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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 technique using computer-controlled mirrors to sharpen images distorted by the atmosphere
cosmic fireball
retrograde motion
Active Optics
Parallax
2. Mercury
Electromagnetic Radiation
molecular clouds
matter dominated universe
smallest diameter
3. Elliptical orbits that come inside orbit of the Earth.
least dense
Main Sequence Stars
Apollo asteroids
Quasar
4. A highly variable galaxy nucleus of which BL Lac is one. Their light is highly energetic and their spectra are featureless. (face on)
blazar
Gravitational Lens
interstellar dust
Planetary Nebula
5. A word used in astronomy to describe all elements besides hydrogen and helium
A family of radiant energy- includes light
Metals
Synchrotron Rotation
Jupiters red spot
6. The rock that makes up the lunar highlands
anorthosite
Heliocentric
planetesimal
Electromagnetic Radiation: Ultraviolet Light
7. The process that powers the sun and hydrogen bombs
Thermonuclear Fusion
solar nebula
protostar
Supercluster
8. 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 _____.
Magnification
Atomic Number
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Flat - Remain Parallel - Exactly 1
9. A star that blows itself apart
Superior planets
Cepheid variables
Supernova (You can be my supernova girl)
Rich Cluster
10. 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.
Radiative Diffusion
tectonics of Earth
Nebula
Particle Horizon
11. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Hyashi track
Kirkwood gaps
Yes - frozen at the poles- remains protected from the suns rays
Spectroscopy
12. When the Sun moves from south to north across the celestial equator (about March 21)
Sunspots
Autumnal Equinox
Nebula
Vernal Equinox
13. The normal eastward movement of a planet against the background of hte distant stars.
Io (jupiters moon)
Focal Plane
direct motion
opposition
14. An energetic event taking place in the early universe
Coldest surface
Hubble law
Gamma-ray Burst
Ground State
15. A small and dim but hot star.
condensation temperature
Globular Cluster
White Dwarf
Cepheid Variable
16. A spinning neutron star
rotation curve = dark matter?
mare basalt
Ole Roemer
Pulsar
17. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
matter dominated universe
Bulge
Neutron Star
Wein's Law
18. The oldest part of the Milky Way
nucleus
blazar
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.
19. A spectrum of light with energy at only a few wavelengths.
contrast northern lowlands and the southern highlands of mars...
Electromagnetic Radiation: Radio
Emission Spectrum
Largest diameter
20. Sa - Sb galaxies where two magnificent arms wind their way from nucleus out in a symmetrical manner.
Grand design spirals
Asymptotic giant Branch Star
Light Pollution
High Velocity Stars
21. The apparent path of the Sun through the stars on the celestial sphere.
Ecliptic
Grand design spirals
anorthosite
Main Sequence Stars
22. Clouds of low density gas often found glowing faintly on either side of an AGN.
Population 1 vs Population 2 stars
radio lobe
Callisto (Jupiter)
Magnification
23. Arcs of increased mass concentration that slow stars and gas down as they orbit through which cause the formation of stars.
density waves
tectonics of Earth
direct motion
Proton-proton chain
24. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
radio lobe
shape and color of SPIRAL galaxies
Flat - Remain Parallel - Exactly 1
partile horizon
25. Jupiter
Absolute Magnitude
Secondary Mirror
Largest diameter
Stephen-Boltzman Law
26. 10^2 nm 10^7 nm
chondrite
Particle Horizon
Electromagnetic Radiation: Gamma Ray
Light: travels like a wave - detected like a particle
27. How is the Hubble Law consistent with an expanding universe?
density waves
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.
Color Index
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.
28. 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
Umbra
reflection star clusters
Sunspots
Liquid metallic hydrogen
29. A word meaning 'the same everywhere throughout.'
Sunspot cycle
Light-Year
Coronal Loop
homogeneous
30. Thick rigid crust - no longer has plate tectonics but still has convective hot spots that create earth-like volcanoes except that last for billions of years because of lack of tectonics.
tectonics of Earth
Vernal Equinox
tectonics of Mars
Sc spiral galaxy
31. The high- temperatature outer layer of the sun
Flare
Corona
Nucleus
Grand design spirals
32. Centered on the Earth
chemical differentiation
Spectral Lines
Geocentric
Make up of the terrestrial planets
33. Centered on the sun.
Most dense
quasar
Heliocentric
asteroid
34. A rock or iron specimen that has fallen from space
Chromosphere
meteorite
conjunction
shape and color of ELLIPTICAL galaxies
35. A star fusing hydrogen to helium in it's core
Synodic Day
Ganymede (Jupiter)
Main Sequence Stars
Electromagnetic Radiation: Visible Light
36. Venus
jovian
hottest surface
synchronous rotation
Plank's Law
37. Is space infinitely large?
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38. The shadow area behind the Earth or Moon where the Sun is completely obscured.
Umbra
tectonics of Venus
Oort Cloud
Open Cluster
39. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
most eccentric orbit
general star population
CNO Cycle
Io (jupiters moon)
40. In a CLOSED UNIVERSE - the curvature of space-time is _________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
Positive - Converge - Greater than 1
rotation curve = dark matter?
Precession
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
41. The most mass a white dwarf can have before collapsing to a neutron star
Chandrasekhar Limit
Cepheid variables
Synchrotron Rotation
High Velocity Stars
42. Flat disk with gas - dust - H2 regions - molecular clouds - dust young stars and remnants of old planetary nebula and supernova remnants. stars spin together with similar velocities called differential rotation
coma
disk
great dark spots
Quasar
43. A massive variable star used to find distances to the galaxies or clusters that contain them.
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
general star population
Cepheid Variable
Kirchhoff's Law
44. An element of a highly efficient - two-dimensional electronic light detector
Terrestrial Planets
Focal Length
Light Curve
Pixel
45. A measure of how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
disk
mass
Gamma-ray Burst
Wein's Law
46. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
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.
density
opposition
critical density
47. Elliptical orbits that come inside orbit of the Earth.
Continuous Spectrum
Apollo asteroids
interstellar dust
Resolving Power
48. The average distance between the Earth and the Sun (=1.5 x10^8km)
Astronomical Unit
matter dominated universe
Instability strip
Electromagnetic Radiation: Microwave
49. Mercury
comet
Blackbody Curve
Focal Length
smallest diameter
50. The normal eastward movement of a planet against the background of hte distant stars.
The Local Group
cosmological principle
direct motion
critical density