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Know your solar system! Use the website study and learn the different planets and where they are in the solar system.

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This science worksheet will teach your third-grade students about the planets in the solar system. Your young astronomers will name each of the eight planets and their order by reading from a list of clues. After completing this solar system worksheet, they will have learned the two planets that have rings, that Mercury is the closest planet to the sun, and more interesting facts about Earth and space science!

Penmanship Practice: Cursive

This workbook focuses on penmanship practice. In the process, she'll also get a head start on composition by using her new handwriting skills to write short stories and paragraphs.

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Solar System | Worksheet | Education.com

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This science worksheet will teach your third-grade students about the planets in the solar system. Your young astronomers will name each of the eight planets and their order by reading from a list of clues.

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Now that you know the planets and where they are, make a map of the planets on the ground as a class.

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NASA has just notified you that the Aliens have invaded Neptune and Uranus and taken control of them. Use the calculator to determine how many planets are left and the percentage of control the aliens have.

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Make math easy with our online calculator and conversion site. All of our tools covering finance, education, health, cooking, and more are free to use! Our easy to use calculators deliver fast, reliable results on any device. Give it a try now!

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The aliens have quickly taken out Saturn and Jupiter and are now moving through the asteroid belt. Using the article below, come up with things you think might stop the aliens.

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Within the main asteroid belt, scattered in orbits around the sun are bits and pieces of rock left over from the dawn of the solar system. Most of these objects, called planetoids or asteroids - meaning "star-like" - orbit between Mars and Jupiter in a grouping known as the main asteroid belt.

The main asteroid belt lies more than two-and-a-half times as far as does from and contains millions of asteroids. Most of these are relatively small, from the size of boulders to a few thousand feet in diameter. But some are significantly larger.

How did the asteroid belt form?

Early in the life of the solar system, dust and rock circling the sun were pulled together by into planets. But not all of the ingredients created new worlds. A region between Mars and Jupiter became the asteroid belt.

Occasionally people wonder whether the belt was made up of the remains of a destroyed planet, or a world that didn't quite get started. However, according to NASA, the total mass of the belt is less than , far too small to weigh in as a planet. Instead, the debris is shepherded by Jupiter, which kept it from coalescing onto other growing planets.

Observations of other planets are helping scientists to better understand the solar system. According to a developing theory known as, in the first 5 million years of the solar system, Jupiter and are thought to have moved inward toward the sun before changing direction and heading back to the outer solar system. Along the way, they would have scattered the original asteroid belt before them, then sent material flying back to refill it.

"In the Grand Tack model, the asteroid belt was purged at a very early stage and the surviving members sample a much larger region of the solar ," John Chambers of the Carnegie Institution for Science wrote in a "Perspectives" piece published online in the journal Science.

Our solar system isn't the only one to boast an asteroid belt. A cloud of dust around a star known as zeta Leporis looks a lot like a young belt. "Zeta Leporis is a relatively young star - approximately the age of our sun when the Earth was forming," Michael Jura said in a. "The system we observed around zeta Leporis is similar to what we think occurred in the early years of our own solar system when planets and asteroids were created." A professor at the University of California, Los Angeles, Jura has since passed away.

Other also contain signs of asteroid belts, suggesting that may be common.

At the same time, studies of white dwarfs, sun-like stars at the end of their lifetimes, show signatures of rocky material falling onto their surface that suggest such belts are common around dying systems.

(Image credit: ISAS/JAXA)

Belt composition

Most of the asteroids in the main belt are made of rock and stone, but a small portion of them contain iron and nickel metals. The remaining asteroids are made up of a mix of these, along with carbon-rich materials. Some of the more distant asteroids tend to contain more ices. Although they aren't large enough to maintain an atmosphere, but there is evidence that some asteroids contain water.

Some asteroids are large, solid bodies - there are more than 16 in the belt with a diameter greater than 150 miles (240 km). The largest asteroids, Vesta, Pallas and Hygiea, are 250 miles (400 km) long and bigger. The region also contains the dwarf planet Ceres. At 590 miles (950 km) in diameter, or about a quarter of the size of our moon, Ceres is round yet is considered too small to be a full-fledged planet. However, it makes up approximately a third of the mass of the asteroid belt.

