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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. All possible types of energy that can be emitted and absorbed by atoms.
MOONS: most geologically active
mass
Europa (Jupiters moon)
Electromagnetic Radiation
2. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
chemical differentiation
CCD
Electromagnetic Radiation: Microwave
Parallax
3. How did Earth come to have an oxygen rich atmosphere?
Focal Plane
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.
Plague
Callisto (Jupiter)
4. Norhern lowlands- darker in color and have far fewer craters as if an ancient sea or ice field covered them. southern highlands- much higher in density of craters.
dark energy
homogeneous
Interstellar Extinction
contrast northern lowlands and the southern highlands of mars...
5. A streak of light in the atmosphere
Neutron Star
accretion disk
Brown dwarf
meteor
6. The relation that tells how light dims with distance.
nucleus
Inverse Square Law
Sunspots
Flat - Flat
7. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
Light Curve
synchronous rotation
interstellar dust
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
8. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
Electromagnetic Radiation: Radio
Total Eclipse
molecular clouds
asteroid
9. Mercury
Black Hole
smallest diameter
accretion
Radiative Diffusion
10. The act of removing an electron from an atom.
Electromagnetic Radiation: Ultraviolet Light
Supercluster
Pulsar
Ionization
11. The point in its orbit where a planet is nearest the sun
Eyepiece Lens
great dark spots
Perihelion
difference between maria and highlands of the moon.
12. 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
Extrasolar Planet
disk
Turn off Point
meteoriod
13. The normal eastward movement of a planet against the background of hte distant stars.
High Velocity Stars
direct motion
Eclipses of the Moons of Jupiter
Dark Nebula
14. A subatomic particle with a negative charge. It creates light.
Electron
Objective Lens
shape and color of ELLIPTICAL galaxies
MOONS: larger than mercury
15. The state of having a balance between inflowing and outflowing heat-- the temp at every radial point is different but constant
interstellar dust
cosmic fireball
Thermal Equilibrium
Hydrostatic Equilibrium
16. Mercury - Venus - Earth - Mars
Terrestrial Planets
Kirkwood gaps
Active Optics
Negative - Diverge - Less than 1
17. The 'edge' of the universe. Light beyond this has not reached us yet.
Doppler Shift
partile horizon
radiant
Geocentric
18. The surface of the sun
Vernal Equinox
Photosphere
Maria
Supercluster
19. The average distance between the Earth and the Sun (=1.5 x10^8km)
Poor Cluster
aphelion
Summer Solstice
Astronomical Unit
20. Comglomerates of ice and rock that orbit the sun in highly elliptical paths
Convection
comet
Thermonuclear Fusion
Blackbody Curve
21. The nuclei of very distant galaxies. Likely a manifestation of supermassive black holes
Quasar
deferent
widmanstatten pattern
interstellar dust
22. The state of having a balance between inflowing and outflowing heat-- the temp at every radial point is different but constant
Trojan asteroids
Thermal Equilibrium
Cosmic Microwave Background (CMB)
E=mc2
23. Infinitely long -> 10 cm
Electromagnetic Radiation: Radio
MOONS: largest size
Open - flat - and closed.
differential rotation
24. A repeated - periodic push or pull capable of summing into a larger push or pull
Eyepiece Lens
fusion crust
resonance
Main Sequence
25. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
Quasar
CNO Cycle
Photometry
semimajor axis
26. 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)
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.
MOONS: larger than mercury
quasar
Cassini division
27. A cloud of ionized hydrogen. Formed when young stars heat the surrounding gas
Plank's Law
Cosmic Microwave Background
Electromagnetic Radiation: Infrared
HII Region
28. The law that predicts the possible types of spectra.
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29. The gap etween saturn's A and B rings
Hyashi track
Density Wave
Cassini division
Globular Cluster
30. Electromagnetic Radiation
aphelion
Callisto (Jupiter)
Halo
A family of radiant energy- includes light
31. VENUS
weight
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
Yes - frozen at the poles- remains protected from the suns rays
evidence of water on mars
32. The Big Bang says that the universe has not existed forever. It had a distinct beginning about 14 billion years ago called the 'Big Bang'. Therefore light from any object more than 14 billion light years away has not had time to reach us. The other p
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33. Massive compact halo objects (MACHO) - weakly interacting massive particles (WIMPY's)
Continuous Spectrum
Dark matter candidates
Horizontal Branch Star
Geocentric
34. When material is heated and moves taking the heat energy with it
Convection
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
Perihelion
Hubble law
35. The Big Bang was not an explosion of matter into empty space - like the explosion of a bomb. Instead - it was an emergence of space and time filled with pure energy where before none of this was present. The point from which is emerged is called the
The Big Bang Theory resolves Olber's Paradox
The Big Bang Theory
High Velocity Stars
thinnest atmosphere
36. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
matter dominated universe
Dwarf planets
Electromagnetic Radiation: Gamma Ray
opposition
37. Hot cells of gas that rise and fall in the hotosphere
Thickest atmosphere
density
Granules
Seyfert galaxy
38. A star that blows itself apart
Supernova (You can be my supernova girl)
Cosmic Microwave Background
Ammonia - methane - and water
Titus-Bode Law
39. A high-pressure bulge in Neptune's southern hemisphere
Blackbody Curve
neutrino
Dark Nebula
great dark spots
40. Elliptical orbits that come inside orbit of the Earth.
Apollo asteroids
widmanstatten pattern
Degeneracy
Electromagnetic Radiation: Microwave
41. Why do Galaxies move very rapidly in the interiors of the dense clusters?
Inverse Square Law
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
matter dominated universe
partile horizon
42. Finding a star's absolute magnitude from it's placement on an HR diagram. After finding the absolute magnitude - we measure the apparent magnitude - for a distance modulus and use this to find the distance. This method is good for finding distances t
MOONS: most geologically active
Spectroscopic parallax
Seeing
Differential Rotation
43. 1 mm 1μm
Make up of the terrestrial planets
In an expanding universe all galaxies see all other galaxies that are not gravitationally bound to them receding away. This is what we see in the Hubble Law. We infer that the Hubble law also holds true for all other galaxies.
meteorite
Electromagnetic Radiation: Infrared
44. Moon in less than the angular diameter of the Sun.
Annular Eclipse
Kuiper belt
Planck time
Secondary Mirror
45. A highly variable galaxy nucleus of which BL Lac is one. Their light is highly energetic and their spectra are featureless. (face on)
Ammonia - methane - and water
blazar
Gravitational Lens
Maria
46. The 11 or 22 period on the sun durin which sunspots increase - decrease - change polarity - increase and decrease again.
Kirchhoff's Law
Sunspot cycle
quasar
Synchrotron Rotation
47. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
dark matter
density parameter
The Local Group
Proton-proton chain
48. A prominence seen against the disk of the sun
Filament
White Dwarf
Largest diameter
Perihelion
49. A measure of how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
resonance
mass
Negative - Diverge - Less than 1
Vernal Equinox
50. The shadow area behind the Earth or Moon where the Sun is completely obscured.
accretion
Umbra
shape and color of ELLIPTICAL galaxies
Seyfert galaxy