SUBJECTS
|
BROWSE
|
CAREER CENTER
|
POPULAR
|
JOIN
|
LOGIN
Business Skills
|
Soft Skills
|
Basic Literacy
|
Certifications
About
|
Help
|
Privacy
|
Terms
|
Email
Search
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 shadow area behind the Earth or Moon where the Sun is completely obscured.
Celestial Equator
Hipparchus
Umbra
hottest surface
2. An element of a highly efficient - two-dimensional electronic light detector
Pixel
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.
Hubble law
aphelion
3. A location on an H-are Diagram where evolving stars pulsate
Sa spiral galaxy
cosmic singularity
Instability strip
Jovian Planets
4. The science of measuring light energy by wavelength.
Spectroscopy
Kuiper belt
CCD
Absorption Spectrum
5. The distance light travels in one year (=9.46x10^12km).
Hipparchus
Seyfert galaxy
zone
Light-Year
6. Earth
roche limit
Halo
Most dense
Nucleus
7. The entity responsible for spiral arms in grand-design spiral galaxies
Density Wave
HII Region
Liquid metallic hydrogen
asteroid
8. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
Metals
The Local Group
matter dominated universe
3 reasons we orbit satellites to observe universe
9. What are the three possible geometries of the universe?
Neutron Star
Open - flat - and closed.
Flat - Remain Parallel - Exactly 1
radio lobe
10. Light-flaky crust - convective currents cause it to wrinkle and bunch (1/5 of surface). uniform cratering suggests lack of weathering and tectonics. volcanoes are flat due to atmospheric pressure.
quasar
Absolute Magnitude
Disk
tectonics of Venus
11. The trapping of heat by carbon dioxide or other gases in the Earth's atmosphere.
radiant
Corona
chemical differentiation
greehouse effects
12. Where is the center of the expansion
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.
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.
Dwarf planets
evidence of water on mars
13. A technique using computer-controlled mirrors to sharpen images distorted by the atmosphere
Big Bang
semimajor axis
Black Hole
Active Optics
14. Half of the longest diameter across an ellipse
asteroid
density waves
semimajor axis
Electromagnetic Radiation: Ultraviolet Light
15. A volume of space where few - if any - galaxies are located
Hubble law
Focal Length
MOONS: most geologically active
Void
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
Ionization
meteorite
scarp
17. Matter that reveals itself only through its gravitational attraction
Hydrostatic Equilibrium
supernova
Dark Matter
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.
18. Is space infinitely large?
19. All wavelengths of light emitted by a blackbody.
scarp
Blackbody Curve
Flocculent spirals
chemical differentiation
20. The final end state of a high mass star. .An entity for which gravity has completely overwhelmed all other forces of nature.
Black Hole
conjunction
great red spot
jovian
21. Ancient stream channels - flood planes - and sedimentary-type rock. Frozen water is found in the polar ice caps and in the soil.
density
Energy Level
Light: travels like a wave - detected like a particle
evidence of water on mars
22. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
epicycle
CCD
Focal Length
radio lobe
23. A spread of light with an uninterrupted wavelength distribution of energy.
Continuous Spectrum
Kuiper belt
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
Thermal Equilibrium
24. The Greek philosopher responsible for making the stellar magnitude scale.
Hipparchus
critical density
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.
Electromagnetic Radiation: Gamma Ray
25. 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.
general star population
disk
Occam's razor
Coronal Loop
26. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
Lagrangian Razor
meteor shower
Celestial Sphere
rotation curve=winding dilemma?
27. Venus
Winter Solstice
Penumbra
Eyepiece Lens
Thickest atmosphere
28. The powdered stone fragments that make up the lunar 'soil'
synchronous rotation
radio lobe
Emission Spectrum
regolith
29. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
epicycle
Plague
Asymptotic giant Branch Star
Grand design spirals
30. A telescope that uses mirrors to focus light
Parsec
Reflector
Drake equation
Focal Plane
31. Is there water on the moon?
quasar
Yes - frozen at the poles- remains protected from the suns rays
Oort cloud
Wein's Law
32. The process that powers the sun and hydrogen bombs
mapping the structure of Milky Way disk
Thermonuclear Fusion
Geocentric
MOONS: largest size
33. Latin for 'cloud'. A word used to describe the collections of gas and dust in the Milky Way and other galaxies
Nebula
Oort Cloud
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.
Astronomical Unit
34. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
neutrino
Make up of the terrestrial planets
Instability strip
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
35. The shadow behind the Earth or Moon where the Sun is partially obscured.
Trojan asteroids
radiant
Penumbra
Liquid metallic hydrogen
36. The mix of pure photon energy that emerged at the start of the universe.
cosmic fireball
Spectral Lines
Density Wave
Thermal Equilibrium
37. What Ole Roemer used to measure the speed of light in a vacuum
Eclipses of the Moons of Jupiter
planetesimal
Jovian Planets
dark energy
38. The class of all objects having high energy radiation coming from their nuclei. Active Galactic Nucleus- Blazars - Quasars - Radio and Emit synchrotron radiation
differential rotation
Drake equation
Europa (Jupiters moon)
AGN
39. Sa - Sb galaxies where two magnificent arms wind their way from nucleus out in a symmetrical manner.
Grand design spirals
Jovian Planets
superclusters
Photon
40. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
cosmological principle
Plank's Law
Main Sequence
Sunspot cycle
41. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Lagrangian Razor
Main Sequence
cosmic singularity
cosmological principle
42. The rate of expansion of the universe.
deferent
Hubble constant
Refractor
shape and color of SPIRAL galaxies
43. 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)
Annular Eclipse
Light: travels like a wave - detected like a particle
H2 Regions
density waves
44. A particle of light.
Quasar
standard candle
Celestial Sphere
Photon
45. The nuclei of very distant galaxies. Likely a manifestation of supermassive black holes
highlands
Europa (Jupiters moon)
Liquid metallic hydrogen
Quasar
46. The mass of an object divided by its volume
fastest rotation
density
Nova
Summer Solstice
47. A prominence seen against the disk of the sun
Filament
Thickest atmosphere
Main Sequence
differential rotation
48. A younger cluster of stars - found in the galaxy disk
Open Cluster
Grand design spirals
Blackbody
Dark Matter
49. The distance a moon can be from a planet before shattering from tidal forces
meteoriod
Maria
roche limit
Metals
50. VENUS
Dark Nebula
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
Interstellar Extinction
Neutron Star