Other asteroids are piles of rubble held together by gravity. Most asteroids aren't quite massive enough to have achieved a spherical shape and instead are irregular, often resembling a lumpy potato. The asteroid 216 Kleopatra resembles a dog bone.

Asteroids are classified into several types based on their chemical composition and their reflectivity, or albedo.

C-type asteroids make up more than 75 percent of known asteroids. The "C" stands for carbon, and the surfaces of these extremely dark asteroids are almost coal-black. Carbonaceous chondrite meteorites on Earth have a similar composition, and are thought to be pieces smashed off of the larger asteroids. While C-type asteroids dominate in the belt, according to the European Space Agency, they make up only about 40 percent of the asteroids closer to the sun. These include subgroups of B-type, F-type, and G-types.

S-type asteroids are the second most common type, making up about 17 percent of known asteroids. They dominate the inner asteroid belt, becoming rarer farther out. They are brighter and have metallic nickel-iron mixed with iron- and magnesium-silicates. The "S" stands for silicaceous.

M-type asteroids ("M" for metallic) are the last major type. These asteroids are fairly bright and most of them are composed of pure nickel-iron. They tend to be found in the middle region of the asteroid belt.

The remaining rare types of asteroids are A-type, D-type, E-type, P-type, Q-type, and R-type.

In 2007, launched a mission, Dawn, to visit Ceres and Vesta. Dawn reached Vesta in 2011 and remained there for over a year before traveling on to reach Ceres in 2015. It will remain in orbit around the dwarf planet until the end of its mission.

While most of the asteroid belt is made up of rocky objects, Ceres is an icy body. Hints of organic material spotted by Dawn suggest that it may have formed farther out in the solar system before landing in the belt. While the organics have only been seen on the surface, that doesn't mean more material might lie on the dwarf planet.

"We cannot exclude that there are other locations rich in organics not sampled by the survey, or below the detection limit," Maria Cristina De Sanctis, of the Institute for Space Astrophysics and Space Planetology in Rome, told Space.com by email.

(Image credit: NASA/JPL-Caltech )

Asteroid mining

Asteroids have more than enough gold, plus other precious metals, to provide a few lifetimes' worth of fortunes. But there are plenty of other reasons asteroids are valuable. But how do we get these metals from these faraway asteroids? Perhaps the best way is to bring the rocks to Earth. Most of the metals we use in our everyday lives are buried deep within the Earth. And we mean deep: when our young planet was still molten, almost all of the heavy metals sank to the core, which is pretty hard to get to. The accessible veins of gold, zinc, platinum and other valuable metals instead came from later asteroid impacts on Earth's surface.

Those asteroids are the fragmented remains of almost-planets, but they contain all the same mixtures of elements as their larger planetary cousins - and you don't have to dig down into their cores to get it. But the main problem with asteroids is that they are far away. To launch from Earth's surface and go into orbit, a rocket needs to change its velocity from zero to eight kilometres (five miles) per second.

To rendezvous with an average asteroid, the rocket has to change its velocity by another 5.5 kilometres (3.4 miles) per second. That requires almost as much fuel as the launch itself, which the rocket would have to carry as dead weight, adding to the already-high cost of trying to set up a remote mining operation in the first place. And once the asteroid was mined, asteroid prospectors would be faced with a difficult choice: They could try to refine the ore right there on the asteroid, which would entail setting up an entire refining facility, or ship the raw ore back to Earth, with all the waste that would involve.

Building a belt

The main belt lies between Mars and Jupiter, roughly two to four times the Earth-sun distance, and spans a region about 140 million miles across. Objects in the belt are divided into eight subgroups named after the main asteroids in each group. These groups are the Hungarias, Floras, Phocaea, Koronis, Eos, Themis, Cybeles and Hildas.

