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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 point in the sky where meteors appear to come from during a shower
radiant
interstellar dust
Io (jupiters moon)
Apollo asteroids
2. Jupiter - Saturn - Uranus - Neptune
Hyashi track
MOONS: largest size
radio galaxy
Jovian Planets
3. The powdered stone fragments that make up the lunar 'soil'
Photosphere
self-propagating star formation
regolith
Rich Cluster
4. The oldest grouping of stars - found in the galaxy halo
Globular Cluster
coma
Winter Solstice
contrast northern lowlands and the southern highlands of mars...
5. Centered on the sun.
molecular clouds
Heliocentric
superclusters
Vernal Equinox
6. Very center of galaxy. suggestion of a black hole
Trojan asteroids
Light Pollution
Oort cloud
nucleus
7. 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)
Radio Galaxy
The Big Bang Theory resolves Olber's Paradox
most moons
Doppler Shift
8. Dark areas on the sun that are cooler than the surrounding photosphere
Dwarf planets
Sunspots
OB Associations
cosmology
9. The law that predicts the possible types of spectra.
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10. A logarithmically scaled value for the measured brightness of a star.
Make up of the terrestrial planets
Apparent Magnitude
Planetary Nebula
Terrestrial Planets
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
nucleus
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.
protostar
12. Possible Fates of the Universe
Molecular Clouds
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
Electromagnetic Radiation: Visible Light
quarks
13. Ganymede and Titan
Halo
MOONS: larger than mercury
300000 KM/sec
Ole Roemer
14. A representation of the changes in color and brightness of an evolving protostar.
Hyashi track
chondrite
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Filament
15. A small chunk of rock in space
Prominence
meteoriod
differential rotation
Supernova (You can be my supernova girl)
16. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
Ganymede (Jupiter)
Maria
Callisto (Jupiter)
Trojan asteroids
17. The cosmological principle is the assumption that the universe is isotropic and homogeneous.The Big Bang assumes it to be a correct principle so that what we observe is exactly like What is too far away to be observed.
blazar
Cosmological Principle
Spectroscopy
Refractor
18. The slow wobble of the Earth on its rotation axis.
Cosmological Principle
Open - flat - and closed.
Precession
Red Giant
19. Jupiter
Electromagnetic Radiation: X-Ray
semimajor axis
most moons
Spectroscopy
20. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
Sb spiral galaxy
difference between maria and highlands of the moon.
Drake equation
regolith
21. The 'edge' of the universe. Light beyond this has not reached us yet.
planetesimal
radiation dominated universe
partile horizon
homogeneous
22. Old - pock marked - icy surface - interior is not differentiated - geologically dead - NOT ACTIVE SURFACE
Callisto (Jupiter)
Void
Continuous Spectrum
nova
23. The layer of the sun just above the photosphere
radiation pressure
radiation pressure
Cepheid Variable
Chromosphere
24. 1 mm 1μm
Quasar
Electromagnetic Radiation: Infrared
blazar
Differential Rotation
25. 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
Umbra
synchrotron radiation
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.
26. N=are*Fp(Ne)(Fl)(Fi)(Fc)(L) N: number of civilizations possible to communicate with are*: rate solar-like stars are created Fp: fraction of stars with planets Ne: number of planets like ours Fl: fraction of planets with life Fi: intelligent life Fc:
Pulsar
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.
Drake equation
Photon
27. A planet that is farther from the sun than the Earth is
Superior planets
Big Bang
Gravitational Lens
Metals
28. The process of acquiring material
Kirkwood gaps
accretion
Black Hole
Thermonuclear Fusion
29. The study of the universe as a whole.
cosmology
Electromagnetic Radiation: Radio
Grand design spirals
Triple Alpha rocess
30. First accurately measured the speed of light in a vacuum
Liquid metallic hydrogen
Ole Roemer
terrestrial planet
Disk
31. A spectrum of light with energy at only a few wavelengths.
Lagrangian Razor
Emission Spectrum
AGN
fusion crust
32. A quantity measuring the stability of the Earth's atmosphere
Seeing
nucleus
gravity
Rich Cluster
33. The Greek philosopher responsible for making the stellar magnitude scale.
Proton-proton chain
Superior planets
Hipparchus
Sa spiral galaxy
34. Matter that reveals itself only through its gravitational attraction.
Plank's Law
dark matter
Rich Cluster
opposition
35. Massive compact halo objects (MACHO) - weakly interacting massive particles (WIMPY's)
Turn off Point
Dark matter candidates
terrestrial planet
Limb darkening
36. Hurricane-like vortex in southern-hemisphere winds to north and south blow in opposite directions which keep it spinning and with no subsurface features like mountians it persists.
Blackbody
Jupiters red spot
radio lobe
density waves
37. A method of finding a star's distance from its absolute magnitude and spectral type or color.
Annular Eclipse
Spectroscopic Parallax
Plank's Law
Positive - Converge - Greater than 1
38. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
interstellar dust
chemical differentiation
neutrino
Spectroscopy
39. A technique using computer-controlled mirrors to sharpen images distorted by the atmosphere
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.
Active Optics
Hyashi track
Inverse Square Law
40. The north-south line passing directly overhead through the zenith.
Kuiper belt
reflection star clusters
Meridian
acceleration
41. Loops that trace the magnetic field as it erupts from a sunspot area and arches over to an adjacent area. They glow in the light of gas pouring out of corona and falling into photosphere.
Coronal Loop
dark energy
A family of radiant energy- includes light
protostar
42. A prominence seen against the disk of the sun
resonance
Filament
Planck time
If it is in a denser medium - such as glass - it will move slower
43. 1 mm 1μm
Electromagnetic Radiation: Infrared
CMB
Open - flat - and closed.
Extrasolar Planet
44. The gap inthe outer portion of Saturn's A ring
differential rotation
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.
Winter Solstice
Enke gap
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)
MOONS: roundest shape
Grand design spirals
How is winding dilemma solved?
synchrotron radiation
46. Why do Galaxies move very rapidly in the interiors of the dense clusters?
Kuiper belt
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Light Curve
critical density
47. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
opposition
molecular clouds
resonance
Plank's Law
48. An entity that is likely in the nucleus of most - if not all - galaxies.
Largest diameter
Drake equation
supermassive black hole
tectonics of Mars
49. The fusion process that turns three helium nuclei into a carbon nucleus
tectonics of Mars
Cassini division
Triple Alpha rocess
MOONS: most geologically active
50. The Greek philosopher responsible for making the stellar magnitude scale.
Hipparchus
Halo
nucleus
Penumbra