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GRADE-5-SCIENCE_REVISION_PAPER-THIRD_TERM-2014
GRADE-5-SCIENCE_REVISION_PAPER-THIRD_TERM-2014

... b. A Japanese word that means “harbor wave” is ________________ c. Our nearest star is ________________ d. The water in the air below its boiling point is called ___________________ e. The term that means turning water to water vapour is ______________ f. A natural body that moves around a planet is ...
Science 09 Space Review 1. Know what a light year is
Science 09 Space Review 1. Know what a light year is

... c) Why is a red giant hotter (in the core) than our sun? d) Why does a red giant collapse when fusion ceases? e) What is so bizarre about a neutron star? 12 km across and heavier than the sun 7. You should be able to work with numbers expressed in scientific and exponential notation. a) 2.5E3 = 2500 ...
planet
planet

... • "A planet is a celestial body that (a) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and (b) is in orbit around a star, and is neither a star nor a satellite of a planet." What would then qualify as a plane ...
Three Media Reports by Carole Gallagher
Three Media Reports by Carole Gallagher

1. The Sun has a surface temperature of about 6000 K.
1. The Sun has a surface temperature of about 6000 K.

... and metals. Out farther, ices could freeze onto the dust grains, so they got included in the planetesimals. In addition, the more massive planetary cores made of rocks, metals, and ices could pull gasses in. This made them even more massive. There are many asteroids, mostly outside of Mars’ orbit, a ...
TTh HW06 key
TTh HW06 key

... 1. Thermonuclear fusion reactions in the core of the Sun convert four hydrogen nuclei into one helium nucleus. The helium nucleus has A) less mass than the four hydrogen nuclei. B) the same mass as the four hydrogen nuclei. C) an undetermined amount of mass that depends on the temperature at which t ...
Kepler`s Second Law
Kepler`s Second Law

... 2.3b illustrate Kepler’s second law of planetary motion with the aid of a diagram 2.3c demonstrate an understanding of Kepler’s third law relating planetary distances to orbital periods and perform simple calculations using the formula: T 2 = R3 where T is in years and R is in AU ...
Stars from Afar
Stars from Afar

... An HR diagram shows the two most important characteristics of stars, which are temperature and absolute magnitude (brightness) and/or luminosity. ...
Fig. 16-7, p.363
Fig. 16-7, p.363

... • Planets like Earth are believed therefore to form as normal byproducts of stars forming • There are two types of planets in our solar system, Earth-like and Jupiter-like, results of a process we think we understand • Almost 200 planets have now been found around other stars, but those planetary sy ...
Lecture - UMass Amherst
Lecture - UMass Amherst

... 2. There are ~100 billion "Suns" in a galaxy like our own Milky Way Galaxy. 3.Astronomers can see billions of galaxies. ...
Document
Document

... heard? And how shall they hear without a preacher? 15) And how shall they preach unless they are sent? Just as it is written, "How beautiful are the feet of those who bring glad tidings of good things!" 16) However, they did not all heed the glad tidings; for Isaiah says, "LORD, who has believed our ...
SAP_Paper1_FutureOfUniverse
SAP_Paper1_FutureOfUniverse

... (Murray, C.D. & Dermott). While this end scenario of tidal acceleration is unlikely to actually happen we will see effects of the process. In 600 million years, tidal acceleration will have pushed the Moon’s orbit far enough from Earth that total solar eclipses are no longer possible (NASA). As the ...
Polarimetry & Star
Polarimetry & Star

... Distribution of Recycling Plants The "Initial Mass Function" (IMF) ...
Solar SyStem - Lorenz Educational Press
Solar SyStem - Lorenz Educational Press

... The Sun is a star made up of hot gases that explode with energy similar to that of a continuously exploding nuclear bomb. It is the center of our Solar System. It provides us with heat and light. The Sun has been spinning on its axis and exploding for about 5 billion years. The Sun is an average-siz ...
the Up2d8 Maths resource
the Up2d8 Maths resource

... Uranus ...
apparent magnitude
apparent magnitude

... • At a depth of about 10,000 km into Jupiter’s atmosphere, the pressure is high enough to change hydrogen gas into a liquid. • Deeper still, the pressure changes the liquid hydrogen into a liquid, metallic state. • Unlike most planets, Jupiter radiates much more energy into space than it receives f ...
Space+-+the+final+frontier
Space+-+the+final+frontier

... Uranus ...
Name - MIT
Name - MIT

... E) F type 37) For main sequence stars, the general rule is that the lower the surface temperature, … A) the greater the size of the core B) the greater the masses of the stars. C) the less luminous are the stars. D) the greater the diameter of the star E) the shorter the lifetime on the main sequenc ...
TRANSIT
TRANSIT

... to date, an exoplanet with a radius only 50% larger than the Earth and possibly having liquid water on its surface. Using the ESO 3.6m telescope, a team of Swiss, French, and Portuguese scientists discovered a super-Earth about 5 times the mass of the Earth that orbits a red dwarf, already known to ...
Vagabonds of the Universe
Vagabonds of the Universe

... • Vagabond- a person with out a fixed home who moves from place to place and has no apparent means of support, wander… • These objects do have fixed homes…. ...
Astronomy - Core Knowledge UK
Astronomy - Core Knowledge UK

... Lesson 1: The Universe and the Big Bang This lesson is the first in a series that introduces Year 4 children to the topic of astronomy. By its nature, this is both quite a difficult topic for children but also hugely fascinating. In this lesson, children will learn a bit about the origins of the Un ...
Teacher Resource Pack Unit Planning Resources
Teacher Resource Pack Unit Planning Resources

... much younger than our sun. Most of them apparently are not an isolated single star as our sun is but are part of systems of two or more stars orbiting around a common center of mass. So too there are other galaxies and clusters of galaxies different from our own in size, shape, and direction of moti ...
The Solar System and its Planets
The Solar System and its Planets

... and  Helium.    You  can’t   stand  on  it!   ...
Chapter 02 Earth in Space
Chapter 02 Earth in Space

... Chapter 02 - Earth in Space ...
Name - MIT
Name - MIT

... 37) The rings of energetic charged particles around Earth that are held in place by Earth's magnetic field are called the ... A) B) C) D) E) ...
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Timeline of astronomy

Timeline of astronomy around 2300 BC.
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