Category Archives: Jovians

includes Jupiter, Saturn, Uranus, Neptune

Blog 3 – Uranus

Uranus is the 7th planet from the Sun, at approximately 19.2 AU away. It is primarily composed of hydrogen, helium, and hydrogen compounds. It is an ice giant, and its iconic pale blue-green color comes from methane. Sunlight passes through the atmosphere, and is then reflected by Uranus’ clouds. Methane absorbs the red within the […] Continue reading

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JUICE Explorer

As discussed briefly in class, the European Space Agency (ESA) just successfully launched the Juice (formerly JUICE: JUpiter ICy moons Explorer) mission on April 14th! I had no idea this mission even existed before it was mentioned, so I decided to explore it further. The goal of this mission is focused on Jupiter’s moons. While […] Continue reading

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The Great Red Spot

If you look for an image of Jupiter in any article or textbook, you’ll likely see the famous Great Red Spot in that picture. This immense storm on Jupiter’s surface is more than double the size of Earth, and has raged on for centuries. The incredible size and duration of the Great Red Spot begs […] Continue reading

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Blog #6: Detecting Extrasolar Planets

The photo above features the transit method of detecting extrasolar planets. Detecting extrasolar planets is a very delicate and challenging task for scientists. The distances between stars and relative sizes of stars compared to planets make it extremely hard to pick them out. Stars are also typically a billion times brighter than planets. There are […] Continue reading

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Lightning on Jupiter

How fitting that mysterious lightning has been observed on the planet named after the god of sky and storms! Lightning on Jupiter has been reported multiple times over the years during multiple space missions: the 1979 Voyager mission, 1990s Galileo Jupiter mission, and again during the 2007 New Horizons mission. Now that we’ve got Juno […] Continue reading

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Why is Jupiter the way it is?

Have you ever wondered why Jupiter looks so colorful? Well look no further than Jupiter’s atmosphere, where you’ll find similar and yet different features from Earth’s own atmosphere. Jupiter’s atmosphere consists of the thermosphere, stratosphere, and the troposphere, much like Earth’s atmosphere, yet where they differ is what each layer consists of. Jupiter’s thermosphere is […] Continue reading

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What is up with Io?

Today I wanted to talk about one of the most fascinating moons in the Solar System, Io is one of the four Galilean moons that orbits Jupiter, which are each large enough to be counted as planets or dwarf planets if they orbited the Sun. Io is covered in snow, and yet is by far […] Continue reading

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Determining Saturn’s Rotation Speed

Throughout the 1900s, planetary rotation speeds was generally measured in one of two ways: observing the frequency of which fixed features on planets’ surfaces appear, or observing the patterns of the magnetic field, which change periodically when the magnetic field isn’t aligned with the planet’s axis of rotation. For example, both Earth and Jupiter have […] Continue reading

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Blog #3 Formation of the Solar System

The formation of the Solar System is truly a testament to our good fortune of life being possible on a planet located in the “Goldilocks Zone” near the Sun. The initial conditions allowed for not only Earth to be composed of rocky elements such as carbon but for the Earth to be protected from flying […] Continue reading

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Lack of Cratering: Io and Europa

During class, we have discussed magnetospheres, tectonics, geological activity, and their relation to the cores of the “Big Five”: Earth, Venus, Mercury, the Moon, and Mars. Specifically the moon has very obvious cratering across its entire surface, and its craters remain intact for billions of years. This is due to it not having an atmosphere […] Continue reading

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