Circumference and Diameter of the Earth

This view of Earth comes from NASA's Moderate Resolution Imaging Spectroradiometer aboard the Terra satellite.

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The Earth is the largest of the terrestrial planets in the Solar System, and the 3rd planet from the Sun. Are you looking for the circumference and diameter of the Earth?

The equatorial circumference of the Earth is 40,075 km. This is the distance around the equator of the Earth. If you measure the circumference of the Earth, while passing through the poles, the distance is only 40,007 km. This is because the Earth isn’t a perfect sphere. It’s rotating rapidly, which causes the equator to bulge out.

The equatorial diameter of the Earth is 12,756 km. This is the diameter of the Earth measured from one side of the Earth, passing through the center. If you go from pole to pole through the center, the distance is only 12,713 km.

We have written several articles about Earth for Universe Today. Here’s an article about the Earth’s magnetic field, and here’s an article about the surface area of Earth.

If you’d like more info on Earth, check out NASA’s Solar System Exploration Guide on Earth. And here’s a link to NASA’s Earth Observatory.

We’ve also recorded an episode of Astronomy Cast all about planet Earth. Listen here, Episode 51: Earth.

First Planet From the Sun

Planet Mercury
Planet Mercury

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The first planet from the Sun is Mercury, orbiting the Sun at an average distance of 57.91 million km. It’s also the smallest planet in the Solar System, measuring just 4,879 kilometers across. Mercury is named after the Roman god of commerce; he was the same entity as the Greek god Hermes – the messenger of the gods.

Mercury is a desolate, sun-baked world pockmarked by impact craters. It lacks any atmosphere, so the intense heat from the Sun escapes back into space on the planet’s night side. At noon on Mercury’s equator, temperatures can rise to 700 kelvin (426 °C), but on the night side of Mercury, it dips down to 100 kelvin (-173 °C). But Mercury isn’t the hottest planet in the Solar System; that’s actually Venus – its heat-trapping atmosphere boosts its temperature to 735 kelvin (461 °C).

Early astronomers didn’t even realize that Mercury was a single planet. They thought that it was actually two separate planets; one for when Mercury was seen after sunset, and another object for when it was seen in the morning before sunrise. Even the first rudimentary telescope couldn’t resolve the surface of Mercury, and it wasn’t until the first mission to pass Mercury in 1974, that astronomers could really see what Mercury looked like.

Mercury takes 88 days to complete one orbit around the Sun. Compare this to Venus, which takes 224.7 days, and Earth which takes 365.25 days. Since Mercury is the first planet in the Solar System, it has the fastest orbit, and then each planet has a successively longer orbit. Mercury’s day is almost as long as its year; 58.6 days.

It’s the smallest planet in the Solar System, but it’s the second densest. It has a density of 5.427 g/cm3. This is just after Earth, with a density of 5.515 g/cm3. Astronomers think that Mercury has a large metallic core, surrounded by a rocky mantle and a thin crust of rock. It doesn’t seem to have any active volcanism, but there might still be some venting of gasses which cont into a thin atmosphere around Mercury.

Mercury has no rings or moons.

We have written many articles about the first planet from the Sun. Here’s an article all about Mercury, and here’s some additional information about Mercury.

If you’d like more information on Mercury, check out NASA’s Solar System Exploration Guide, and here’s a link to NASA’s MESSENGER Misson Page.

We’ve also recorded an entire episode of Astronomy Cast all about Mercury. Listen here, Episode 49: Mercury.

Circumference of the Moon

Flying Across the Moon
Flying Across the Moon

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The equatorial circumference of the Moon is 10,916 km. And the circumference of the Moon in miles is 6,783 miles. So, if you wanted to drive your lunar rover around the Moon and return back where you started, you’d need to travel 10,916 kilometers.

Need some comparison? The equatorial circumference of the Earth is 40,075 km. That makes the size of the Moon’s circumference about 27.24% the size of the Earth.

