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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. Distribution of dust (tells us disk is thin) - find distances to O&B stars and H2 regions (arms are sights of star formation and OB stars live and die at location of birth) -Milky way has four arms. Sun is in spur apart from arms.
mapping the structure of Milky Way disk
direct motion
Electromagnetic Radiation: Radio
The Big Bang Theory
2. A push or a pull
force
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
Seyfert galaxy
Yes - frozen at the poles- remains protected from the suns rays
3. Venus
general star population
Flocculent spirals
Roundest orbit
MOONS: largest size
4. A continuous spectrum of light missing energy at a few wave lengths.
era of recombination
Absorption Spectrum
Focal Plane
Roundest orbit
5. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
Winter Solstice
Make up of the terrestrial planets
anorthosite
Pulsar
6. The movement of the Earth's crustal plates riding on top of the mantle.
Gravitational Lens
rotation curve = dark matter?
Sa spiral galaxy
plate tectonics
7. Large nebula consisting of very cold gas and dust
zone
Cassegrain Focus
Molecular Clouds
Hydrostatic Equilibrium
8. A cloud of ionized hydrogen. Formed when young stars heat the surrounding gas
HII Region
mare basalt
CNO Cycle
fewest moons
9. The source of the force that is accelerating the expansion rate of the universe.
dark energy
Maria
Galilean satellite
synchrotron radiation
10. An element of a highly efficient - two-dimensional electronic light detector
Superior planets
Chromosphere
Parallax
Pixel
11. Titan
contrast northern lowlands and the southern highlands of mars...
Sunspot cycle
Plank's Law
MOONS: thickest atmosphere
12. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
regolith
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
Negative - Diverge - Less than 1
CMB
13. Dying large-mass stars lose their outer layers in a violent explosion creating large - chaotic remnants. these brighten like nova but are so much brighter and only occur ONCE PER STAR
Yes - frozen at the poles- remains protected from the suns rays
matter dominated universe
supernova
force
14. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
Dark Matter
Negative - Diverge - Less than 1
great dark spots
Vernal Equinox
15. A distance measure determined by the shifting of a star against the background sky every 6 months.
Perihelion
Plank's Law
Dark Matter
Parsec
16. A force exerted by reflecting sunlight
Hydrostatic Equilibrium
radiation pressure
Continuous Spectrum
Nebula
17. The gap etween saturn's A and B rings
Photon
most moons
Kuiper belt
Cassini division
18. We can infer the absolute magnitude of pulsating variable stars by measuring their pulsation periods. The longer the pulsations - the greater their luminosities. We then again measure their apparent magnitudes - compare it with their absolute magnitu
radio lobe
Apparent Magnitude
zone
Cepheid variables
19. A quantity measuring the stability of the Earth's atmosphere
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.
Neutron Star
coma
Seeing
20. 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
The Big Bang Theory resolves Olber's Paradox
Olber's paradox
mare basalt
reflection star clusters
21. Comglomerates of ice and rock that orbit the sun in highly elliptical paths
most eccentric orbit
Synodic Day
Spectroscopic Parallax
comet
22. A representation of the changes in color and brightness of an evolving protostar.
Oort Cloud
radiation dominated universe
jovian
Hyashi track
23. Venus (retrograde)
slowest rotation
Population 1 vs Population 2 stars
superclusters
Maria
24. A younger cluster of stars - found in the galaxy disk
Sidereal Day
Dark Nebula
Disk
Open Cluster
25. The point in its orbit where a planet is farthest from the sun
aphelion
Absolute Magnitude
Spectroscopy
Red Giant
26. Then the Sun moves from north to south across the celestial equator (about September 23)
mare basalt
Autumnal Equinox
Callisto (Jupiter)
contrast northern lowlands and the southern highlands of mars...
27. 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
Poor Cluster
Spectroscopic parallax
Shepherd satellite
differential rotation
28. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
Dark Nebula
quasar
Differential Rotation
Blackbody Curve
29. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
Filament
density parameter
Dark Nebula
planetesimal
30. The shadow area behind the Earth or Moon where the Sun is completely obscured.
Annular Eclipse
comet
widmanstatten pattern
Umbra
31. Any change in the speed or direction of an object's motion
smallest diameter
Sunspots
reflection star clusters
acceleration
32. Material that shoots rapidly out into space. Flares cause Auroras
Light Gathering Power
Flare
Extrasolar Planet
Celestial Equator
33. 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.
Light: travels like a wave - detected like a particle
MOONS: roundest shape
Spectroscopic Parallax
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
34. How is the Hubble Law consistent with an expanding universe?
Radio Galaxy
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.
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
cosmic fireball
35. The process similar to conduction by which energy moves from the solar core to the convective layer
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.
Radiative Diffusion
Light-Year
shape and color of SPIRAL galaxies
36. A phenomenon seen when the Earth passes through the orbit of a burned out comet
cosmological red shift
meteor shower
Molecular Clouds
evidence of water on mars
37. When the Sun moves from south to north across the celestial equator (about March 21)
Vernal Equinox
Zenith
cosmology
Radiative Diffusion
38. The normal eastward movement of a planet against the background of hte distant stars.
MOONS: larger than mercury
direct motion
Photon
radio lobe
39. Earth
Flat - Flat
Most dense
CCD
radiant
40. A large - irregularly shaped rocky object orbiting the sun mostly between mars and jupiter. Left-over planetesimals
Planck time
general star population
asteroid
smallest diameter
41. A huge sphere of tenuous gas surrounding the nucleus of a comet
Wein's Law
Io (jupiters moon)
coma
Steady State Theory (Leads to Olber's Paradox)
42. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
rotation curve=winding dilemma?
Annular Eclipse
Objective Lens
Largest diameter
43. Why does the earth have few craters while the moon has many?
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
A family of radiant energy- includes light
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
difference between maria and highlands of the moon.
44. Latin for 'cloud'. A word used to describe the collections of gas and dust in the Milky Way and other galaxies
cosmological red shift
Cepheid Variable
Nebula
cosmic singularity
45. 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.
tectonics of Venus
Energy Level
deferent
Io (jupiters moon)
46. When a planet lines up with the sun inthe sky
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Thermonuclear Fusion
Synchrotron Rotation
conjunction
47. Young clusters in disk are irregularly shaped since they have no time to relax into the rounder relaxed shape of globular clusters-will constantly be torn apart and assimilated.
tectonics of Earth
Energy Level
Summer Solstice
open star clusters
48. The 'edge' of the universe. Light beyond this has not reached us yet.
Gamma-ray Burst
fewest moons
partile horizon
quasar
49. A small and dim but hot star.
highlands
Sc spiral galaxy
Focal Plane
White Dwarf
50. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
molecular clouds
thinnest atmosphere
radiation pressure
Plague