Category Archives: Class

Nuclear Fusion

At noon on a hot summer’s day, have you ever wondered how the Sun acquires so much energy that the light coming from it, 150 million kilometers away, can bring so much heat that it even burns your eyes and skin? The answer lies in hydrogen fusion happening in the Sun’s core. In its initial […] Continue reading

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The Diversity of Terrestrial World Atmospheres: Venus, Mars and Earth

Terrestrial planets’ atmospheres, including those of Venus, Earth, and Mars, are crucial to their general behavior and possible habitability. Many elements, including the planet’s distance from the sun, the makeup of its surface, and the presence of geological activity, all impact these atmospheres. The atmospheres of terrestrial worlds display a startling variation in behavior and […] Continue reading

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The Titius-Bode law

Titius Bode’s law is a fascinating concept in astronomy that has been intriguing scientists for centuries. This law is a mathematical relationship between the distances of the planets in our solar system from the Sun. It was first formulated in the 18th century by Johann Daniel Titius and later popularized by Johann Elert Bode. According […] Continue reading

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The International Space Station

The international space station is a collaboration that unites humanity to pursue the largest frontier, space. The ISS is the largest and most equipped space station humanity has ever had in space and provides opportunities to research exploration of space and how to help people back on earth. The ISS orbits the earth 386 kilometers […] Continue reading

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The (Possible) Oceans of Europa

Among all of Earth’s unique aspects and characteristics, the presence of water may be the most significant. Water is necessary to life as we know it; from humans ourselves down to microscopic organisms, all living things need water to survive. It is no wonder, then, that life in the Solar System is exclusive to Earth; […] Continue reading

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The Imaginary Planet

While the five planets visible to the naked eye have been known for almost all of astronomy’s history, it was not until the discovery of Uranus in 1781 by Sir William Herschel that astronomers began searching for other planets in our Solar System. After Neptune was discovered in 1846, astronomers began turning their telescopes towards […] Continue reading

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“How Stars Shaped Our Bodies and Our Home Planet”

A portion of a nearby galaxy is illuminated in this Hubble Space Telescope image by the remnants of a once-explosive supernova. (Image credit: NASA/ESA/HEIC/Hubble Heritage Team) Nearly every component of our body and the planet we call home was created inside stars. Heavy atoms like carbon, nitrogen, and oxygen are produced from lighter elements like […] Continue reading

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Time Dilation and the Theory of Relativity

With our totally unrestricted guidelines on Blog 4, I would like to make a bit of a deviation from the content of our course and discuss time dilation and the theory of relativity! When I first learned about time dilation, which refers to the difference in elapsed time as measured by different clocks due to […] Continue reading

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Blog #4 – Evidence for the Existence of Dark Matter

Dark Matter is a fascinating topic, yet we know so little about it. Regardless, a good amount of evidence exists that indicates dark matter is real. One pertains to the flatness of rotation curves for spiral galaxies at extended distances. The graph does not drop off, but rather, continues in (essentially) a flat rotation curve, […] Continue reading

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The Other Side of a Black Hole

Based on Einstein’s theory of relativity, black holes have a theoretical opposite know as “white holes”. Rather than it being impossible for matter to exit (as is the case with black holes), it would be impossible for matter to enter a white hole. Physically, it would look very similar to a black hole: the only […] Continue reading

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