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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 huge sphere of tenuous gas surrounding the nucleus of a comet
supernova
Open Cluster
coma
most eccentric orbit
2. Mercury and venus
fewest moons
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
meteorite
self-propagating star formation
3. The high- temperatature outer layer of the sun
roche limit
Main Sequence
Corona
Maria
4. The universe is isotropic - homogeneous - and without beginning or end in time and space. If the universe is truly homogeneous then every line of sight will eventually end on a galaxy. If it has existed forever then there has been enough time for lig
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5. The equation that describes how matter equates with energy
CNO Cycle
Gamma ray bursts
E=mc2
standard candle
6. The act of removing an electron from an atom.
Ionization
difference between maria and highlands of the moon.
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Primary Mirror
7. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
Flare
Dark Nebula
Primary Mirror
Red Giant
8. The part of the Milky way that has on-going star formation
Occam's razor
cosmological principle
Disk
Parallax
9. A cloud of ionized hydrogen. Formed when young stars heat the surrounding gas
Cosmological Principle
fewest moons
HII Region
Autumnal Equinox
10. The cosmological principle is the assumption that the universe is isotropic and homogeneous.The Big Bang assumes it to be a correct principle so that what we observe is exactly like What is too far away to be observed.
Neutron Star
Cosmological Principle
Photometry
Objective Lens
11. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
Differential Rotation
Positive - Converge - Greater than 1
Drake equation
CNO Cycle
12. The projection of the Earth's equator onto the celestial sphere.
disk
Celestial Equator
Bulge
asteroid
13. The fusion process that turns three helium nuclei into a carbon nucleus
Triple Alpha rocess
Vernal Equinox
Refractor
least dense
14. A subatomic particle with a negative charge. It creates light.
chondrite
nucleus
Electron
chondrite
15. When the Sun is farthest south of the celestial equator (About December 22)
Hyashi track
dark matter
Europa (Jupiters moon)
Winter Solstice
16. The organization of clusters of galaxies into sheets and strings
critical density
least dense
Supercluster
shape and color of SPIRAL galaxies
17. A galaxy emitting large amounts of energy at long wavelengths.
Spectroscopic Parallax
Electromagnetic Radiation: X-Ray
Hipparchus
radio galaxy
18. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
Black Hole
Secondary Mirror
Dark Matter
shape and color of SPIRAL galaxies
19. The number of protons in an atom.
cosmological red shift
Total Eclipse
Atomic Number
Cepheid variables
20. A word used in astronomy to describe all elements besides hydrogen and helium
Metals
evidence of water on mars
Lagrangian Razor
Filament
21. The oldest terrain on the moon
highlands
Nova
Planck time
Penumbra
22. A rock or iron specimen that has fallen from space
Active Optics
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Flocculent spirals
meteorite
23. Sulfurous volcanoes - pools of liquid sulfur - surface resembles cheese pizza ACTIVE SURFACE
rotation curve=winding dilemma?
If it is in a denser medium - such as glass - it will move slower
resonance
Io (jupiters moon)
24. 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)
Magnification
meteor shower
blazar
matter dominated universe
25. An empirical scheme for predictin ghe orbital distances of planets
Lagrangian Razor
Titus-Bode Law
Galilean satellite
cosmic singularity
26. The law that predicts the possible types of spectra.
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27. Elliptical orbits that come inside orbit of the Earth.
Gravitational Lens
Dark Nebula
Convection
Apollo asteroids
28. The mass of an object divided by its volume
Geocentric
tectonics of Mars
density
asteroid
29. A fusion process in which protons build together to form helium
density waves
Electromagnetic Radiation
Sunspot cycle
Proton-proton chain
30. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
interstellar dust
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
Spectroscopic Parallax
meteorite
31. The apparent path of the Sun through the stars on the celestial sphere.
Ecliptic
Nebula
highlands
interstellar dust
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.
cosmic singularity
If it is in a denser medium - such as glass - it will move slower
Thermal Equilibrium
Neutron Star
33. The place in the sky that the Earth's axis points toward (can be either north or south)
Kuiper belt
Europa (Jupiters moon)
Colestial Pole
Proton-proton chain
34. A measure of how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
superclusters
Chromosphere
Electromagnetic Radiation
mass
35. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
Blackbody
Main Sequence
Make up of the terrestrial planets
Open - flat - and closed.
36. Long - meandering cliff formed when a planet surface cools and shrinks
Inverse Square Law
Ammonia - methane - and water
scarp
Disk
37. 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 _____.
weight
Pulsar
general star population
Flat - Remain Parallel - Exactly 1
38. A measure of the ability of a telescope to see fine detail
If it is in a denser medium - such as glass - it will move slower
We don't know. It might be but does not have to be.
Resolving Power
scarp
39. The trapping of heat by carbon dioxide or other gases in the Earth's atmosphere.
Color Index
Astronomical Unit
greehouse effects
Globular Cluster
40. The instant of time after the Big Bang when space and time obtained their characteristics. (t=10^-43 sec when gravity freezes out-instant when gravity started existing as a separate force)
meteor
disk
Annular Eclipse
Planck time
41. The universe is isotropic - homogeneous - and without beginning or end in time and space. If the universe is truly homogeneous then every line of sight will eventually end on a galaxy. If it has existed forever then there has been enough time for lig
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42. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
Callisto (Jupiter)
Electromagnetic Radiation: Radio
Hubble law
critical density
43. Then the Sun moves from north to south across the celestial equator (about September 23)
supermassive black hole
Cepheid variables
Absorption Spectrum
Autumnal Equinox
44. Matter so dense that even light cannot escape its gravity
The Local Group
direct motion
Black Hole
Titus-Bode Law
45. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
Parallax
Ganymede (Jupiter)
Umbra
Oort cloud
46. The rotation of a star or planet at different speeds at its equator and poles
differential rotation
Bok Globule
conjunction
Wein's Law
47. An energetic event taking place in the early universe
OB Associations
Gamma-ray Burst
meteoriod
Celestial Equator
48. Infinitely long -> 10 cm
Black Hole
critical density
density waves
Electromagnetic Radiation: Radio
49. A galaxy sending out a stream of material from its nucleus
cosmological red shift
tectonics of Venus
Radio Galaxy
Callisto (Jupiter)
50. Radiation given off by electrons accelerating in a magnetic field
Thermonuclear Fusion
meteor
Synchrotron Rotation
Sc spiral galaxy