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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 small chunk of rock in space
meteoriod
SETI
reflection star clusters
Bulge
2. Venus
Chandrasekhar Limit
Liquid metallic hydrogen
hottest surface
Secondary Mirror
3. Extremely round - lots of liquid water - ice rafts on surface ACTIVE SURFACE
Focal Length
Ionization
Europa (Jupiters moon)
Coldest surface
4. The instant of time after the Big Bang when space and time obtained their characteristics. (t=10^-43 sec when gravity freezes out-instant when gravity started existing as a separate force)
Planck time
semimajor axis
Wein's Law
Plague
5. What do we think the actual fate of the universe will be and why do we think this?
Poor Cluster
molecular clouds
Big Crunch
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.
6. The family of radiant energy that includes light as a subset
Electromagnetic Radiation
Electromagnetic Radiation: Microwave
greehouse effects
direct motion
7. 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.
Jovian Planets
nova
Flare
cosmic fireball
8. The family of radiant energy that includes light as a subset
Roundest orbit
belt
Electromagnetic Radiation
greehouse effects
9. 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.
H-are Diagram
tectonics of Mars
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
10. A planet orbiting about a distant star
Proton-proton chain
Pixel
Extrasolar Planet
Disk
11. The Big Bang says that the universe has not existed forever. It had a distinct beginning about 14 billion years ago called the 'Big Bang'. Therefore light from any object more than 14 billion light years away has not had time to reach us. The other p
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12. The point in its orbit where a planet is nearest the sun
acceleration
Perihelion
Open - flat - and closed.
cosmological principle
13. 1 mm 1μm
Extrasolar Planet
open star clusters
Flat - Remain Parallel - Exactly 1
Electromagnetic Radiation: Infrared
14. Mercury
planetary nebula
difference between maria and highlands of the moon.
smallest diameter
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
15. A star that erratically and explosively brightens and dims
The Big Bang Theory
Emission Spectrum
Flocculent spirals
Nova
16. A star that blows itself apart
Supernova (You can be my supernova girl)
Halo
MOONS: largest size
Self-Propogating Star Formation
17. First accurately measured the speed of light in a vacuum
matter dominated universe
Ole Roemer
Corona
Main Sequence Stars
18. The displacement of spectral lines to redder colors caused by the expansion of the universe.
cosmological red shift
Cepheid Variable
radio galaxy
accretion
19. When the Sun is farthest south of the celestial equator (About December 22)
solar nebula
tectonics of Venus
accretion disk
Winter Solstice
20. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
Most dense
Flat - Remain Parallel - Exactly 1
Brown dwarf
Neutron Star
21. After stars form they pump light energy into surrounding gas causing it to heat up and glow (H2=ionized hydrogen - H1= neutral hydrogen in molcular couds)
Doppler Shift
CCD
Occam's razor
H2 Regions
22. A spinning neutron star
Pulsar
aphelion
Reflector
open star clusters
23. The faint glow of light left over from the Big Bang. cosmic microwave background are the photons that remain after the big bang that have not turned into matter.
CMB
planetesimal
standard candle
Blackbody
24. The crust of a meteorite caused by its entry into Earth's atmosphere
cosmic singularity
fusion crust
Disk
Eyepiece Lens
25. The universe is isotropic - homogeneous - and without beginning or end in time and space. If the universe is truly homogeneous then every line of sight will eventually end on a galaxy. If it has existed forever then there has been enough time for lig
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26. 10 cm -> 1 mm
Electromagnetic Radiation: Microwave
Astronomical Unit
general star population
Celestial Sphere
27. Centered on the Earth
Nova
most eccentric orbit
Geocentric
meteor
28. What Ole Roemer used to measure the speed of light in a vacuum
Electromagnetic Radiation
Refractor
Eclipses of the Moons of Jupiter
gravity
29. A small round distribution of gas surrounding a dying star
Spectroscopy
Electromagnetic Radiation: Microwave
radio galaxy
Planetary Nebula
30. The oldest grouping of stars - found in the galaxy halo
bulge
Globular Cluster
Ammonia - methane - and water
Liquid metallic hydrogen
31. Electromagnetic Radiation
A family of radiant energy- includes light
White Dwarf
Ground State
Light-Year
32. A collection of galaxies like the one the Milky Way belongs to
Cosmic Microwave Background
Poor Cluster
Photometry
roche limit
33. The amount an image is enlarged by a telescope
Magnification
Summer Solstice
Penumbra
Continuous Spectrum
34. The philosophical stand that says a simpler explanation is more likely to be correct than a complicated one.
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35. As open clusters age - they push gas away but dust remains this can reflect light giving the cluster a blue-ish color. also called reflection nebula
reflection star clusters
Oort cloud
critical density
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
36. A bridge of material held in position above the solar surface. They can remain for hours even days
homogeneous
Prominence
Milky way Galaxy
Electron
37. 100 nm 10 nm
Electromagnetic Radiation: Ultraviolet Light
density parameter
inferior planets
greatest elongation
38. When massive objects bend space and time enough to create multiple images of an object located behind them
fewest moons
fastest rotation
Gravitational Lens
meteorite
39. In Ptolemy's geocentric solar system - the large circle on which a planet's epicycle moved around the Earth.
Self-Propogating Star Formation
Flare
meteoriod
deferent
40. The law that describes the blackbody curve - and let to quantum mechanics.
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41. That which is responsible for Jupiter's magnetic field
Liquid metallic hydrogen
supernova
Dark matter candidates
Emission Spectrum
42. The process of acquiring material
cosmological red shift
Light Curve
accretion
isotropic
43. The imaginary sphere centered on the Earth that hols the stars.
jovian
Brown dwarf
Celestial Sphere
direct motion
44. The normal eastward movement of a planet against the background of hte distant stars.
radio lobe
Limb darkening
most eccentric orbit
direct motion
45. The Greek philosopher responsible for making the stellar magnitude scale.
Trojan asteroids
Red Giant
Planck time
Hipparchus
46. The law that describes the blackbody curve - and let to quantum mechanics.
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47. The process responsible for creating the arms of flocculent spiral galaxies
Self-Propogating Star Formation
Electromagnetic Radiation: Visible Light
300000 KM/sec
Filament
48. 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)
Continuous Spectrum
Photometry
mare basalt
How is winding dilemma solved?
49. The rotation of a star or planet at different speeds at its equator and poles
Apollo asteroids
differential rotation
Drake equation
gravity
50. The fusion process that turns three helium nuclei into a carbon nucleus
Hyashi track
homogeneous
molecular clouds
Triple Alpha rocess