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Space Interactive Internet Scavenger Hunt
Space Interactive Internet Scavenger Hunt

... death of a star, though no such star has yet been discovered, making it only a hypothetical possibility. Scientists believe it would take a star such as the sun over 14 billion years to reach the black dwarf stage, a period of time greater than the estimated age of the universe. If black dwarfs were ...
Edexcel GCSE - physicsinfo.co.uk
Edexcel GCSE - physicsinfo.co.uk

... One seismic wave has an average speed of about 10 km/s as it travels through the Earth. Using data from the graph, a scientist estimated the time that this seismic wave would take to travel down to the Earth’s core and back. ...
the Up2d8 Maths resource
the Up2d8 Maths resource

... Uranus ...
Space+-+the+final+frontier
Space+-+the+final+frontier

... Uranus ...
Exam 2
Exam 2

... The average temperature of Mars is less than that of Earth. What would be the relative wavelengths of the peak emissions of the infra-red spectra from these planets? a. The wavelength of peak emission from Mars will be at a longer wavelength than that from the Earth. b. The emission from the two pla ...
Name - reynardearthsci
Name - reynardearthsci

... a. The rock formed deep in the Earth’s interior. ___________ b. The rock is black and shiny. __________ c. Meteorologists have predicted a snow storm next week. __________ d. The rock cooled very rapidly. ___________ e. The record low temperature for this date was set in 1957. __________ 4. What typ ...
Lecture 3, PPT version
Lecture 3, PPT version

... The moon rises about 50 minutes later from one day to the next. New moon must rise and set with the sun (6am and 6pm), respectively. Full moon must rise when the sun is setting (6pm), and must set at sunrise the following day (6am). First quarter is mid-way between new and full, so it must rise at n ...
Unit 2 Study Guide (word)
Unit 2 Study Guide (word)

... one spin of a planet on its axis. As the planet spins half of the planet is facing the sun and the other half is facing away. The lit side is day and the dark side is night. The spinning of the planet is the reason we have day/night. A second motion is revolution. This is the motion of a planet arou ...
Unit 2 Study Guide - Grant County Schools
Unit 2 Study Guide - Grant County Schools

... one spin of a planet on its axis. As the planet spins half of the planet is facing the sun and the other half is facing away. The lit side is day and the dark side is night. The spinning of the planet is the reason we have day/night. A second motion is revolution. This is the motion of a planet arou ...
Class 11 and 12 lecture slides (giant planets)
Class 11 and 12 lecture slides (giant planets)

... This implies it is contracting at a rate of 0.4 km / million years ...
Unit 6: Space
Unit 6: Space

... SC.8.E.5.In.10: Recognize that the Moon's revolution around the Earth takes about thirty days. SC.8.E.5.In.9: Recognize that the four seasons are related to Earth’s position as it travels (revolves) around the Sun. SC.8.E.5.Su.7: Recognize that Earth revolves around the Sun creating the four seasons ...
TOPIC 14 – MOTIONS OF EARTH, MOON, SUN
TOPIC 14 – MOTIONS OF EARTH, MOON, SUN

... 37. Why does this deflection occur? _____________________________ 38. What are some examples of matter deflected with respect to Earth’s surface? __________________________________________________ Evidence of Earth’s Revolution Around the Sun 39. How long does it take the Earth to revolve around the ...
Formation of Solar System
Formation of Solar System

... Rotating solar nebula was gaseous and hot. The molecules move quickly and are ionised in collisions – thus a plasma of ions and free electrons forms. The motion of charged particles creates a magnetic field. The nucleus of the solar nebula thus had a magnetic field associated with it. Matter close ...
Geocentric Model of the Universe
Geocentric Model of the Universe

... Sunrise Noon ...
Astronomy Powerpoint
Astronomy Powerpoint

... nuclei into the nucleus of a helium atom, releasing a tremendous amount of energy. • During nuclear fusion, energy is released because some matter is actually converted to energy. • It is thought that a star the size of the sun can exist in its present stable state for 10 billion years. As the sun i ...
Document
Document