The Moon isn’t the largest moon in the Solar System – it only has an equatorial radius of 1,737.4 km. The largest moon is Jupiter’s moon Ganymede, with an equatorial radius of 2,634 km. That means Ganymede’s circumference is 16,550 km; bigger than the Moon’s circumference by about 5,634 km.

Want some more measurements?

The circumference of the Moon in meters: 10,916,000 meters
The circumference of the Moon in centimeters: 1,091,600,000 centimeters
The circumference of the Moon in feet: 35,813,648 feet
The circumference of the Moon in inches: 429,763,780 inches

We’ve written many articles about the Moon for Universe Today. Here’s an article about the full Moon, and here’s an article about the atmosphere of the Moon.

If you’d like more info on the Moon, check out NASA’s Solar System Exploration Guide on the Moon, and here’s a link to NASA’s Lunar and Planetary Science page.

We’ve also recorded an entire episode of Astronomy Cast all about the Moon. Listen here, Episode 113: The Moon, Part 1.

Circumference of Saturn

Saturn

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The equatorial circumference of Saturn is 378,675 km (or 235,298 miles). Not that it’s actually possible, but if you wanted to drive your car around Saturn’s equator, that’s how far you’d have to travel. Just for comparison, the equatorial circumference of Earth is 40,075 km, so Saturn’s circumference is 9.4 times larger than the Earth.

Want to make the calculation for yourself? Well, the formula for calculating the circumference of a circle is 2 x pi x r, where R is the radius of the circle. The equatorial radius of Saturn is 60,268 km, so you can do the math yourself.

Of course, Saturn isn’t the largest planet in the Solar System, that’s Jupiter. Jupiter’s circumference is 449,197 km, or 1.19 times bigger than Saturn. And the largest object in the Solar System is the Sun, with an equatorial circumference of 4,379,000 km. That’s 11.56 times bigger than Saturn.

We’ve written many articles about Saturn for Universe Today. Here’s an article about what Saturn’s rings are made of, and here’s an article about how many moons Saturn has.

If you’d like more info on Saturn, check out Hubblesite’s News Releases about Saturn. And here’s a link to the homepage of NASA’s Cassini spacecraft, which is orbiting Saturn.

We’ve also recorded an episode of Astronomy Cast all about Saturn. Listen here, Episode 59: Saturn.

How Much Bigger is Jupiter Than Earth?

Jupiter compared to Earth. Image credit: NASA

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Jupiter is the 5th planet from the Sun, and the largest planet in the Solar System. How much bigger is Jupiter than Earth? Just to give you a sense of scale, Jupiter is 2.5 times more massive than all the rest of the planets in the Solar System combined.

Jupiter’s diameter is 11.2 times larger than Earth. In other words, you could put 11.2 Earths side-by-side to match the diameter of Jupiter.

And Jupiter’s volume is even bigger. It would take 1321.3 Earths to fill up the volume of Jupiter. In terms of surface area, Jupiter is 121.9 times bigger than the Earth. That’s how many Earths could be flattened out to cover the surface of Jupiter.

Jupiter has 317.8 times the mass of the Earth.

Even though Jupiter is an enormous, massive planet, it’s much smaller than the Sun. The Sun accounts for 99.86% of the mass of the Solar System. You could fit 109 Earths side by side to match the diameter of the Sun, and it would take 1.3 million planets the size of the Earth to fill it up.

We’ve written many articles about Jupiter for Universe Today. Here’s an article about pictures of Jupiter, and here’s an article about missions to Jupiter.

If you’d like more information on Jupiter, check out Hubblesite’s News Releases about Jupiter, and here’s a link to NASA’s Solar System Exploration Guide to Jupiter.

We’ve also recorded an episode of Astronomy Cast just about Jupiter. Listen here, Episode 56: Jupiter.

Circumference of Mars

Mars Closest Encounter
Mars Closest Encounter

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The equatorial circumference of Mars is 21,344 km (or 13,263 miles). This is the distance you would have to go if you wanted to travel completely around the equator of Mars.

