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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. The wavelengths where a specific element can absorb or emit light.
Flocculent spirals
Drake equation
jovian
Spectral Lines
2. The point where an inferior planet is as far away from the sun as it can be (as seen from the Earth)
density parameter
blazar
greatest elongation
High Velocity Stars
3. Jupiter
Electromagnetic Radiation: Infrared
most moons
How is winding dilemma solved?
aphelion
4. The shadow area behind the Earth or Moon where the Sun is completely obscured.
Umbra
zone
semimajor axis
tectonics of Venus
5. Galaxies whose nuclei emit jets of materil at high speeds. material comes from supermassive black holes
Flare
supernova
radio galaxy
dark matter
6. 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)
quarks
Neutron Star
planetary nebula
Stephen-Boltzman Law
7. A crystalline patter found in iron meteorites
Ammonia - methane - and water
Sc spiral galaxy
widmanstatten pattern
Kirchhoff's Law
8. 100 nm 10 nm
Electromagnetic Radiation: Ultraviolet Light
Annular Eclipse
Inverse Square Law
Halo
9. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
tectonics of Earth
Lagrangian Razor
Celestial Sphere
mapping the structure of Milky Way disk
10. The dimming of starlight by intervening dust
Cosmic Microwave Background
Interstellar Extinction
planetesimal
Differential Rotation
11. The law stating that hotter blackbodies look bluer than cooler blackbodies.
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12. The act of removing an electron from an atom.
Ionization
matter dominated universe
Callisto (Jupiter)
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
13. When one side of a body always faces the planet it revolves around
synchronous rotation
Turn off Point
Absorption Spectrum
conjunction
14. The rotation of a star or planet at different speeds at its equator and poles
deferent
Olber's paradox
differential rotation
Doppler Shift
15. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
accretion disk
Hubble constant
tectonics of Mars
CCD
16. 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.
open star clusters
Chandrasekhar Limit
Milky way Galaxy
Liquid metallic hydrogen
17. Orbit in Jupiters orbit
Molecular Clouds
Olber's paradox
rotation curve=winding dilemma?
Trojan asteroids
18. Large bulge - tightly wound spiral arms - relatively few h2 regions and are smooth
Observations of distant type Ia supernovae indicate that the expansion of the universe is speeding up with time - not slowing down! So there must be a force causing this.
Sa spiral galaxy
Emission Spectrum
Black Hole
19. Galaxies whose nuclei emit jets of materil at high speeds. material comes from supermassive black holes
blazar
radio galaxy
differential rotation
Rich Cluster
20. An empirical scheme for predictin ghe orbital distances of planets
Wein's Law
Celestial Equator
Titus-Bode Law
Enke gap
21. Arcs of increased mass concentration that slow stars and gas down as they orbit through which cause the formation of stars.
Globular Cluster
Nova
Radio Galaxy
density waves
22. A star without enough mass to begin hydrogen fusion
Brown dwarf
Zenith
Blackbody Curve
Halo
23. Material that shoots rapidly out into space. Flares cause Auroras
Flare
Interstellar Extinction
OB Associations
Sidereal Day
24. Either Io -Europa - Ganymede - or Callisto
Hipparchus
Galilean satellite
H2 Regions
cosmic fireball
25. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
supermassive black hole
Big Bang
Parsec
accretion disk
26. Consists of old red stars in slow orbits that plunge through disk and bulge. about 1% are old - round globular clusters.
Globular Cluster
self-propagating star formation
Halo
belt
27. The normal eastward movement of a planet against the background of hte distant stars.
direct motion
dark energy
accretion
Kuiper belt
28. Extremely round - lots of liquid water - ice rafts on surface ACTIVE SURFACE
Thickest atmosphere
Europa (Jupiters moon)
Winter Solstice
Radio Galaxy
29. Extends to a distance of 50000AU. Same objects as in the Kuiper belt-when they fall in toward the sun they become comets. Debris from comets hitting the Earths atmosphere cause meteor showers.
highlands
Oort Cloud
Differential Rotation
smallest diameter
30. A term referring to Earth-like planets
Synodic Day
standard candle
Energy Level
terrestrial planet
31. How did Earth come to have an oxygen rich atmosphere?
CCD
Zenith
Jupiters red spot
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.
32. First accurately measured the speed of light in a vacuum
condensation temperature
evidence of water on mars
contrast northern lowlands and the southern highlands of mars...
Ole Roemer
33. Then the Sun moves from north to south across the celestial equator (about September 23)
Autumnal Equinox
smallest diameter
smallest diameter
Electromagnetic Radiation: Infrared
34. Light scattered through the atmosphere that degrades astronomical images
Light Pollution
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.
shape and color of ELLIPTICAL galaxies
Summer Solstice
35. The gap inthe outer portion of Saturn's A ring
Yes - frozen at the poles- remains protected from the suns rays
Enke gap
Wein's Law
Electromagnetic Radiation: Radio
36. The rock that makes up the lunar maria
mare basalt
nucleus
Hyashi track
Radiative Diffusion
37. A plot of star absolute magnitude verses spectral type.
protostar
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Convection
H-are Diagram
38. Rich= dense crowded cores of galaxies - poor= few members and a looser organization of galaxies
E=mc2
Focal Plane
Rich vs poor clusters
Nowhere visible to us. If there are higher dimension then the center would be visible to someone who lives in one. If there are no higher dimensions then the center does not exist.
39. A measure of the force of gravity on an object
weight
Big Bang
jovian
Titus-Bode Law
40. Latin for 'cloud'. A word used to describe the collections of gas and dust in the Milky Way and other galaxies
Nebula
Differential Rotation
greehouse effects
great dark spots
41. Thick rigid crust - no longer has plate tectonics but still has convective hot spots that create earth-like volcanoes except that last for billions of years because of lack of tectonics.
tectonics of Mars
Cosmic Microwave Background
White Dwarf
great red spot
42. The light produced when particles from the sun collide with atmospheric molecules
Ammonia - methane - and water
Chandrasekhar Limit
planetesimal
aurora
43. The 'edge' of the universe. Light beyond this has not reached us yet.
Big Crunch
Flare
Light Curve
partile horizon
44. Large nebula consisting of very cold gas and dust
Molecular Clouds
Ecliptic
Light Pollution
Energy Level
45. Comglomerates of ice and rock that orbit the sun in highly elliptical paths
Convection
meteor shower
Sc spiral galaxy
comet
46. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
Density Wave
shape and color of SPIRAL galaxies
density parameter
Neutron Star
47. The projection of the Earth's equator onto the celestial sphere.
High Velocity Stars
Photon
Electromagnetic Radiation: Visible Light
Celestial Equator
48. The dark - relativley smooth areas on the moon; Latin for sea
Total Eclipse
Heliocentric
Turn off Point
Maria
49. The rock that makes up the lunar maria
Cepheid Variable
quarks
mare basalt
standard candle
50. How is the Hubble Law consistent with an expanding universe?
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.
most eccentric orbit
shape and color of ELLIPTICAL galaxies
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.