SOLAR SYSTE M SYLVIA MÁRQUEZ. INTRODUCTION Imagine a place where the sun shines 11 times brighter than in Earth. What would happen if scientists try to.

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Presentation transcript:

SOLAR SYSTE M SYLVIA MÁRQUEZ

INTRODUCTION Imagine a place where the sun shines 11 times brighter than in Earth. What would happen if scientists try to visit and investigate more about a planet such as Mercury? What would they do to protect a spacecraft sent to this planet? That’s what engineers had to do when designing the Mercury MESSENGER spacecraft. They covered the ship with sunshades that could protect the instruments from temperatures that reach 370°. The sunshades were made of a ceramic fabric from different elements: silicon, aluminum, and boron. This fabric was resistant to heat and reflected the sun’s heat away from the spacecraft, keeping it at a comfortable room temperature of 20°

ASSESS Why did engineers need to design a sunshade for Mercury MESSENGER? What other challenges do you think there would be for engineers designing a spacecraft to travel to Mercury? What challenges did engineers have to overcome designing a ship for a mission to Neptune?

VOCABULARY solar system astronomical unit planet dwarf planet planetesimals

WHAT MAKES UP THE SOLAR SYSTEM? Our solar system consists of the sun, the planets, their moons, and a variety of smaller objects. The sun is the center and the rest is orbiting around the sun. The force of gravity holds the solar system together.

DISTANCES IN THE SOLAR SYSTEM Distances in the solar system are so large that they cannot be easily measured in meters or kilometers. Instead, scientists use a unit called astronomical unit (AU) equal to the average distance between Earth and the sun. The distance between Earth and the sun is 150,000,000 kilometers The solar system extends more than 100,000 AU from the sun.

CONVERTING UNITS To convert from astronomical units (AU) to kilometers (km), you can multiply the number of AU by 150,000,000 Calculate: Mars is 1.52 AU from the sun. About how many kilometers is Mars from the sun? The answer is 228,000,000 km If you know the distance of the object from the sun, you can find its distance in AU. For example: Let’s say that there is a moon that is at a distance of 352,000,000 from the sun. Find the distance in AU. The answer is: 2.35 AU

AVERAGE DISTANCE OF THE PLANETS Find the distance of each planet in kilometers

DISTANCE FROM THE SUN These are the real distance in kilometers, check your answers. 150,000,000

THE SUN It is the center of the solar system. It is about percent of the mass of the whole solar system. Despite being more than a million times the volume of Earth, our sun is a very ordinary mid-sized star. There are stars that have volumes thousand times greater than our sun. This is a good thing, because large stars tend to burn and die quickly, but our sun will last for five billion more years.

PLANETS There are many different objects in the solar system In 2006, astronomers decided that a planet must be round, orbit the Sun, and have cleared out the region of the solar system along its orbit The first four planets are small and are mostly made of rock and metal The last four planets are very large and are mostly made of gas and liquid

Each planet has a “day” and a “year” Its day is the time it takes to rotate on its axis Its year is the time it takes to orbit the Sun

DWARF PLANETS For many years, Pluto was considered the ninth planet in the solar system, but Pluto shares the area of its orbit with other objects Pluto is now considered a dwarf planet A dwarf planet is an object that orbits the Sun and has enough gravity to be spherical, but has no cleared the area of its orbit There are five dwarf planets in our solar system: Pluto, Ceres, Makemake, Eris, and Haumea As scientists observe more distant objects, the number of dwarf planets might grow

DWARF PLANETS

HOW DID THE SOLAR SYSTEM FORM? Scientists think the solar system formed about 4.6 billion years ago from a cloud of hydrogen, helium, rock, ice, and other materials pulled together by gravity The process began as gravity pulled the cloud’s material together The cloud collapsed and started to rotate, forming a disk Most of the material was pulled to the center As the material got tightly packed, it got hotter and the pressure increased Eventually, the temperature and pressure became so high that hydrogen atoms were pressed together to form helium This process, called nuclear fusion, releases large amounts of energy Once nuclear fusion began, the Sun gave off light and became a stable star Sunlight is one form of energy produced by fusion

NUCLEAR FUSION

THE PLANETS FORM Away from the Sun, planets began to form as gravity pulled rock, ice, and gas together The rock and ice formed small bodies called planetesimals Overtime, planetesimals collided and stuck together, and eventually, they combined to form all the other objects in the solar system

Inner Planets Most water evaporated, preventing ice forming Close to the Sun Comparatively, low in mass Small and rocky Gravity was too weak to hold on to light gases such as hydrogen and helium Outer Planets Greater distance from the Sun Cooler temperatures Ice formed, adding mass Gravity was strong enough to hold hydrogen and helium, forming the gas giant planets Beyond the gas giants, temperatures were even lower Ice and other materials produced comets and dwarf planets

WHAT’S IN THEIR NAMES Where in the solar system could you find Lewis and Clark’s guide Sacagawea, artist Frida Kahlo, writer Helen Keller, and abolitionist Sojourner Truth all in the same place? On Venus! In fact, almost every feature on Venus is named for a real, fictional, or mythological woman. In general, the person or people who discover an object or feature in the solar system get to choose its name. But scientists have agreed on some guidelines. Features on Mercury are named for authors, artists, and musicians. Many craters on Mars are named for towns on Earth. And most craters on Earth’s moon are named for astronomers, physicists, and mathematicians.

THE REST OF THE INFORMATION WILL BE GIVEN IN YOUR ORAL PRESENTATIONS