so much brighter and only occur ONCE PER STAR
Milky way Galaxy
Metals
supernova
SETI
17. The 11 or 22 period on the sun durin which sunspots increase - decrease - change polarity - increase and decrease again.
density
Sunspots
Ganymede (Jupiter)
Sunspot cycle
18. A measure of the seasonal shifting of a star's position against farther stars or galaxies. The closer the star - the greater is the angular distance it shifts. We use it to find distances to stars that are up to 1000 pc away.
Thickest atmosphere
great dark spots
Penumbra
Parallax
19. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
Flat - Flat
Occam's razor
molecular clouds
Callisto (Jupiter)
20. The state of having a balance between inward and outard pressures in a gas--the inward force from gravity is balanced by the outward force from heat.
Hydrostatic Equilibrium
Negative - Diverge - Less than 1
Thermal Equilibrium
Cassegrain Focus
21. Theory virtually demands that the geometry of the universe be ______. Results of measuring lumps in the cosmic background radiation indicate that the universe geometry is ________.
Density Wave
Synchrotron Rotation
Kuiper belt
Flat - Flat
22. Matter that reveals itself only through its gravitational attraction.
dark matter
Halo
Resolving Power
Molecular Clouds
23. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
Reflector
Gamma ray bursts
radiation dominated universe
Resolving Power
24. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
tectonics of Earth
Thickest atmosphere
Superior planets
Electromagnetic Radiation
25. 100 nm 10 nm
Thermal Equilibrium
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
Electromagnetic Radiation: Ultraviolet Light
Thermal Equilibrium
26. A perfect absorber and radiator of electromagnetic radiation.
great red spot
Astronomical Unit
Blackbody
The Big Bang Theory
27. When the Sun moves from south to north across the celestial equator (about March 21)
Quasar
Vernal Equinox
Electromagnetic Radiation: X-Ray
density waves
28. 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.
Sidereal Day
tectonics of Venus
Main Sequence
Plank's Law
29. The surface of the sun
H-are Diagram
MOONS: thickest atmosphere
Photosphere
Superior planets
30. A planet that is closer to the sun than the earth
quasar
inferior planets
cosmological red shift
Cosmological Principle
31. The equation that describes how matter equates with energy
H2 Regions
Blackbody Curve
E=mc2
Big Crunch
32. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
Electromagnetic Radiation
Neutron Star
Coldest surface
MOONS: larger than mercury
33. The shadow area behind the Earth or Moon where the Sun is completely obscured.
cosmological red shift
Meridian
Umbra
Electromagnetic Radiation: X-Ray
34. 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
Open - flat - and closed.
Instability strip
Oort Cloud
35. Extremely round - lots of liquid water - ice rafts on surface ACTIVE SURFACE
Europa (Jupiters moon)
Planetary Nebula
Kuiper belt
Liquid metallic hydrogen
36. Galaxies whose nuclei emit jets of materil at high speeds. material comes from supermassive black holes
Geocentric
Terrestrial Planets
Parallax
radio galaxy
37. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
Ionization
chondrite
opposition
roche limit
38. Ancient stream channels - flood planes - and sedimentary-type rock. Frozen water is found in the polar ice caps and in the soil.
solar nebula
chondrite
evidence of water on mars
Extrasolar Planet
39. A small and dim but hot star.
White Dwarf
Autumnal Equinox
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
Photometry
40. A particle of light.
Coldest surface
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.
Photon
MOONS: thickest atmosphere
41. Orbit in Jupiters orbit
Jupiters red spot
Trojan asteroids
Cosmological Principle
fewest moons
42. A collection of galaxies like the one the Milky Way belongs to
Poor Cluster
Sunspot cycle
We don't know. It might be but does not have to be.
Summer Solstice
43. When massive objects bend space and time enough to create multiple images of an object located behind them
Make up of the terrestrial planets
Gravitational Lens
The Local Group
Titus-Bode Law
44. What causes the zones and belts on jupiter and saturn?
Nucleus
belt
H2 Regions
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
45. The seasonal shifting of a nearby star's position relative to more distant objects.
Proton-proton chain
Inverse Square Law
Parallax
Light Curve
46. 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.
Turn off Point
chondrite
weight
Globular Cluster
47. A spinning neutron star
Neutron Star
3 reasons we orbit satellites to observe universe
Pulsar
meteorite
48. The organization of clusters of galaxies into sheets and strings
Dark matter candidates
Hubble constant
Bulge
Supercluster
49. A very dense - highly populated cluster of galaxies
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
Annular Eclipse
Io (jupiters moon)
Rich Cluster
50. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
Supernova (You can be my supernova girl)
Make up of the jovian planets
Coronal Loop
critical density