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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 change in the wavelength of light caused by a motion between the observer and light (or wave) source (blue shift if getting closer - red shift if moving away)
open star clusters
Doppler Shift
Eyepiece Lens
Colestial Pole
2. Dark - reddish - low-pressure bands in Jupiter's atmosphere
belt
Largest diameter
Hipparchus
reflection star clusters
3. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
accretion disk
Kirchhoff's Law
Density Wave
Spectroscopic parallax
4. 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
nucleus
Dark Nebula
Cepheid variables
Kuiper belt
5. In what chemical form are jupiters nitrogen - carbon and oxygen?
Umbra
Reflector
Ammonia - methane - and water
differential rotation
6. Small compact stars called white dwarfs can have material deposited on their surfaces. In time material heats up and explodes in surface nuclear reaction- star brightens - settles - repeats.
nova
Shepherd satellite
Ammonia - methane - and water
neutrino
7. Dying small mass stars lose their outer layers in a relatively gentle way - creating a round or bipolar nebula about the star (round like planets)
MOONS: roundest shape
planetary nebula
Radio Galaxy
Sc spiral galaxy
8. A particle of light.
Blackbody Curve
Focal Plane
Photon
Globular Cluster
9. The distance light travels in one year (=9.46x10^12km).
Oort Cloud
bulge
great red spot
Light-Year
10. The family of radiant energy that includes light as a subset
MOONS: larger than mercury
Electromagnetic Radiation
Extrasolar Planet
cosmic singularity
11. The rock that makes up the lunar highlands
anorthosite
Geocentric
fusion crust
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.
12. The fusion process that turns three helium nuclei into a carbon nucleus
Ole Roemer
Hubble law
Apparent Magnitude
Triple Alpha rocess
13. Orbit in Jupiters orbit
Trojan asteroids
opposition
Lagrangian Razor
Electron
14. A small and dim but hot star.
White Dwarf
shape and color of ELLIPTICAL galaxies
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
cosmological principle
15. 10^2 nm 10^7 nm
Eclipses of the Moons of Jupiter
Electromagnetic Radiation: Infrared
jovian
Electromagnetic Radiation: Gamma Ray
16. When one side of a body always faces the planet it revolves around
synchronous rotation
Cosmic Microwave Background (CMB)
Autumnal Equinox
Blackbody
17. 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.
Olber's paradox
Population 1 vs Population 2 stars
Dark Matter
Emission Spectrum
18. Population 1 with higher metals and contain many young stars in star clusters. Distribution of stars is everywhere in disk (arms only have 5% more stars)
general star population
Chromosphere
Dark Nebula
cosmology
19. Venus
molecular clouds
neutrino
Thickest atmosphere
Sb spiral galaxy
20. Theory virtually demands that the geometry of the universe be ______. Results of measuring lumps in the cosmic background radiation indicate that the universe geometry is ________.
Electromagnetic Radiation: Gamma Ray
standard candle
Extrasolar Planet
Flat - Flat
21. 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)
How is winding dilemma solved?
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
Halo
disk
22. Earth
Seyfert galaxy
Nebula
molecular clouds
Most dense
23. Sulfurous volcanoes - pools of liquid sulfur - surface resembles cheese pizza ACTIVE SURFACE
Io (jupiters moon)
CCD
Astronomical Unit
Cepheid Variable
24. The point where an inferior planet is as far away from the sun as it can be (as seen from the Earth)
Energy Level
Gamma ray bursts
greatest elongation
roche limit
25. A force exerted by reflecting sunlight
Precession
radiation pressure
Supercluster
Autumnal Equinox
26. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
Chromosphere
accretion disk
Bok Globule
Cosmological Principle
27. A telescope that uses lenses to focus light
Umbra
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.
Steady State Theory (Leads to Olber's Paradox)
Refractor
28. A particle of light
Photon
tectonics of Mars
SETI
Globular Cluster
29. Dark areas on the sun that are cooler than the surrounding photosphere
Coronal Loop
Occam's razor
hottest surface
Sunspots
30. The seasonal shifting of a nearby star's position relative to more distant objects.
Parallax
Make up of the jovian planets
Enke gap
Largest diameter
31. The state of having a balance between inflowing and outflowing heat-- the temp at every radial point is different but constant
great red spot
great dark spots
Celestial Equator
Thermal Equilibrium
32. A particle of light
Occam's razor
Kuiper belt
Disk
Photon
33. The oldest terrain on the moon
highlands
Flare
Cassini division
Apollo asteroids
34. How is the Hubble Law consistent with an expanding universe?
Eyepiece Lens
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.
Hyashi track
Negative - Diverge - Less than 1
35. The law stating that hotter blackbodies look bluer than cooler blackbodies.
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36. The fate of the universe if it is closed. The universe expanding as much as possible and then retracting
Metals
Light Gathering Power
Big Crunch
Pulsar
37. A huge sphere of tenuous gas surrounding the nucleus of a comet
force
coma
Meridian
Resolving Power
38. Extremely round - lots of liquid water - ice rafts on surface ACTIVE SURFACE
Europa (Jupiters moon)
planetary nebula
Spectroscopic parallax
Terrestrial Planets
39. A spread of light with an uninterrupted wavelength distribution of energy.
density parameter
Electromagnetic Radiation: Visible Light
Continuous Spectrum
Big Bang
40. The entity responsible for spiral arms in grand-design spiral galaxies
Density Wave
Triple Alpha rocess
Geocentric
cosmic singularity
41. The law that syas light energy from a blackbody increases as (temperature^4)
Void
radio lobe
Stephen-Boltzman Law
Zenith
42. When the Sun is farthest north of the celestial equator (about June 22)
Ecliptic
Summer Solstice
nova
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
43. Matter so dense that even light cannot escape its gravity
Black Hole
Make up of the terrestrial planets
meteorite
zone
44. A faint - remarkably uniform distribution of radiation in space
Zenith
chondrite
Heliocentric
Cosmic Microwave Background
45. 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)
Make up of the jovian planets
How is winding dilemma solved?
regolith
comet
46. A star that has become a red giant for the second and final time. It is burning helium to carbon in a shell surrounding the core
Liquid metallic hydrogen
Positive - Converge - Greater than 1
Continuous Spectrum
Asymptotic giant Branch Star
47. A quantity measuring the stability of the Earth's atmosphere
Seeing
Dark matter candidates
Eclipses of the Moons of Jupiter
mass
48. The organized effort to find life elsewhere in the universe. (Search for Extra-Terrestrial Intelligence)
synchronous rotation
self-propagating star formation
SETI
Cosmic Microwave Background (CMB)
49. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Light Gathering Power
How is winding dilemma solved?
Main Sequence
If it is in a denser medium - such as glass - it will move slower
50. A phenomenon seen when the Earth passes through the orbit of a burned out comet
Planetary Nebula
Apollo asteroids
meteor shower
Sb spiral galaxy