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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 word meaning 'the same in all directions.'
Electromagnetic Radiation: Radio
Atomic Number
Ammonia - methane - and water
isotropic
2. The projection of the Earth's equator onto the celestial sphere.
Terrestrial Planets
Celestial Equator
Kirkwood gaps
Void
3. When a planet lines up with the sun inthe sky
accretion
OB Associations
conjunction
Prominence
4. The lowest energy of an atom.
White Dwarf
Ground State
Oort cloud
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
5. Electromagnetic Radiation
Sunspot cycle
A family of radiant energy- includes light
Secondary Mirror
Light: travels like a wave - detected like a particle
6. 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.
Electromagnetic Radiation
smallest diameter
Cosmic Microwave Background (CMB)
Main Sequence
7. 1-orbit aroudn the sun 2- are in hydrostatic equilibrium and 'mostly round' 3- have not cleared debris around its orbit 4- are not satellites
Dark Matter
quasar
planetesimal
Dwarf planets
8. The elementary building blocks from which protons and neutrons are formed.
belt
Flocculent spirals
tectonics of Venus
quarks
9. The larger bodies that formed early in teh solar nebula that were chemically differentiated
planetesimal
force
Brown dwarf
Gamma-ray Burst
10. The dimming of starlight by intervening dust
Sidereal Day
E=mc2
Interstellar Extinction
cosmic fireball
11. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
molecular clouds
Photometry
Granules
Flat - Flat
12. A term referring to the orbital character of stars near the Sun
Electromagnetic Radiation: Microwave
Differential Rotation
Flare
Quasar
13. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Kirkwood gaps
Geocentric
Roundest orbit
Interstellar Extinction
14. Dark areas on the sun that are cooler than the surrounding photosphere
Sunspots
Coronal Loop
density parameter
solar nebula
15. Jupiter - Saturn - Uranus - Neptune
Cassini division
Jovian Planets
Ganymede (Jupiter)
Astronomical Unit
16. Long - meandering cliff formed when a planet surface cools and shrinks
molecular clouds
Hyashi track
scarp
MOONS: thickest atmosphere
17. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Population 1 vs Population 2 stars
meteorite
Vernal Equinox
Main Sequence
18. The process responsible for creating the arms of flocculent spiral galaxies
MOONS: thickest atmosphere
Self-Propogating Star Formation
Open - flat - and closed.
least dense
19. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
Inverse Square Law
Photometry
Neutron Star
density
20. Why do Galaxies move very rapidly in the interiors of the dense clusters?
Flat - Remain Parallel - Exactly 1
Penumbra
self-propagating star formation
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
21. Material that shoots rapidly out into space. Flares cause Auroras
Flare
Triple Alpha rocess
quasar
supernova
22. A younger cluster of stars - found in the galaxy disk
Open Cluster
Total Eclipse
Neutron Star
quasar
23. A very dense - highly populated cluster of galaxies
Rich Cluster
Globular Cluster
Thermal Equilibrium
resonance
24. A word used in astronomy to describe all elements besides hydrogen and helium
Metals
Triple Alpha rocess
aphelion
accretion disk
25. Mercury and venus
great red spot
Light-Year
Filament
fewest moons
26. A volume of space where few - if any - galaxies are located
Magnification
weight
Void
Reflector
27. 10 nm 10^2 nm
rotation curve = dark matter?
Hubble constant
force
Electromagnetic Radiation: X-Ray
28. A force exerted by reflecting sunlight
Zenith
radiation pressure
Winter Solstice
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
29. A galaxy sending out a stream of material from its nucleus
jovian
Radio Galaxy
mass
Blackbody Curve
30. Venus
hottest surface
Photometry
anorthosite
Resolving Power
31. Poitns of gravitational stability in the orbit of a planet
Most dense
mapping the structure of Milky Way disk
Lagrangian Razor
supernova
32. 30AU to 50Au from sun - consists of ancietn premordial objects made of frozen ice and dust-35000 objects or more that are larger than 100 km in diameter and many more smaller than this
Focal Length
dark matter
Kuiper belt
Main Sequence
33. Matter so dense that even light cannot escape its gravity
Colestial Pole
Black Hole
Rich vs poor clusters
Kirkwood gaps
34. Light scattered through the atmosphere that degrades astronomical images
self-propagating star formation
Light Pollution
CCD
Nowhere visible to us. If there are higher dimension then the center would be visible to someone who lives in one. If there are no higher dimensions then the center does not exist.
35. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
tectonics of Earth
rotation curve = dark matter?
Penumbra
Ionization
36. The name for the only seriously considered theory of the universe.
Cassini division
Big Bang
Liquid metallic hydrogen
Cosmic Microwave Background (CMB)
37. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
shape and color of ELLIPTICAL galaxies
If it is in a denser medium - such as glass - it will move slower
Sb spiral galaxy
Sc spiral galaxy
38. The entity responsible for spiral arms in grand-design spiral galaxies
Jovian Planets
Density Wave
tectonics of Venus
great red spot
39. A large - irregularly shaped rocky object orbiting the sun mostly between mars and jupiter. Left-over planetesimals
Light Gathering Power
Shepherd satellite
Cepheid Variable
asteroid
40. Originially thought to be stars emitting radio radiation but are now concluded to be nuclei of distant galaxies (same as radio galaxies aka emit streams of material)
Oort Cloud
planetary nebula
quasar
Meridian
41. The entity from which the whole universe is postulated to have come from.
cosmic singularity
blazar
chemical differentiation
Cepheid variables
42. The mirror that gathers the light in a reflector
Photon
plate tectonics
Primary Mirror
asteroid
43. A large and bright but cool star.
Spectroscopy
greatest elongation
Red Giant
molecular clouds
44. Elliptical orbits that come inside orbit of the Earth.
Molecular Clouds
jovian
Apollo asteroids
blazar
45. 1. We see rapid movements or high energy radiation coming at some level from the nuclei of nearly every galaxy we have looked at. 2. We suspect that the creation of these supermassive black holes is part of the galaxy formation process.
thinnest atmosphere
Negative - Diverge - Less than 1
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
homogeneous
46. Jupiter
least dense
radio galaxy
HII Region
most moons
47. The 'edge' of the universe. Light beyond this has not reached us yet.
Positive - Converge - Greater than 1
partile horizon
MOONS: thickest atmosphere
Emission Spectrum
48. The process that powers the sun and hydrogen bombs
molecular clouds
Grand design spirals
Thermonuclear Fusion
bulge
49. A perfect absorber and radiator of electromagnetic radiation.
Titus-Bode Law
critical density
Blackbody
quasar
50. The relation that tells how light dims with distance.
Inverse Square Law
Annular Eclipse
Neutron Star
partile horizon