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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 apparent magnitude a star would have if it were at a distance of 10 parsecs.
Absolute Magnitude
greatest elongation
Supernova (You can be my supernova girl)
Cepheid variables
2. A star without enough mass to begin hydrogen fusion
H2 Regions
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
Brown dwarf
great red spot
3. Any change in the speed or direction of an object's motion
standard candle
acceleration
Blackbody Curve
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.
4. The rock that makes up the lunar maria
difference between maria and highlands of the moon.
protostar
Blackbody Curve
mare basalt
5. Sc galaxies
Kuiper belt
Flocculent spirals
Gravity only pulls matter back together. Therefore - if gravity is the only force that operates on cosmic scales then the expansion of the universe should decrease with time. The critical density is the value of matter density sufficient to halt the
We don't know. It might be but does not have to be.
6. Very center of galaxy. suggestion of a black hole
dark matter
Dark Matter
nucleus
E=mc2
7. A star that blows itself apart
Primary Mirror
Celestial Equator
Supernova (You can be my supernova girl)
Hipparchus
8. The light produced when particles from the sun collide with atmospheric molecules
If it is in a denser medium - such as glass - it will move slower
Main Sequence Stars
Nova
aurora
9. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
tectonics of Earth
coma
Roundest orbit
Electromagnetic Radiation: Gamma Ray
10. Hot cells of gas that rise and fall in the hotosphere
cosmological red shift
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.
Granules
matter dominated universe
11. 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)
planetary nebula
contrast northern lowlands and the southern highlands of mars...
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Yes - frozen at the poles- remains protected from the suns rays
12. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
Spectral Lines
Photometry
Magnification
Photon
13. Sa - Sb galaxies where two magnificent arms wind their way from nucleus out in a symmetrical manner.
conjunction
Grand design spirals
Big Bang
comet
14. When a planet lines up with the sun inthe sky
Seyfert galaxy
disk
conjunction
mapping the structure of Milky Way disk
15. The location in the Milky Way where stars orbit like a solid wheel
Supernova (You can be my supernova girl)
Bulge
Gravitational Lens
Oort Cloud
16. How is the Hubble Law consistent with an expanding universe?
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
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.
3 reasons we orbit satellites to observe universe
Emission Spectrum
17. The point directly overhead.
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.
slowest rotation
Zenith
homogeneous
18. When the Sun is farthest north of the celestial equator (about June 22)
Filament
Winter Solstice
Summer Solstice
Differential Rotation
19. Radiation given off by electrons accelerating in a magnetic field
Synchrotron Rotation
Filament
Lagrangian Razor
3 reasons we orbit satellites to observe universe
20. 1μm 100 nm
CCD
Callisto (Jupiter)
semimajor axis
Electromagnetic Radiation: Visible Light
21. The average distance between the Earth and the Sun (=1.5 x10^8km)
chondrite
Pixel
asteroid
Astronomical Unit
22. The process of acquiring material
Extrasolar Planet
Proton-proton chain
accretion
Hydrostatic Equilibrium
23. Either Io -Europa - Ganymede - or Callisto
Precession
Galilean satellite
Focal Plane
radiation pressure
24. A fusion process in which protons build together to form helium
Limb darkening
Yes - frozen at the poles- remains protected from the suns rays
Proton-proton chain
chemical differentiation
25. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
CCD
radiation pressure
molecular clouds
smallest diameter
26. A large and bright but cool star.
Open - flat - and closed.
Red Giant
Ganymede (Jupiter)
Blackbody Curve
27. The location around an atom where an electron resides.
Coronal Loop
gravity
Flocculent spirals
Energy Level
28. The rock that makes up the lunar highlands
anorthosite
slowest rotation
Electromagnetic Radiation
MOONS: thickest atmosphere
29. In Ptolemy's geocentric solar system - the large circle on which a planet's epicycle moved around the Earth.
zone
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.
deferent
Cassegrain Focus
30. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Extrasolar Planet
matter dominated universe
Parallax
Kirkwood gaps
31. Why does the earth have few craters while the moon has many?
radiation pressure
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Parallax
Light Pollution
32. The final end state of a high mass star. .An entity for which gravity has completely overwhelmed all other forces of nature.
Open - flat - and closed.
tectonics of Venus
Maria
Black Hole
33. What are the three possible geometries of the universe?
Yes - frozen at the poles- remains protected from the suns rays
mass
Objective Lens
Open - flat - and closed.
34. A collection of comets in the plane of the solar system - located beyond the orbit of Pluto
Kuiper belt
roche limit
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.
difference between maria and highlands of the moon.
35. The lowest energy of an atom.
Ground State
Turn off Point
Focal Plane
Corona
36. The imaginary sphere centered on the Earth that hols the stars.
Planetary Nebula
Winter Solstice
Limb darkening
Celestial Sphere
37. The lowest energy of an atom.
Jupiters red spot
Ground State
radiation pressure
thinnest atmosphere
38. The crust of a meteorite caused by its entry into Earth's atmosphere
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Light Pollution
retrograde motion
fusion crust
39. Venus
Thickest atmosphere
Annular Eclipse
Big Bang
Olber's paradox
40. Very center of galaxy. suggestion of a black hole
Apollo asteroids
chondrite
general star population
nucleus
41. A cloud of ionized hydrogen. Formed when young stars heat the surrounding gas
HII Region
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Jupiters red spot
protostar
42. A location on an H-are Diagram where evolving stars pulsate
Instability strip
Parsec
CMB
Dwarf planets
43. The slow wobble of the Earth on its rotation axis.
radio lobe
Refractor
Precession
opposition
44. In Ptolemy's geocentric solar system - the large circle on which a planet's epicycle moved around the Earth.
Ganymede (Jupiter)
Cepheid Variable
deferent
Ecliptic
45. Mercury and venus
interstellar dust
fewest moons
radiation dominated universe
The Big Bang Theory resolves Olber's Paradox
46. Comglomerates of ice and rock that orbit the sun in highly elliptical paths
density
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Annular Eclipse
comet
47. A subatomic particle with a negative charge. It creates light.
Halo
Make up of the jovian planets
Cepheid Variable
Electron
48. The lens that gathers the light in a refractor
Spectroscopic Parallax
Synchrotron Rotation
Electromagnetic Radiation: Visible Light
Objective Lens
49. The law that describes the blackbody curve - and let to quantum mechanics.
50. The relation that tells how light dims with distance.
Cassini division
Inverse Square Law
inferior planets
Apollo asteroids
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