* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
Download ITS3
History of Mars observation wikipedia , lookup
Aquarius (constellation) wikipedia , lookup
Tropical year wikipedia , lookup
Solar System wikipedia , lookup
Astronomical unit wikipedia , lookup
Rare Earth hypothesis wikipedia , lookup
History of Solar System formation and evolution hypotheses wikipedia , lookup
Geocentric model wikipedia , lookup
Extraterrestrial atmosphere wikipedia , lookup
Astrobiology wikipedia , lookup
Planets beyond Neptune wikipedia , lookup
Definition of planet wikipedia , lookup
IAU definition of planet wikipedia , lookup
Late Heavy Bombardment wikipedia , lookup
Planetary habitability wikipedia , lookup
Satellite system (astronomy) wikipedia , lookup
Dialogue Concerning the Two Chief World Systems wikipedia , lookup
Formation and evolution of the Solar System wikipedia , lookup
Extraterrestrial life wikipedia , lookup
USING IN SCIENCE IT: Information Handling Level 5 Pupil Notes ITS3 USING IT IN SCIENCE IT: Information Handling Level 5 Planets 2 ACTIVITIES Read the data sheet on The Solar System. 1 Create a database about Planets from the information you have been given. Use the following fields: Name of Planet (text field) Size (Earth 1) Temperature (°C) ) all numeric Distance from Sun (million km) ) fields Day Length (hours) 2 Sort the planets into DISTANCE FROM THE SUN starting with the closest. Save and print this list. 3 Sort the planets using SIZE into numerical order, with the smallest planet first. Save and print this list. 4 How many planets are larger than the Earth? Print this out. Explain how you used the computer to give you the answer: 5 Print the NAME and TEMPERATURE of those planets which have a temperature of more than 5°C. Data Sheet The Solar System - The Sun is, in fact, a star in the Milky \Nay. it is positioned in the “Orion Spur”, near the edge of the constellation, it takes 200 million years to complete one orbit of the constellation. The Sun is the only object in the solar system which gives off (radiates) light - all the others just reflect it. Our Sun is an average size star Sirius B is a dwarf star, whilst Antaris is a red giant, about 300 times larger than the Sun. if it were possible to drive a car around the equator of the Sun at 88 kph it would take 5.5 years to complete the journey non-stop! The Sun is shrinking at a rate of 1 metre every hour, but this may be an oscillation. Every 2 hours and 40 minutes the surface of the Sun pulses, travelling at kph, altering the diameter by as much as 10km. Viewed from Earth, the Sun has the same apparent size as the Moon, which makes eclipses possible. The Sun is 149 million km from Earth. The diameters at the equators and poles are roughly the same at 1,392,000 km. The Sun rotates once every 30 days and its mass is 332,950 times greater than Earth. its maximum surface temperature is 6100°C and this falls to a minimum of 3 870°C. Mercury Mercury is the second smallest planet in our solar system and is only 58 million km from the sun. its surface temperature averages 350C. it is difficult to see as it only rarely drops below the Sun’s disc. (The Earth is 2 ½ times larger than Mercury). its surface is battered into many craters formed by millions of meteors hitting it as they were drawn towards the Sun. in this respect it appears very similar to our own Moon, but it does not have the large flat areas which the Moon has. its only large flat area is called the Caloris Basin, which is over 1350 km in diameter (about the same length as Britain) caused by a very large impact. Mercury also has enormous vertical cliffs up to 3 km high and 480 km long. Astronomers think that these are relatively recent, as they cut through craters and other features. lt is believed that they were caused by the planet shrinking, as it is extremely hot on the side which faces the Sun and bitterly cold on the other. Mercury rotates slowly on its axis, its day length is 1461 hours. Venus In size and distance from the Sun, Venus is almost a twin of Earth. in fact, it is 9/10 the size of the Earth. it is easily spotted, as it is the brightest object in the sky after the Sun and Moon. its atmosphere consists of clouds of sulphuric acid, which makes it very different from our own. Venus is i08 million km from the sun and has a surface atmosphere of 480°C. About i 5% of its surface consists of mountains and lowlands, it has two vast upland areas: they are Aphrodite Terra, which is as large as Africa, and Ishtar Terra, which is the same size as Australia. The highest mountains on Ishtar Terra are more than 2 km higher than Everest. The surface has craters which are the result of impacts with meteors and volcanic activity. The 4 Pupil Notes ITS3 surface temperature is higher than that of Earth. Strangely, Venus rotates in the opposite direction to all of the other planets, a result, so some scientists believe, of a collision aeons ago. it has the lowest rotation time of any planet, its day length is 5832 hours! Earth Earth is the only planet in the solar system on which we are sure that life exists. This is because on Earth water can exist as a solid, a liquid and a gas. Water covers around 90% of the surface of the planet and the land masses move slowly on “plates”. The Earth moves around the Sun, so our position compared with other stars and planets changes, causing apparent movement in them. We are 150 million km from the Sun and our average surface temperature is 15°C. The planet is slightly pear-shaped with a small bulge in the southern hemisphere and an imaginary line called the equator separating the two hemispheres. Because the Earth tilts, we get seasons, as does