Although Hollywood often displays ships making close calls through asteroid belts, the trip is generally uneventful. A number of spacecraft have safely traveled through the asteroid belt without incident, including NASA's New Horizons mission to .

"Fortunately, the asteroid belt is so huge that, despite its large population of small bodies, the chance of running into one is almost vanishingly small - far less than one in a billion," wrote New Horizons principle investigator. "If you want to come close enough to an asteroid to make detailed studies of it, you have to aim for one."

Within the asteroid belt are relatively empty regions known as Kirkwood gaps. These gaps correspond to orbital resonances with Jupiter. The 's gravitational pull keeps these regions far emptier than the rest of the belt. In other resonances, the asteroids can be more concentrated.

(Image credit: Getty )

Discovery of the asteroid belt

Johann Titius, an 18th-century German astronomer, noted a mathematical pattern in the layout of the planets and used it to predict the existence of one between Mars and Jupiter. Astronomers scoured the heavens in search of this missing body. In 1800, 25 astronomers formed a group known as the Celestial Police, each searching 15 degrees of the for the missing planet. But the discovery of the first body in this region came from a nonmember, Italian astronomer Giuseppe Piazzi: he named it Ceres. A second body, Pallas, was found a little over a year later.

For some time, both of these objects were referred to as planets. But the discovery rate of these objects increased, and by the beginning of the 19th century, more than 100 had been found. Scientists quickly realized that these were too small to be considered planets, and they began to call them asteroids.

Additional resources

You can read more about asteroids and the updated current asteroid count at NASA's Solar System Exploration asteroid page. Additionally you can learn more about the formation of the main asteroid belt in this article by Cosmos Magazine.

Bibliography

" Asteroids". NASA Solar System Exploration (2021).

" The Grand Tack". Southwest Research Institute.

" Forming Terrestrial Planets". Science (2014).

" UCLA Astronomers Identify Evidence Of Asteroid Belt Around Nearby Star: Findings Indicate Potential For Planet Or Asteroid Formation". University of California (2001).

" Asteroids: Structure and composition of asteroids". European Space Agency (2022).

" SwRI Scientist Studies Geology of Ceres to Understand Origin of Organics". Southwest Research Institution (2017).

" New Horizons Crosses The Asteroid Belt". Space Daily (2006).

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The main asteroid belt, between Mars and Jupiter, is where most asteroids orbit.

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The asteroid belt has slowed the aliens down, but they are still pushing forward. Play this game to practice your defense for our satellites.

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Shield these satellites from bad space weather!

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The aliens have made it to Mars, but they have stopped there. They are comparing Mars and Earth to get ready to invade our planet! Use the article below to discover the similarities and differences between Earth and Mars.

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NASA's real-time portal for Mars exploration, featuring the latest news, images, and discoveries from the Red Planet.

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Notice that water has different forms that it can be in. Using the link below, decide how the water can best be used to defend the Earth

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Water is a natural resource that is vital to the presence of life on Earth. Water exists in abundance on our planet Earth. However, only a very small fraction of it is fit for human consumption. Let us first understand the distribution of water on Earth. Study the pie chart given below.
Where is most of the water on Earth found?

About three-fourth of the Earth's surface is covered with water. That is why it is also called the water planet. But do you know how much water is readily available for use? Most of the water (about 97%) is in the seas and oceans as salt water. This water is too salty to be used for drinking and irrigation. Thus, only a tiny fraction (about 3%) of the Earth's water is available to us as freshwater. Out of this, 2.997% is locked up in the mountains or glaciers or is buried so deep under that it costs too much to extract. So, only about 0.003% of the fresh water is easily available to us in the form of groundwater, river, lake, stream, soil moisture, and water vapour.

Most of the water that exists on Earth is in the seas and oceans. Sea and ocean water is highly salty and hence unfit for drinking. Most of the fresh water is frozen in the glaciers and in the polar ice caps, and is thus not readily available. Only a small fraction of fresh water is readily available for use. Therefore, all of us must make an effort to use water judiciously.
FORMS OF WATER
In nature, water exists in three states. It could be in the form of liquid (e.g., rain, river, sea), solid (e.g., ice, snow, hail), or gas (e.g., water vapour).

