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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 quantity measuring the stability of the Earth's atmosphere
Active Optics
Kuiper belt
partile horizon
Seeing
2. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
meteor shower
Make up of the terrestrial planets
comet
tectonics of Venus
3. A planet that is closer to the sun than the earth
inferior planets
CNO Cycle
Plague
Drake equation
4. Why does the earth have few craters while the moon has many?
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Reflector
aphelion
Ganymede (Jupiter)
5. The powdered stone fragments that make up the lunar 'soil'
Spectroscopy
regolith
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
Cassegrain Focus
6. The fusion process that turns three helium nuclei into a carbon nucleus
synchronous rotation
Halo
radio galaxy
Triple Alpha rocess
7. 1 mm 1μm
Electromagnetic Radiation: Infrared
Instability strip
Nucleus
Electromagnetic Radiation: Visible Light
8. Saying that the sky should not get dark at night because all lines of sight end on a star meaning that the night sky should be ablaze BUT the big bang - because the universe had a beginning - says that the sky gets dark because out in space - galaxie
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9. When material is heated and moves taking the heat energy with it
matter dominated universe
The Local Group
Convection
deferent
10. IO
Molecular Clouds
MOONS: most geologically active
Pulsar
Neutron Star
11. Mercury
dark energy
Black Hole
most eccentric orbit
White Dwarf
12. Matter that reveals itself only through its gravitational attraction.
dark matter
Gravity only pulls matter back together. Therefore - if gravity is the only force that operates on cosmic scales then the expansion of the universe should decrease with time. The critical density is the value of matter density sufficient to halt the
Yes - frozen at the poles- remains protected from the suns rays
The Big Bang Theory
13. 10 cm -> 1 mm
tectonics of Mars
Sa spiral galaxy
Electromagnetic Radiation: Microwave
Heliocentric
14. A fusion process in which protons build together to form helium
Sidereal Day
Proton-proton chain
accretion disk
Poor Cluster
15. Hydrogen and helium (mainly)
Kuiper belt
Make up of the jovian planets
density waves
nova
16. The first rock-sized bodies that formed in the solar nebula from dust grains
open star clusters
chondrite
Photon
Seyfert galaxy
17. A word used in astronomy to describe all elements besides hydrogen and helium
Grand design spirals
Metals
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Color Index
18. Star speed at outer edge of galaxy should begin to diminish - but they dont so we guess that this means there is increasing force (aka dark matter)
rotation curve = dark matter?
Annular Eclipse
Flare
Neutron Star
19. 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
rotation curve=winding dilemma?
Geocentric
reflection star clusters
coma
20. The linear correlation between the rate of the expansion of the universe and distance. Says that as galaxies get farther away in space - the speed with which they recede from us increases. So we can measure the amount of recessional velocity and use
Ground State
rotation curve = dark matter?
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Hubble law
21. 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.
CCD
Flare
Electromagnetic Radiation: Infrared
Particle Horizon
22. An empirical scheme for predictin ghe orbital distances of planets
Hubble law
Titus-Bode Law
Photometry
Drake equation
23. Sc galaxies
Electromagnetic Radiation
Europa (Jupiters moon)
Jovian Planets
Flocculent spirals
24. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
partile horizon
H2 Regions
3 reasons we orbit satellites to observe universe
Planck time
25. Centered on the sun.
Pixel
quasar
CNO Cycle
Heliocentric
26. A small round distribution of gas surrounding a dying star
contrast northern lowlands and the southern highlands of mars...
Oort cloud
Planetary Nebula
Eyepiece Lens
27. When the Moon entirely blocks the Sun.
terrestrial planet
Plague
Total Eclipse
Zenith
28. A subatomic particle with a negative charge. It creates light.
supermassive black hole
Electron
MOONS: thickest atmosphere
density parameter
29. A small round distribution of gas surrounding a dying star
Metals
Heliocentric
Differential Rotation
Planetary Nebula
30. Titan
radio galaxy
synchronous rotation
MOONS: thickest atmosphere
Pixel
31. Distance from sun to nucleus- 8 kiloparsecs (26000 LY) - diameter of Milky way- 150000 LY - length for sun to orbit once around milky way- 250 million years
Milky way Galaxy
Plague
most eccentric orbit
Steady State Theory (Leads to Olber's Paradox)
32. The oldest terrain on the moon
Callisto (Jupiter)
Quasar
MOONS: largest size
highlands
33. Flattened spherical distribution of old stars with some young stars too. 'hub' of Milky way - stars orbit with solid body speeds. Elongated into bar shape
Hyashi track
Light Gathering Power
bulge
Sunspot cycle
34. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
Cosmic Microwave Background
Sb spiral galaxy
Refractor
Cosmological Principle
35. Stars orvits do not define the spiral patterns - instead they are density waves that move at slower speeds (arms are defined by young O and B stars and gas clouds)
Umbra
radiation pressure
Callisto (Jupiter)
How is winding dilemma solved?
36. The oldest grouping of stars - found in the galaxy halo
MOONS: most geologically active
Globular Cluster
Spectral Lines
shape and color of SPIRAL galaxies
37. The rock that makes up the lunar highlands
aphelion
anorthosite
self-propagating star formation
Emission Spectrum
38. A large and bright but cool star.
critical density
Perihelion
radiation pressure
Red Giant
39. IO
Milky way Galaxy
Gamma-ray Burst
MOONS: most geologically active
Open Cluster
40. A method of finding a star's distance from its absolute magnitude and spectral type or color.
Dark matter candidates
Spectroscopic Parallax
shape and color of SPIRAL galaxies
Focal Length
41. The imaginary sphere centered on the Earth that hols the stars.
density waves
cosmological red shift
Synchrotron Rotation
Celestial Sphere
42. A subatomic particle with a negative charge. It creates light.
Positive - Converge - Greater than 1
Autumnal Equinox
Electron
Parallax
43. The location in the Milky Way where stars orbit like a solid wheel
density waves
Gravity only pulls matter back together. Therefore - if gravity is the only force that operates on cosmic scales then the expansion of the universe should decrease with time. The critical density is the value of matter density sufficient to halt the
Annular Eclipse
Bulge
44. A technique using computer-controlled mirrors to sharpen images distorted by the atmosphere
cosmological principle
Instability strip
direct motion
Active Optics
45. Sa - Sb galaxies where two magnificent arms wind their way from nucleus out in a symmetrical manner.
Grand design spirals
Titus-Bode Law
Cepheid Variable
Drake equation
46. The location of a supermassive black hole
Void
Roundest orbit
Sunspots
Nucleus
47. Why does the earth have few craters while the moon has many?
evidence of water on mars
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Ammonia - methane - and water
Parsec
48. N=are*Fp(Ne)(Fl)(Fi)(Fc)(L) N: number of civilizations possible to communicate with are*: rate solar-like stars are created Fp: fraction of stars with planets Ne: number of planets like ours Fl: fraction of planets with life Fi: intelligent life Fc:
Nebula
Drake equation
jovian
The Big Bang Theory
49. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
CCD
Photometry
epicycle
greehouse effects
50. Mercury
Planck time
meteorite
most eccentric orbit
Dwarf planets