You can calculate the Mars circumference on your own if you want. The equatorial radius of Mars is 3,397 km, so you can just use the mathematical formula, C = 2 x Π x Radius. Did you get the same answer?

And just for comparison, the equatorial circumference of Earth is 40,075 km. So the circumference of Mars is 53% of the circumference of Earth.

Like many of the planets in the Solar System, Mars is rotating on its axis, turning once every 24.6 hours. This rotation causes Mars’ equator to bulge out from the center of the planet. If you wanted to drive around the planet, passing through each of its poles, you would have a shorter journey because of this. This is called the meridional circumference, and for Mars, this is only 21,244 km.

We have written many articles about Mars for Universe Today. Here’s an article with some pictures of planet Mars, and here’s an article about the temperature of Mars.

If you’d like more info on Mars, check out Hubblesite’s News Releases about Mars, and here’s a link to the NASA Mars Exploration home page.

We’ve also recorded an episode of Astronomy Cast all about Mars. Listen here, Episode 52: Mars.

How Many Miles Around the Earth?

Planet Earth, as seen from Apollo 17 mission. Credit: NASA/)PL

Planet Earth, which we humans and all currently-known forms of life call home, is the third planet from the Sun, and the largest of the terrestrial planets. With a mean radius of 6,371 km (3,958.8 miles), it is slightly larger than Venus (which has a radius of approx. 6,050 km), almost twice the size of Mars (~3,390 km), and almost three times the size of Mercury (~2,440 km).

Basically, Earth is a pretty big world. But just how big if one were to measure it from end to end? If one were to just start walking, how many kilometers (and/or miles) would they have to go before they got back to where they started. Well, the short answer is just over 40,075 km (or just over 24,901 miles). But as always, things get a little more complicated when you look closer.

Continue reading “How Many Miles Around the Earth?”

What Type of Planet is Mars?

The Grand Canyon of Mars
The Grand Canyon of Mars

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“What type of planet is Mars?” is a question that many readers ask. Mars is one of the four terrestrial planets. Mercury, Venus, and Earth are the other three. All of the terrestrial planets are made up of rock and metals. The remaining planets are classified as the outer gas giants.

All of the terrestrial planets have the same basic structure: core, mantle, crust; although each layer differs in thickness depending on the planet. Mercury has an average density of 5.43 g/cm3. Earth is the only planet more dense than Mercury. Mercury most likely has a liquid core that is mostly an iron-nickel alloy. The core accounts for as much as three-fourths of the planet’s radius. There are no numbers available for how thick the mantle and core are. Venus has a crust that extends 10-30 km below the surface. After that, the mantle reaches to a depth of some 3,000 km. The planetary core is a liquid iron-nickel alloy. Average planet density is 5.240 g/cm3.

Even though we live on Earth, not everyone is aware of its density and the depth of the various layers of our home world. The crust thickness averages 30 km for land masses and 5 kilometers for seabeds. The mantle extends on to an additional depth of 2,900 km. The core begins at a depth of around 5,100 km and is in two distinct parts: the outer core of liquid iron-nickel alloy and the inner core which is a solid alloy of iron-nickel. Average planet density is 5.520 g/cm3. The final terrestrial planet is Mars. Mars is roughly one-half the diameter of Earth, which leads scientists to speculate that the core has cooled and solidified. The depth of the crust and mantle are not known for sure, but the average planet density is 3.930 g/cm3. While there are only four terrestrial planets in our Solar System, here is a report on how NASA is trying to find more in other star systems.

Since we are talking specifically about Mars, we will talk about the composition of the planet’s surface material. There are hundreds of volcanoes on the surface of Mars. Several are regarded as the tallest mountains in the Solar System. Without plate tectonics, these volcanoes erupted for millions of years. Those massive eruptions explain why the entire surface is covered in basalt that is high in iron content. The iron content in the basalt has interacted with the Martian atmosphere and oxidized. The iron oxide explains why the entire Martian surface is coated in a reddish dust.