You can heat water over a stove to convert it into vapour. What happens if you leave water in an uncovered vessel on a summer afternoon outside your house? After a few hours, you will find that the level of water in the vessel has decreased. This is because a lot of it would have escaped into the atmosphere in the form of water vapour. The process by which a liquid is converted to its vapour is called evaporation.

What about the reverse process? The process by which the vapour of a substance is converted to its liquidform is called condensation. Water vapour is also added into the air by the leaves of plants, through the process of transpiration. Evaporation and condensation of water take place on a very large scale on the surface of the Earth and its atmosphere. These processes play a key role in cloud formation and rain.

All the three states of water are also present in our natural environment at any given time.
Solid: Glaciers, icebergs, snow, hail, frost, and ice crystals in the clouds are solid forms of water.
Liquid: Rain, dew, and clouds are water droplets or liquid forms of water. Liquid water also covers three-quarters of the surface of the Earth in the form of lakes, rivers, and oceans.
Gaseous: Water vapour, fog, steam, and clouds are gaseous forms of water. Water exists in all the three states because water can change its state very easily in a range of temperatures, i.e., between 0°C (ice) and 100°C (vapour). This change also takes place on its own in our environment forming a cycle which we know as the water cycle.

WATER CYCLE
Water droplets in the clouds keep bumping against one another, and sometimes stick to form bigger drops. When these drops become too heavy to float in the air, they drop down back to the Earth as rain. The water that comes down as rain, in time, evaporates and goes up to form clouds again. This leads to form a cycle, known as the water cycle. It is also called the hydrological cycle. Water cycle is the cyclic movement of water from the atmosphere to the Earth and back to the atmosphere through various processes.

CLOUD FORMATION
When the temperature of air increases, it expands (i.e., its particles move away from one another). This makes the air lighter and it rises in the atmosphere, taking water vapour with it. As the air rises, it begins to cool. The water vapour condenses on dust particles present in the atmosphere to form millions of tiny droplets. Tiny ice crystals will be formed instead if it is very cold. This cluster of tiny water droplets floating in air is what we call a cloud.

Activity

Aim: To observe condensation of water.
Materials needed: A glass or metal tumbler, ice-cold water and a handkerchief
Method:

1. Take the tumbler and wipe it dry, both inside and outside.

2. Pour ice-cold water into the tumbler.

3. Wait for sometime and see what happens to the outer surface of the tumbler.

Observation: You will find that the outer surface of the tumbler becomes foggy with water droplets on it.
Conclusion: This is because water vapour in the atmosphere condenses on the cold surface of the tumbler.

Aim: To demonstrate condensation of steam.
Materials needed: A vessel with boiling water and a metal lid.
Method:

1. Ask an adult to boil some water in a vessel and carefully place the vessel on a table.

2. Hold the lid on top of the vessel so that the steam coming from the water touches it.

Observation: After a short while, you will find that the side of the lid facing the steam will have droplets of water.
Conclusion: This is because steam from the water condenses on the metal lid. The same can be done by holding a spoon over a steaming cup of water, tea, or coffee.

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What Are The Different Forms Of Water - A Plus Topper

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Different Forms Of Water On Earth Water is a natural resource that is vital to the presence of life on Earth. Water exists in abundance on our planet Earth. However, only a very small fraction of it is fit for human consumption. Let us first understand the distribution of water on Earth.

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You discovered the main difference! Earth has water! This could be the way you save the Earth! The supplies given to create a water defense system for your home.

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This day is to recap on what happened. Using the order of the planets, explain where the asteroid belt is in the solar system, the difference in Earth and Mars, and why you could not use the water to push the Aliens off of Mars.

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The water that you used defended Earth and every other planet behind it, but you cannot push them further back from Mars. Read the article below once again and decide why.

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NASA's real-time portal for Mars exploration, featuring the latest news, images, and discoveries from the Red Planet.