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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. A measure of the ability of a telescope to see fine detail
The Big Bang Theory resolves Olber's Paradox
Resolving Power
Neutron Star
Eclipses of the Moons of Jupiter
2. A star that blows itself apart
Turn off Point
cosmological principle
Supernova (You can be my supernova girl)
Cepheid Variable
3. The seasonal shifting of a nearby star's position relative to more distant objects.
Energy Level
Parallax
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
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.
4. A telescope that uses mirrors to focus light
Grand design spirals
Dark Matter
Nebula
Reflector
5. 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 ________.
Supernova (You can be my supernova girl)
Flat - Flat
Inverse Square Law
Big Bang
6. The wavelengths where a specific element can absorb or emit light.
Terrestrial Planets
Spectral Lines
Coronal Loop
reflection star clusters
7. The nuclei of very distant galaxies. Likely a manifestation of supermassive black holes
Quasar
Ole Roemer
mare basalt
Main Sequence Stars
8. The material from which the solar system formed
cosmic singularity
dark energy
solar nebula
OB Associations
9. 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)
Light: travels like a wave - detected like a particle
Resolving Power
Callisto (Jupiter)
Neutron Star
10. The name for the only seriously considered theory of the universe.
Synchrotron Rotation
Lagrangian Razor
cosmological principle
Big Bang
11. The force of attraction between any two objects having mass
aurora
Disk
gravity
Electromagnetic Radiation: X-Ray
12. IO
MOONS: most geologically active
Horizontal Branch Star
smallest diameter
How is winding dilemma solved?
13. The temp at which a substance in the vacuum of space solidifies
Cosmic Microwave Background (CMB)
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
condensation temperature
cosmology
14. Venus
Asymptotic giant Branch Star
conjunction
Flare
Thickest atmosphere
15. The telescope configuration that has the focus placed at the back of the primary mirror
Umbra
Cassegrain Focus
radio lobe
Parsec
16. As open clusters age - they push gas away but dust remains this can reflect light giving the cluster a blue-ish color. also called reflection nebula
isotropic
reflection star clusters
Light: travels like a wave - detected like a particle
jovian
17. When the Sun is farthest north of the celestial equator (about June 22)
Summer Solstice
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.
partile horizon
Sc spiral galaxy
18. A volume of space where few - if any - galaxies are located
Void
comet
acceleration
Annular Eclipse
19. Centered on the Earth
Geocentric
quasar
Void
Planetary Nebula
20. The fate of the universe if it is closed. The universe expanding as much as possible and then retracting
Metals
Big Crunch
protostar
density parameter
21. Jupiter - Saturn - Uranus - Neptune
Thermal Equilibrium
Jovian Planets
Density Wave
Perihelion
22. The surface of the sun
Photosphere
Photon
Sa spiral galaxy
Bok Globule
23. The shadow area behind the Earth or Moon where the Sun is completely obscured.
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.
Triple Alpha rocess
critical density
Umbra
24. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
Radiative Diffusion
coma
radiation dominated universe
Thermal Equilibrium
25. The gap inthe outer portion of Saturn's A ring
E=mc2
Enke gap
H2 Regions
Penumbra
26. A highly variable galaxy nucleus of which BL Lac is one. Their light is highly energetic and their spectra are featureless. (face on)
Hubble law
blazar
radiant
Dark Matter
27. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
The Local Group
Big Bang
Interstellar Extinction
disk
28. A planet orbiting about a distant star
Roundest orbit
Extrasolar Planet
Oort cloud
Differential Rotation
29. The dark - relativley smooth areas on the moon; Latin for sea
Steady State Theory (Leads to Olber's Paradox)
Make up of the terrestrial planets
Maria
tectonics of Venus
30. A faint - remarkably uniform distribution of radiation in space
Cosmic Microwave Background
Extrasolar Planet
chemical differentiation
meteorite
31. Consists of old red stars in slow orbits that plunge through disk and bulge. about 1% are old - round globular clusters.
Olber's paradox
terrestrial planet
Halo
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.
32. The point in its orbit where a planet is nearest the sun
fastest rotation
Liquid metallic hydrogen
Open - flat - and closed.
Perihelion
33. 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.
MOONS: larger than mercury
nova
Winter Solstice
Turn off Point
34. In Ptolemy's geocentric solar system - the large circle on which a planet's epicycle moved around the Earth.
Spectroscopic parallax
Density Wave
Neutron Star
deferent
35. A point in the sky where meteors appear to come from during a shower
radiant
Plague
Electron
Electromagnetic Radiation: Radio
36. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
critical density
The Local Group
Electromagnetic Radiation
Ganymede (Jupiter)
37. 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)
Focal Length
matter dominated universe
Light Curve
Cosmic Microwave Background (CMB)
38. 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.
Cosmic Microwave Background (CMB)
Rich vs poor clusters
Objective Lens
Drake equation
39. The location of a supermassive black hole
Nucleus
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.
Population 1 vs Population 2 stars
40. A push or a pull
Electromagnetic Radiation: Ultraviolet Light
force
meteor shower
fewest moons
41. Is there water on the moon?
Yes - frozen at the poles- remains protected from the suns rays
Hubble constant
acceleration
Radiative Diffusion
42. First accurately measured the speed of light in a vacuum
Electromagnetic Radiation: Infrared
Ole Roemer
chemical differentiation
Ganymede (Jupiter)
43. Latin for 'cloud'. A word used to describe the collections of gas and dust in the Milky Way and other galaxies
Electromagnetic Radiation: Gamma Ray
Electromagnetic Radiation: Visible Light
Nebula
most eccentric orbit
44. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
MOONS: roundest shape
Instability strip
AGN
CCD
45. The place in the sky that the Earth's axis points toward (can be either north or south)
Degeneracy
Poor Cluster
Ganymede (Jupiter)
Colestial Pole
46. A bright area of higher temperature that often proceeds the formation of sunspots.
Plague
fewest moons
Dark matter candidates
terrestrial planet
47. The part of the Milky way that has on-going star formation
Disk
chemical differentiation
matter dominated universe
widmanstatten pattern
48. Any class of objects with a uniform luminosity used to determine distance.
molecular clouds
Apollo asteroids
standard candle
Autumnal Equinox
49. How is the Hubble Law consistent with an expanding universe?
quasar
Halo
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.
Chandrasekhar Limit
50. 100 nm 10 nm
Instability strip
Electromagnetic Radiation: Ultraviolet Light
density
Quasar