... Jupiter’s Moons • The 4 Galilean moons have small rocky or iron cores. They have similar densities to our Moon, indicating that each contains a thick layer of water and ice. ...
Celestial Sphere, Celestial equator, N
Celestial Sphere, Celestial equator, N

... The earth’s daily rotation makes the stars appear to rotate around us. Because we only see half the celestial sphere at any one place, this simple rotation of the stars looks more complicated and actually makes it appear that stars rise and set. The set of stars that rise and set varies with locatio ...
Interactive Tutorial Activities in ASTR 310
Interactive Tutorial Activities in ASTR 310

... C b has a larger diameter, takes less time that a to orbit describes the number of discoveries made by each method? and/or volcanic eruptions E) b receives more impacts than a so there is no way to D b has a smaller diameter, takes longer than a to orbit (a) about equal numbers using each method E b ...
Unit 6 – Earth
Unit 6 – Earth

... systems, if not the majority. They cannot see the planets; they are too far away, but they can detect the wobble caused by the gravitational pull of planets on a star. Distances in space are big, and are measured in light years. 1 light year is about 1016 m. The nearest star, Proxima Centauri, is 4 ...
PowerPoint Presentation - Planetary Configurations
PowerPoint Presentation - Planetary Configurations

... definitively:  Terrain on the Moon  Discovered satellites of Jupiter – a mini-solar system  Observed motion of sunspots implying rotation of the Sun  Observed phases of Venus that confirmed a prediction of the heliocentric model ...
Powerpoint 2003
Powerpoint 2003

... occasionally dotted with small black spots ...
Witnesses to Local Cosmic History - Max-Planck
Witnesses to Local Cosmic History - Max-Planck

... different materials, of course. The reason why the Kuiper belt objects form several main groups with different orbital characteristics is also only partially understood as yet. Four of these families are presently forced into their orbits by the gravity of the large outer planets. For two further gr ...
Solutions 1
Solutions 1

... For the sun to appear on the zenith an observer must live between the Tropic of Cancer and the Tropic of Capricorn or between +23½ o and -23½ o of the Earth's equator (celestial equator). This is the result of the 23½ o tilt of the Earth's celestial equator with respect to the ecliptic (the path of ...
COMMENTS ON HOMEWORK 1 In many cases the answer to a
COMMENTS ON HOMEWORK 1 In many cases the answer to a

... critical points were left unexplained or a few words preceded by a critically placed 'since' or 'because' were provided as a poor substitute for an answer. Take time to think through the explanation requested, and then write it out in your own words. Remember a neatly drawn diagram is often helpful. ...
Owsley Brown II Portable Planetarium K-2 Program
Owsley Brown II Portable Planetarium K-2 Program

... ● When objects collide, the contact forces transfer energy so as to change the objects’ motions. (4-PS3-3) ● The energy released [from] food was once energy from the sun that was captured by plants in the chemical process that forms plant matter (from air and water). (5-PS3-1) ● An object can be see ...
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Comparative planetary science

Comparative planetary science or comparative planetology is a branch of space science and planetary science in which different natural processes and systems are studied by their effects and phenomena on and between multiple bodies. The planetary processes in question include geology, hydrology, atmospheric physics, and interactions such as impact cratering, space weathering, and magnetospheric physics in the solar wind, and possibly biology, via astrobiology.Comparison of multiple bodies assists the researcher, if for no other reason than the Earth is far more accessible than any other body. Those distant bodies may then be evaluated in the context of processes already characterized on Earth. Conversely, other bodies (including extrasolar ones) may provide additional examples, edge cases, and counterexamples to earthbound processes; without a greater context, studying these phenomena in relation to Earth alone may result in low sample sizes and observational biases.
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