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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 larger bodies that formed early in teh solar nebula that were chemically differentiated
Big Crunch
MOONS: roundest shape
deferent
planetesimal
2. The entity responsible for spiral arms in grand-design spiral galaxies
regolith
Void
Hipparchus
Density Wave
3. A technique using computer-controlled mirrors to sharpen images distorted by the atmosphere
protostar
most eccentric orbit
Drake equation
Active Optics
4. The elementary building blocks from which protons and neutrons are formed.
High Velocity Stars
quarks
comet
Halo
5. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
tectonics of Venus
neutrino
Open - flat - and closed.
Absolute Magnitude
6. The process similar to conduction by which energy moves from the solar core to the convective layer
isotropic
radiant
comet
Radiative Diffusion
7. Long - meandering cliff formed when a planet surface cools and shrinks
hottest surface
Light: travels like a wave - detected like a particle
Corona
scarp
8. 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.
Instability strip
MOONS: larger than mercury
Photon
Turn off Point
9. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
Galilean satellite
Neutron Star
Black Hole
Meridian
10. That which is responsible for Jupiter's magnetic field
Liquid metallic hydrogen
Celestial Equator
Halo
Electromagnetic Radiation: Visible Light
11. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
roche limit
Olber's paradox
Titus-Bode Law
Neutron Star
12. Hurricane-like vortex in southern-hemisphere winds to north and south blow in opposite directions which keep it spinning and with no subsurface features like mountians it persists.
Trojan asteroids
Jupiters red spot
H2 Regions
Wein's Law
13. A highly variable galaxy nucleus of which BL Lac is one. Their light is highly energetic and their spectra are featureless. (face on)
blazar
Electromagnetic Radiation: X-Ray
Apparent Magnitude
Milky way Galaxy
14. Centered on the Earth
Instability strip
Sc spiral galaxy
Geocentric
Zenith
15. Very center of galaxy. suggestion of a black hole
fusion crust
Nebula
nucleus
A family of radiant energy- includes light
16. The powdered stone fragments that make up the lunar 'soil'
Gravitational Lens
Cosmic Microwave Background (CMB)
Dark Nebula
regolith
17. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
great red spot
accretion disk
Hydrostatic Equilibrium
gravity
18. A particle of light
Turn off Point
Photon
The Big Bang Theory
Apollo asteroids
19. When the Moon entirely blocks the Sun.
weight
Maria
most eccentric orbit
Total Eclipse
20. The 'edge' of the universe. Light beyond this has not reached us yet.
Brown dwarf
SETI
partile horizon
Radio Galaxy
21. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Main Sequence
shape and color of SPIRAL galaxies
Supernova (You can be my supernova girl)
300000 KM/sec
22. The equation that describes how matter equates with energy
Pulsar
rotation curve=winding dilemma?
Objective Lens
E=mc2
23. 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
standard candle
thinnest atmosphere
reflection star clusters
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
24. The imaginary sphere centered on the Earth that hols the stars.
Radio Galaxy
Nebula
Celestial Sphere
greehouse effects
25. Neptune or uranus
Coldest surface
supernova
asteroid
Parallax
26. Sudden blasts of gamma radiation from a very distant galaxy caused possibly by a supernova explosion.
coma
H2 Regions
Celestial Sphere
Gamma ray bursts
27. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
nova
solar nebula
Absolute Magnitude
Make up of the terrestrial planets
28. A quantity measuring the stability of the Earth's atmosphere
HII Region
Density Wave
Seeing
OB Associations
29. The entity from which the whole universe is postulated to have come from.
Winter Solstice
hottest surface
3 reasons we orbit satellites to observe universe
cosmic singularity
30. Europa
MOONS: roundest shape
Titus-Bode Law
MOONS: largest size
Big Bang
31. Jupiter
fastest rotation
Flat - Flat
Dark Matter
Turn off Point
32. 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.
Open Cluster
Turn off Point
Sc spiral galaxy
Emission Spectrum
33. A collection of galaxies like the one the Milky Way belongs to
Poor Cluster
critical density
Pulsar
MOONS: larger than mercury
34. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
supernova
isotropic
epicycle
coma
35. The telescope configuration that has the focus placed at the back of the primary mirror
Cassegrain Focus
Wein's Law
Parallax
Roundest orbit
36. The oldest part of the Milky Way
Halo
standard candle
Reflector
weight
37. 100 nm 10 nm
mass
superclusters
A family of radiant energy- includes light
Electromagnetic Radiation: Ultraviolet Light
38. The apparent path of the Sun through the stars on the celestial sphere.
Oort cloud
Kuiper belt
Ecliptic
most eccentric orbit
39. A small spherical dark nebula
H2 Regions
Prominence
Jupiters red spot
Bok Globule
40. The rate of expansion of the universe.
Terrestrial Planets
density
force
Hubble constant
41. Europa
Absolute Magnitude
Absorption Spectrum
MOONS: roundest shape
Thermal Equilibrium
42. A point in the sky where meteors appear to come from during a shower
Filament
Absolute Magnitude
radiant
Parsec
43. In what chemical form are jupiters nitrogen - carbon and oxygen?
Plank's Law
conjunction
Ammonia - methane - and water
plate tectonics
44. The distance light travels in one year (=9.46x10^12km).
Hydrostatic Equilibrium
Light-Year
Most dense
fastest rotation
45. The distance a moon can be from a planet before shattering from tidal forces
roche limit
Asymptotic giant Branch Star
Seeing
supermassive black hole
46. 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
Galilean satellite
Meridian
retrograde motion
disk
47. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
critical density
Spectroscopic Parallax
Poor Cluster
Secondary Mirror
48. Large bulge - tightly wound spiral arms - relatively few h2 regions and are smooth
Ganymede (Jupiter)
Sa spiral galaxy
Main Sequence
Void
49. A measure of the force of gravity on an object
weight
radiant
thinnest atmosphere
SETI
50. Large nebula consisting of very cold gas and dust
Molecular Clouds
meteoriod
Red Giant Branch Star
regolith