Mars. There are ice caps at the poles on each, too. lt is the largest and most dense of the inner planets and has a mass equivalent to that of Pluto, Mercury, Venus, Mars and the Moon all put together. The Moon The Moon is not a planet - it is a satellite which circles the Earth, always keeping the same side towards us. it has dark areas called marias (seas) made from balalitic lava, and many craters. Other features are large crevasses called rules and bright streaks called rays. The Moon is covered in a coating of dust called regolith. It would take 81 Moons to have the same mass as Earth, and its gravity is about one-sixth of that experienced on Earth. The velocity of an object orbiting the Moon is about the same as a high-powered rifle bullet. So if you stood on a very high mountain and fired a bullet horizontally, two hours later you will have shot yourself in the back (if you stay there)! Mars Mars is a desert world which is very rich in iron oxide (rust). it is about half the size of the Earth. it has polar ice caps made from water and frozen carbon dioxide (dry ice - like they use in special effects at the theatre). Mars is 228 million km from the Sun and has an average surface temperature of -50°C. it is a tilted planet and therefore has seasons. in summer, enormous dust storms occur which can cover half the planet. On Mars is Olympus Mons, the largest volcano in the solar system it is the size of France and - Pupil Notes ITS3 5 three times higher than Mount Everest! Other volcanoes and craters exist on the surface. The canyon Valles Marineris is as wide as the USA. lt also snows on Mars - but it is frozen carbon-dioxide not water. / Asteroids (minor planets) Beyond Mars is the Asteroid Belt. Asteroids are divided into three main types. About 75% are C types which are carboniferous and very dark, i 4% are S types which are rust red, and 5% are M types which are metallic. (Others lie outside this classification). Shapes and sizes vary tremendously. Some like Victoria and Pallas have their own moon asteroids. Hektor is shaped like a peanut shell and thought to be two asteroids stuck together. it is believed that the gravity of Jupiter stopped these asteroids from forming into a planet. Jupiter Jupiter is the largest planet in the solar system, it is 11 times bigger than the Earth, with a mass over twice that of all the other planets combined. Jupiter is 778 million km from the Sun and has an average surface temperature of -1 50°C. lt consists mostly of hydrogen and helium, and savage storms, which can be seen from Earth, rage across its surface. The great ‘Red Spot’ is a permanent cloud of swirling, rising gas which was first observed in 1 655 and is twice as big as Earth. Jupiter gives out more energy than it gets from the Sun, due to its contraction which produces a strong magnetic field. This magnetic field’s radiation is strong enough to kill a person, and Jupiter generates plasmas which are hotter than the Sun’s core. The planet rotates faster than any other planet - it takes about 10 hours to rotate at its equator. Saturn Saturn is the second largest planet in the solar system, it is 9.4 times larger than our planet. it is encircled by a series of bright rings. Saturn is i 427 million km from the Sun and has an average surface temperature of -180°C. Like Jupiter, its visible surface consists of swirling clouds, it has a very low density, and if we could find a stretch of sea water which is large enough it would actually float! Despite its size, its gravity is less than Earth’s and it has a distinct bulge at the equator. Day length on Saturn is 10.3 hours. One feature is the aurorae on the surface - these are electromagnetic disturbances like the Northern Lights sometimes visible in Britain. Uranus Uranus is a greenish/blue planet, with the rarity of being ‘tipped over’ onto its side. Each pole is in sunlight or darkness for 42 years, and then they swap over. Uranus is 2870 million km from 6 Pupil Notes ITS3 the Sun. lt has an average surface temperature of -200°C. it too has minor rings like Saturn’s and winds which blow in the direction of the planet’s rotation have been discovered. Uranus is thought to have a large rocky core covered by a layer of ice and its colour is produced by an atmosphere containing large quantities of methane gas. Uranus is four times the size of the Earth but rotates much faster, it’s day length is only 10.8 hours. Neptune Neptune is 4497 million km from the Sun and was only discovered in 1 846. it has an average surface temperature of -220°C. The existence of Neptune was produced by mathematics. A wobble was detected in the orbit of Uranus, and so scientists started to look for a cause. Like Jupiter, it goes off more energy than it receives from the Sun, and it also has an atmosphere containing methane clouds. One cloud is as large as the Earth (‘The Great Dark Spot’). Neptune is 3.8 times the size of the Earth, and is also thought to have rings. lts moons orbit in the opposite direction to its own rotation. Neptune’s day length is 5.8 hours. Pluto in 1978, a moon of Pluto was discovered called Charon. Pluto itself was discovered in 1930 by astronomers searching for “Planet X” which was causing a wobble in the orbits of Neptune and Uranus. The earth is 5 times larger than Pluto. it is thought that Pluto and Charon may be escaped moons from Neptune, but no real proof exists. Sometimes Pluto is not the outermost planet. For periods of 20 years, its orbit takes it inside that of Neptune this happened in i 979, Pluto regaining its outermost position in 1 999. Pluto is 5900 million km from the Sun and is very cold with an average surface temperature of -2 40°C. -