A | B | C | D | E | F | G | H | I | J | K | L | M | N | O | P | Q | R | |
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1 | GROUP | SUBGROUP | CONCEPT | Grade | Subject | TextINFO | TextOBS | TextINQUIRY | TextREASON | TextMyth | VisWType | VisWText | VisWLabel | Satisfactory level | Remark | |||
2 | Earth | Properties | Spherical like a foot ball, flat at poles | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
3 | Earth | Properties | Blue color as viewed from space due to presence of water | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
4 | Earth | Properties | Presence of life due to water | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
5 | Earth | Motion | RotationL Spinning movement about an axis, Period 24 hours | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
6 | Earth | Motion | Revolution: Circling around the Sun, period ~365 days | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
7 | Earth | Motion | Revolution: Elliptical orbits | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
8 | Earth | Motion | Precession motion: Change in direction earth's axis of rotation, (like a top). Period 26000 years | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
9 | Earth | Duration of the Day time | Sun above horizon: Star at higher altitude stays above the horizon for a longer time than those below horizon | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
10 | Earth | Duration of the Night time | Sun below horizon: vice versa | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
11 | Pole Star | Located using nearby constellations, Ursa Major and Cassiopeia (North) and Crux and Centaurus (South) | 0 | 0 | 0 | 0 | 0 | 0 | 0 | |||||||||
12 | Earth | Pole Star | Used in navigation | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
13 | Earth | Poles | Geographic poles: two ends of axis of rotation | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
14 | Earth | Latitude | Equator: Plane perpendicular to axis of rotation passing through centre | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
15 | Earth | Latitude | Equator divides the sphere in two halves Norther/Souther Hemisphere | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
16 | Earth | Latitude | Circular slices parallel to the equator and perpendicular to axis of rotation | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
17 | Earth | Latitude | Represented in degree, Angle is subtended by two points on the same longitude to the center of the earth, with one point fixed at the equator. | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
18 | Earth | Latitude | Equator (0 deg), Tropic of Cancer (23.5deg North), Tropic of Capricon (23.5deg South), North Poles (90degN), South Pole (90degS) | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
19 | Earth | Latitude | Circumference of the equator is the largest and it decreases as we go to higher latitudes. | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
20 | Earth | Longitude | Lines joining two poles line the orange slices | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
21 | Earth | Longitude | Prime Medirean, referred as 0 hour longitude | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
22 | Earth | Longitude | Represented in units of time. 360 deg::24 hours, then 10deg: ?? | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
23 | Earth | Longitude | Day-Night line (12 hours) | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
24 | Earth | Longitude | Prime Meridean and Day-Night line | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
25 | Earth | Longitude | Distance between two longitudes decrease as we go from equator to poles | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
26 | Earth | Longitude | Local meridean: When sun passes over head | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
27 | Earth | Longitude | Time Zone: Local time varies | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
28 | Earth | Day-Night | Rotation of the earth about itself | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
29 | Earth | Day-Night | Side facing the Sun has day | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
30 | Earth | Day-Night | Side away from the Sun has night | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
31 | Earth | Day-Night | Period of rotation: The solar day (Time taken by Sun to cross the same position in the sky. | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
32 | Earth | Day-Night | Period of rotation: Sidereal day (Time taken by the earth to rotate by 360 deg.) | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
33 | Earth | Season | Tilt in the earth's axis | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
34 | Earth | Season | The revolution of the earth causes seasons to change. | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
35 | Earth | Season | Summer-Hemisphere tilted towards Sun | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
36 | Earth | Season | Winter- Hemisphere tilted away from Sun | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
37 | Earth | Season | Long Summer day: Sun at higher altitude. | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
38 | Earth | Season | Short winter day: Sun at lower altitude | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
39 | Earth | Season | Equal day and night: on Equinox. Sun overhead at the equator | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
40 | Earth | Season | Direct rays (overhead at noon) concentrated in small region | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
41 | Earth | Season | Inclined rays (lower altitude at noon) spread over wide region | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
42 | Earth | Sky color | Red color at horizon, (rayleigh scattering) red scattered less reach long distance | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
43 | Earth | Sky color | Blue color: blue scattered more spreads around. | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
44 | Earth | Aurorea | Illumination in the night sky near the Earth's poles, Aurora Borealis (Nort), Aurora Australis (South) | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
45 | Earth | Aurorea | They interact with Oxygen and Nitrogen in the atmosphere | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
46 | Earth | Aurorea | Illumination in the night sky near the poles | 0 | 0 | 0 | 0 | 0 | 0 | 0 | ||||||||
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