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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 appearance of the sun at the edge of the solar disk
Limb darkening
Quasar
rotation curve = dark matter?
disk
2. A star that is burning hydrogen to helium in a shell surrounding it's core
Radiative Diffusion
Red Giant Branch Star
superclusters
Limb darkening
3. When the Sun is farthest north of the celestial equator (about June 22)
epicycle
Neutron Star
Planck time
Summer Solstice
4. The process that powers the sun and hydrogen bombs
Electromagnetic Radiation: Radio
isotropic
Thermonuclear Fusion
Bok Globule
5. Is there water on the moon?
Yes - frozen at the poles- remains protected from the suns rays
Focal Length
widmanstatten pattern
gravity
6. The telescope configuration that has the focus placed at the back of the primary mirror
Horizontal Branch Star
conjunction
Cassegrain Focus
Instability strip
7. 30AU to 50Au from sun - consists of ancietn premordial objects made of frozen ice and dust-35000 objects or more that are larger than 100 km in diameter and many more smaller than this
Kuiper belt
weight
How is winding dilemma solved?
Parallax
8. Hot cells of gas that rise and fall in the hotosphere
Electromagnetic Radiation: X-Ray
Eclipses of the Moons of Jupiter
Granules
Light Curve
9. The distance a moon can be from a planet before shattering from tidal forces
roche limit
Secondary Mirror
Ecliptic
accretion
10. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
Sidereal Day
Chandrasekhar Limit
Cassini division
CCD
11. The process similar to conduction by which energy moves from the solar core to the convective layer
Umbra
inferior planets
Convection
Radiative Diffusion
12. Is there water on the moon?
meteoriod
Planetary Nebula
Asymptotic giant Branch Star
Yes - frozen at the poles- remains protected from the suns rays
13. A perfect absorber and radiator of electromagnetic radiation.
smallest diameter
MOONS: thickest atmosphere
Blackbody
Sidereal Day
14. A nearby galaxy with a quasar-like nucleus. closer but less bright than quasars-weaker
Hipparchus
isotropic
Seyfert galaxy
Cassini division
15. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
Maria
Globular Cluster
partile horizon
molecular clouds
16. Sudden blasts of gamma radiation from a very distant galaxy caused possibly by a supernova explosion.
matter dominated universe
Asymptotic giant Branch Star
Gamma ray bursts
most eccentric orbit
17. 10 cm -> 1 mm
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.
Electromagnetic Radiation: Microwave
Photosphere
Doppler Shift
18. Europa
supermassive black hole
MOONS: roundest shape
difference between maria and highlands of the moon.
Photon
19. Sc galaxies
Flocculent spirals
3 reasons we orbit satellites to observe universe
Triple Alpha rocess
MOONS: largest size
20. The study of the universe as a whole.
cosmology
differential rotation
A family of radiant energy- includes light
Flat - Flat
21. The wavelengths where a specific element can absorb or emit light.
homogeneous
Spectral Lines
The Local Group
era of recombination
22. Jupiter - Saturn - Uranus - Neptune
Jovian Planets
Zenith
Flat - Flat
inferior planets
23. The mirror that determines the focus configuration of a reflector
radio lobe
Negative - Diverge - Less than 1
Secondary Mirror
Nebula
24. A star that erratically and explosively brightens and dims
Nova
cosmic fireball
Chromosphere
blazar
25. The larger bodies that formed early in teh solar nebula that were chemically differentiated
epicycle
We don't know. It might be but does not have to be.
Flocculent spirals
planetesimal
26. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
3 reasons we orbit satellites to observe universe
fastest rotation
Io (jupiters moon)
Self-Propogating Star Formation
27. Flattened spherical distribution of old stars with some young stars too. 'hub' of Milky way - stars orbit with solid body speeds. Elongated into bar shape
Ole Roemer
Penumbra
bulge
Coronal Loop
28. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
Gravitational Lens
Sunspot cycle
Cassini division
If it is in a denser medium - such as glass - it will move slower
29. The family of radiant energy that includes light as a subset
semimajor axis
fusion crust
Gamma ray bursts
Electromagnetic Radiation
30. Poitns of gravitational stability in the orbit of a planet
Big Bang
Electromagnetic Radiation
Lagrangian Razor
Steady State Theory (Leads to Olber's Paradox)
31. 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.
Drake equation
Filament
tectonics of Mars
Positive - Converge - Greater than 1
32. Consists of old red stars in slow orbits that plunge through disk and bulge. about 1% are old - round globular clusters.
Extrasolar Planet
Hydrostatic Equilibrium
chondrite
Halo
33. The projection of the Earth's equator onto the celestial sphere.
density waves
Celestial Equator
retrograde motion
Ionization
34. The trapping of heat by carbon dioxide or other gases in the Earth's atmosphere.
cosmic fireball
Blackbody
greehouse effects
regolith
35. When the Sun is farthest south of the celestial equator (About December 22)
comet
Extrasolar Planet
Dwarf planets
Winter Solstice
36. When the Sun moves from south to north across the celestial equator (about March 21)
Eclipses of the Moons of Jupiter
Vernal Equinox
shape and color of ELLIPTICAL galaxies
Negative - Diverge - Less than 1
37. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Kirkwood gaps
Light: travels like a wave - detected like a particle
Jupiters red spot
dark matter
38. The Greek philosopher responsible for making the stellar magnitude scale.
acceleration
semimajor axis
fewest moons
Hipparchus
39. 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
Ammonia - methane - and water
supernova
direct motion
Open - flat - and closed.
40. Radiation emitted when charged particles spiral rapidly in a magnetic field. come off of jets from black holes.
Population 1 vs Population 2 stars
It does not have to expand into anything. It might just be that the 3 dimensions of space are getting bigger. It may also be that our 3 spatial dimensions are expanding into higher dimensions if such things exist.
tectonics of Venus
synchrotron radiation
41. A repeated - periodic push or pull capable of summing into a larger push or pull
Light Curve
gravity
resonance
How is winding dilemma solved?
42. A word meaning 'the same in all directions.'
Red Giant Branch Star
Terrestrial Planets
cosmological principle
isotropic
43. When the Moon entirely blocks the Sun.
resonance
Photon
Total Eclipse
accretion disk
44. The nuclei of very distant galaxies. Likely a manifestation of supermassive black holes
Globular Cluster
Quasar
Magnification
Filament
45. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
Cosmological Principle
Rich vs poor clusters
Photometry
greatest elongation
46. When the Moon entirely blocks the Sun.
Total Eclipse
synchrotron radiation
radiation dominated universe
Electromagnetic Radiation: Infrared
47. A star that blows itself apart
Supernova (You can be my supernova girl)
Oort Cloud
general star population
Seyfert galaxy
48. The location in the Milky Way where stars orbit like a solid wheel
Pixel
Vernal Equinox
Bulge
Ganymede (Jupiter)
49. Centered on the Earth
Geocentric
Shepherd satellite
blazar
Spectroscopy
50. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
comet
radiation dominated universe
greehouse effects
neutrino