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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. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
Winter Solstice
direct motion
If it is in a denser medium - such as glass - it will move slower
Triple Alpha rocess
2. 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
Radio Galaxy
shape and color of ELLIPTICAL galaxies
bulge
Chandrasekhar Limit
3. A cloud of ionized hydrogen. Formed when young stars heat the surrounding gas
Synchrotron Rotation
Spectroscopic parallax
Spectroscopic Parallax
HII Region
4. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
Instability strip
3 reasons we orbit satellites to observe universe
Absolute Magnitude
shape and color of ELLIPTICAL galaxies
5. Consists of old red stars in slow orbits that plunge through disk and bulge. about 1% are old - round globular clusters.
Color Index
Halo
Cosmic Microwave Background
Terrestrial Planets
6. The distance light travels in one year (=9.46x10^12km).
MOONS: largest size
Europa (Jupiters moon)
chemical differentiation
Light-Year
7. Jupiter - Saturn - Uranus - Neptune
The Big Bang Theory resolves Olber's Paradox
Reflector
Jovian Planets
density parameter
8. The name for the only seriously considered theory of the universe.
Cosmic Microwave Background
meteoriod
Planck time
Big Bang
9. A galaxy sending out a stream of material from its nucleus
Triple Alpha rocess
Main Sequence
Thermal Equilibrium
Radio Galaxy
10. An evolved star - past the helium flash that is burning helium to carbon in it's cores
Trojan asteroids
retrograde motion
smallest diameter
Horizontal Branch Star
11. The gap inthe outer portion of Saturn's A ring
Enke gap
Electromagnetic Radiation: Microwave
belt
cosmic fireball
12. What is the universe expanding into?
Corona
CMB
It does not have to expand into anything. It might just be that the 3 dimensions of space are getting bigger. It may also be that our 3 spatial dimensions are expanding into higher dimensions if such things exist.
supermassive black hole
13. A streak of light in the atmosphere
meteor
Planetary Nebula
Secondary Mirror
Electromagnetic Radiation: Radio
14. The wavelengths where a specific element can absorb or emit light.
epicycle
Spectral Lines
Hubble law
Colestial Pole
15. An element of a highly efficient - two-dimensional electronic light detector
Pixel
Filament
Asymptotic giant Branch Star
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
16. A small chunk of rock in space
Precession
meteoriod
tectonics of Venus
Photon
17. A distance measure determined by the shifting of a star against the background sky every 6 months.
Planetary Nebula
Parsec
meteorite
cosmological principle
18. 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.
Plague
Particle Horizon
Turn off Point
Pixel
19. The north-south line passing directly overhead through the zenith.
Make up of the jovian planets
Trojan asteroids
Sa spiral galaxy
Meridian
20. The mass of an object divided by its volume
era of recombination
Horizontal Branch Star
Cepheid Variable
density
21. The fusion process that turns three helium nuclei into a carbon nucleus
OB Associations
Triple Alpha rocess
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Sc spiral galaxy
22. The layer of the sun just above the photosphere
Chromosphere
Color Index
interstellar dust
SETI
23. Ancient stream channels - flood planes - and sedimentary-type rock. Frozen water is found in the polar ice caps and in the soil.
300000 KM/sec
evidence of water on mars
Inverse Square Law
cosmological red shift
24. The apparent backward motion of a planet against the background of stars.
Cassini division
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.
epicycle
retrograde motion
25. The shadow area behind the Earth or Moon where the Sun is completely obscured.
Pixel
deferent
Umbra
Horizontal Branch Star
26. A younger cluster of stars - found in the galaxy disk
Electromagnetic Radiation
Open Cluster
Plank's Law
Energy Level
27. When a planet lines up with the sun inthe sky
conjunction
nova
fastest rotation
Horizontal Branch Star
28. The mirror that determines the focus configuration of a reflector
Thickest atmosphere
mapping the structure of Milky Way disk
Secondary Mirror
Energy Level
29. A collection of galaxies like the one the Milky Way belongs to
density waves
Poor Cluster
Metals
Coldest surface
30. Population 1- similar to the sun and 2% of elements are metal - Population 2- formed before gas was metal- only a fraction of mass is metal.
Cosmic Microwave Background
Population 1 vs Population 2 stars
Photon
shape and color of ELLIPTICAL galaxies
31. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Cosmological Principle
Sc spiral galaxy
terrestrial planet
great red spot
32. The mix of pure photon energy that emerged at the start of the universe.
300000 KM/sec
Light-Year
Big Crunch
cosmic fireball
33. The force of attraction between any two objects having mass
gravity
H-are Diagram
great dark spots
Ganymede (Jupiter)
34. The crust of a meteorite caused by its entry into Earth's atmosphere
Light Pollution
fusion crust
Precession
tectonics of Mars
35. Jupiter
aphelion
Titus-Bode Law
Yes - frozen at the poles- remains protected from the suns rays
most moons
36. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
Cassini division
Winter Solstice
comet
interstellar dust
37. The assumption that the universe is isotropic (same in all directions) and homogeneous (Same everywhere throughout)
Seyfert galaxy
quasar
Continuous Spectrum
cosmological principle
38. Sc galaxies
Plague
Red Giant Branch Star
condensation temperature
Flocculent spirals
39. Sc galaxies
Nucleus
difference between maria and highlands of the moon.
Parallax
Flocculent spirals
40. A word meaning 'the same everywhere throughout.'
CCD
Asymptotic giant Branch Star
homogeneous
Population 1 vs Population 2 stars
41. Sc galaxies where star formation and destruction is so rapid that supernova explosions are mainly responsible for compressing gas to create new stars.
Synchrotron Rotation
self-propagating star formation
Focal Plane
conjunction
42. A planet that is closer to the sun than the earth
Void
inferior planets
Planck time
Electromagnetic Radiation
43. The part of the Milky way that has on-going star formation
Ground State
Yes - frozen at the poles- remains protected from the suns rays
quasar
Disk
44. The dark - relativley smooth areas on the moon; Latin for sea
The Big Bang Theory resolves Olber's Paradox
gravity
Quasar
Maria
45. The assumption that the universe is isotropic (same in all directions) and homogeneous (Same everywhere throughout)
cosmological principle
Thermonuclear Fusion
fastest rotation
Ecliptic
46. Light-flaky crust - convective currents cause it to wrinkle and bunch (1/5 of surface). uniform cratering suggests lack of weathering and tectonics. volcanoes are flat due to atmospheric pressure.
Differential Rotation
tectonics of Venus
quasar
mass
47. The organized effort to find life elsewhere in the universe. (Search for Extra-Terrestrial Intelligence)
slowest rotation
density
Parsec
SETI
48. The act of removing an electron from an atom.
Ionization
anorthosite
synchrotron radiation
Focal Length
49. A large - irregularly shaped rocky object orbiting the sun mostly between mars and jupiter. Left-over planetesimals
Dark matter candidates
asteroid
Ionization
Degeneracy
50. The location around an atom where an electron resides.
MOONS: most geologically active
Energy Level
belt
nova