What s in Our Solar System?

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Transcription:

The Planets

What s in Our Solar System? Our Solar System consists of a central star (the Sun), the main eight planets orbiting the sun, the dwarf planets, moons, asteroids, comets, meteors, interplanetary gas, dust, and all the space in between them. The planets of the Solar System are named for Greek and Roman Gods and Goddesses.

Inner and Outer Planets Inner Planets: Mercury Venus Earth Mars Outer Planets Jupiter Saturn Uranus Neptune

The Sun The sun s energy comes from nuclear fusion (where hydrogen is converted to helium) within its core. This energy is released from the sun in the form of heat and light. Remember: Stars produce light. Planets reflect light. A star s temperature determines its color. The coldest stars are red. The hottest stars are blue.

The Planets of the Solar System Planets are categorized according to composition and size. The Inner Planets-small rocky planets (Mercury, Venus, Earth, and Mars) The Outer Planets-gas giants (Jupiter, Saturn, Uranus, and Neptune)

Characteristics of Small Rocky Planets They are made up mostly of rock and metal. They are very heavy. They move slowly in space. They have no rings and few moons (if any). They have a diameter of less than 13,000 km.

Mercury Mercury has a revolution period of 88 days. Mercury has extreme temperature fluctuations, ranging from 800 F (daytime) to -270 F (nighttime). Even though it is the closest planet to the sun, Scientists believe there is ice on Mercury. The ice is protected from the sun s heat by crater shadows.

Venus Venus is the brightest object in the sky after the sun and moon because its atmosphere reflects sunlight so well. People often mistake it for a star. Its maximum surface temperature may reach 900 F. Venus has no moons and takes 225 days to complete an orbit.

Earth Earth is the only planet known to support living organisms. Earth s surface is composed of 71% water. Water is necessary for life on Earth. The oceans help maintain Earth s stable temperatures. Earth has one moon and an oxygen rich atmosphere.

Earth s Moon It takes the moon approximately 29 days to complete one rotation. The same side of the moon always faces us. The moon s surface is covered in dust and rocky debris from meteor impacts. It has no water or atmosphere. The moon reflects light from the sun onto the earth s surface.

Mars Like Earth, Mars has ice caps at its poles. Mars has the largest volcano in our solar system: Olympus Mons. Olympus Mons is approximately 15 miles high. Mars appears red because of iron oxide, or rust, in its soil. Mars has two moons and takes about two years to complete an orbit.

Characteristics of Gas Giants They are made up mostly of gases (primarily hydrogen & helium). They are very light for their size. They move quickly in space. They have rings and many moons. They have a diameter of less than 48,000 km

Jupiter Jupiter is the largest and most massive planet. It s diameter is 11 times bigger than that of the Earth s. It takes about 12 years for Jupiter to orbit the sun. Jupiter has 16 known moons.

Saturn Saturn is composed almost entirely of hydrogen and helium. Saturn has many rings made of ice. Saturn s rings are very wide. They extend outward to about 260,000 miles from the surface but are less than 1 mile thick. Saturn has 18 known moons, some of which orbit inside the rings It takes Saturn about 30 years to orbit the sun.

Uranus Uranus is blue in color due to methane gas in its atmosphere. Uranus has 11 dark rings surrounding it. Uranus has 21 known moons and takes 84 years to complete one orbit.

Neptune Neptune has the fastest winds in the solar system: up to 2,000 km/hr. Neptune is also blue in color due to methane gas in its atmosphere. Neptune takes 165 years to orbit the sun and has 8 moons.

What keeps the Sun, Earth, and other planets in their orbits? Gravity What determines the gravitational force between two objects? The distance between the objects and the mass of the two objects

Exploring Gravity Lab

The Relative Size of the Planets in the Solar System