Answering ”what type of planet is Mars” took us on a little bit of a tangent. Hopefully, it is a tangent that will inspire you to find out more about the Red Planet.

We have written many articles about Mars for Universe Today. Here’s an article about the gravity on Mars, and here’s an article about the size of Mars.

If you’d like more info on Mars, check out Hubblesite’s News Releases about Mars, and here’s a link to the NASA Mars Exploration home page.

We’ve also recorded an episode of Astronomy Cast all about Mars. Listen here, Episode 52: Mars.

Source:
NASA

What Type of Planet is Venus?

Venus Cloud Tops Viewed by Hubble
Venus Cloud Tops Viewed by Hubble

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Venus is the second planet from the Sun, and a virtual twin of our own planet Earth in many ways. But what type of planet is Venus? There are two major classifications of planets in the Solar System. There are the inner, rocky terrestrial planets and then the outer gas giants. Venus is a terrestrial planet.

The terrestrial planets are the 4 inner rocky worlds in the Solar System: Mercury, Venus, Earth and Mars. The word terrestrial comes from the root term “terra”, which is Latin for Earth. So the terrestrial planets are “Earth like” worlds.

And Venus is the most Earth-like planet in the Solar System. It has almost the exact same size, mass and density. Its composition is probably very similar to Earth, with a metallic core surrounded by a rocky mantle and a thin crust. The main difference between Earth and Venus is the incredibly thick carbon dioxide atmosphere, which raises temperatures on the surface of Venus to the point that it’s hot enough to melt lead.

But compare a terrestrial world like Venus to the gas giants like Saturn and Jupiter. The mean density of Venus is 5.204 g/cm3. While the density of Saturn is only 0.687 g/cm3. The density of Saturn is less than water, and it would float if you could find a pool large enough.

We’ve written many articles about Venus for Universe Today. Here’s an article about pictures of planet Venus, and here’s an article about how to find Venus in the sky.

If you’d like more info on Venus, check out Hubblesite’s News Releases about Venus, and here’s a link to NASA’s Solar System Exploration Guide to Venus. Finally, here’s a link to ESA’s Venus Express spacecraft.

We have also recorded an entire episode of Astronomy Cast all about Venus. Listen here, Episode 50: Venus.

What is the Center of the Earth Made Of?

The Earths interior (University of Chicago)

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We know the surface of the Earth is made of rock, we can examine it ourselves. But what is the center of the Earth made of? Well, reach into your pockets and pull out some coins. That’s roughly what the center of the Earth is made of.

The Earth is broken up into layers. The outermost layer is the crust- that’s what you’re standing on. About 30 km below your feet is where the next layer of the Earth, the mantle, starts. The mantle makes up the majority of the interior of the Earth, and its composed of heated rock under high pressure. But inside the mantle is the core of the Earth, and it’s made of metal.

The Earth’s core is broken up into two distinct regions. The inner core is a sphere of solid metal that measures about 2,440 km across. It’s believed to be comprised of 80% iron and 20% nickel. Surrounding this solid inner core is an outer core of liquid metal that extends for approximately another 2,000 km. Geologists believe that the movement of metal in the outer core gives the Earth its magnetic field, allowing compasses to work.

Needless to say, the center of the Earth is incredibly hot. Scientists estimate that the core of the Earth could get as hot as 7,000 kelvin, and about 5,700 kelvin at the border between the inner and outer cores.

We’ve written many articles about the core of the Earth. Here’s an article about how far down the center of the Earth is, and here’s an article about the center of the Earth.

If you’d like more info on Earth, check out NASA’s Solar System Exploration Guide on Earth. And here’s a link to NASA’s Earth Observatory.

We’ve also recorded an episode of Astronomy Cast all about planet Earth. Listen here, Episode 51: Earth.