The Likelihood of Getting Hit with a Gamma-Ray Burst

A gamma ray burst is expected to hit Earth every 10,000 years to 1,000,000 years. How would this affect human society as we know it, why are gamma rays so dangerous, and can we do anything to stop it?

Gamma ray bursts are extremely energetic spouts of energy, and similar to visible light, are part of the electromagnetic spectrum. Unlike visible light however, gamma rays have significantly higher energy — a single gamma ray photon is more energetic than 1,000,000 photons from the visible light spectrum. This makes gamma rays a form of ionizing radiation: radiation that is strong enough to break chemical bonds.

Gamma rays were first discovered by a satellite sent into space by DARPA, with an original use-case of detecting Soviet nuclear space tests. While no bombs were detected, slight gamma bursts were, and a few years later they were found to be coming from distant galaxies.

There are two sources of gamma ray bursts. The first releases a ‘long gamma ray burst’ when the core of a massive star collapses to create a supernova. The second ‘short gamma ray burst’ occurs when a pair of neutron stars merge. Gamma ray bursts occur in jets as the magnetic fields of the objects forces material into cone like jets, and if the Earth were in one’s path, it would devastate the current state of life on the planet. With our current technology, we could do little to nothing to stop one from obliterating through the atmosphere, but the likelihood of getting hit with a jet-like stream is slim.

A black hole being formed releases a gamma-ray burst.

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Cool Parts of the Atmosphere of Venus

Venus captured by NASA

Composition of Venus’ Atmosphere

96.5% Carbon Dioxide

3.5% Nitrogen

Venus lacks a magnetic field. Its ionosphere separates it from outer space and the sun’s wind.

4 Billion Years Ago it is assumed that the atmosphere of Venus was a lot like earth’s atmosphere. There could have been liquid water. The area 50-65 km above the surface of Venus is the most Earth-like place in the solar system with breathable air that is like helium.

Troposphere

The troposphere is the densest part of the atmosphere. The troposphere has an atmospheric pressure strong enough that carbon dioxide turns into a supercritical fluid. A large amount of carbon dioxide and water vapor help create a strong greenhouse effect. This traps solar energy and increases the temperature.

Venus has an ionosphere. The ionosphere is related to temperature. The high ionization occurs on the dayside of the planet.

Venus has an induced magnetosphere. It is caused by the sun carrying solar wind.

Sources:Venus on Wikipedia

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Nuclear Fusion

DOE Explains Nuclear Fusion

Nuclear fusion is an incredibly interesting topic by which one of the most important parts of our solar system and cosmos utilizes constantly. In the core of our very own sun, hydrogen is converted into helium in a process known as nuclear fusion. In the sun and other stars, Nuclear Fusion reactions power this process by making the two lighter nuclei form into a single heavier nucleus. This then releases energy since the total mass of the resulting single nucleus becomes less than the mass of the two original nuclei. Albert Einstein’s famous equation (E=mc^2) helps to explain why and how this process happens. His equations partly states that energy and mass can be converted into one and other which further shows how this occurs. Nuclear fusion is also incredibly important in that it could be the future form and method that we utilize energy here on Earth. It is a far cleaner energy option than that of oil as it emits no greenhouse gases and could be a bright step in the future to taking care of our Earth. By safely using fusion reactions we can eliminate toxins and pollutants from our atmosphere and take care of our wonderful planet.

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Blog #3: Radioactive Decay and Radiometric Dating

Radioactive decay is one of the processes by which Earth produces heat. Radioactive isotopes start off unstable (these are called the parent isotopes), and so they decay into other, more stable daughter/progeny isotopes. The decay produces alpha, beta, or gamma radiation which is then converted into thermal energy. The decay of isotopes like uranium, thorium, and potassium provides a continuous heat source for heat, despite the fact that our planet has cooled since its formation. We can actually measure the rate at which these radiogenic decay processes are emitting energy through geoneutrino measurements! Geoneutrinos are the same as normal neutrinos except that they come from earth, and they can tell us information about which isotopes they were emitted by. Through neutrino geophysics we have found that about half all of Earth’s total heat flux comes from radioactive decay. (Gando et al., 2011)

We also use uranium, thorium, and potassium for our most common radiometric dating of Earth’s rocks. U-Pb is the most refined method of radiometric dating and is most often used to date zircon, as it can provide accurate ages for a span of 1 million to 4.5 billion years. Zircon is an incredibly durable mineral that can survive extremely high temperatures and practically any earth event. This and the fact that Zirconium does not form with lead (Pb) in it’s initial crystallization, makes U-Pb dating of zircon very accurate, and helpful for understanding the true age of a magmatic system. The oldest earth materials that we have found are the Jack Hills Zircons, found in a quartz conglomerate in western Australia, these zircons are 4.0 – 4.4 Ga!

Jack Hills Zircon showing zoning and U-Pb ages. (Research Gate)

We can also use K-Ar dating (potassium-argon) to find the crystallization age of igneous and volcanic rocks. This provides viable ages for 100,000 to 4 billion years. K-Ar dating is also pretty useful for archaeological dating of the rock record above or below artifacts because neither of the isotopes in the process are a product of human activity.

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What was Theia?

Ancient Planet Theia
Ancient Planet, Theia

Theia was about the size of Mars.

It orbited with Earth. 

It crashed into the Earth and the debris helped create the moon.

The core of Theia combined with the core of Earth.

Scientists disagree on this and some believe that it formed into multiple moons.

It is hypothesized to have orbited in the L4 or L5 position of Earth’s orbit.

It is believed that Jupiter and  Venus caused Theia to run into the Earth.\

Sources: Wikipedia, Planetpedia

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Solar System Formation and Coincidences

This graphic explains the general process of the formation of our solar system

Our solar system has many characteristics that can seem like odd coincidences. Why are all of the planets in the same orbital plane? Why are their orbits all nearly circular instead of being more eccentric? Why do they all orbit in the same direction around the Sun? The nebular theory of solar system formation, as well as the process of heating, spinning, and flattening, explain these coincidences using the simple, fundamental laws of physics. Starting with a large, low-density cloud of gas, it logically follows that it will collapse in on itself over time due to gravity. Because of conservation of energy, gravitational potential energy is converted into kinetic energy during the collapse, which is converted into heat as particles begin to collide. The center, being hot and dense, is where the Sun forms. Due to conservation of angular momentum, the once imperceptible rotation of the cloud speeds up as the cloud shrinks, and due to gravity and collisions, nearly all of the material spins in the same direction. Finally, collisions between clouds regulates the orbit of the materials and flattens the lump into a disk. We now have a flat disk of material spinning in nearly circular orbits in one direction. This explains the three “coincidences” that I mentioned at the start, and shows how you can often explain strange characteristics of the universe using basic laws of physics.

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Blog #4: Coronal Mass Ejections

CME 2017, NOAA

Coronal Mass Ejections are ejections of solar wind and plasma from our Sun’s corona. The blast from a Coronal Mass Ejection (CME), carries about a billion tons of material away from the sun at speeds ranging from 250 km/s to almost 3000 km/s. (NOAA) If they are directed toward Earth when they are ejected from the sun’s upper atmosphere, the fastest traveling CMEs can reach Earth in the matter of hours (15-18hrs) and the slowest take a matter of days. CMEs and solar flares are similar but don’t always happen at the same time, and scientists don’t entirely understand how they relate.

Important aspects of analyzing CMEs include size, direction, and speed. Knowing these can determine the likeliness of a CME affecting Earth and are determined from satellite imaging. CMEs contain radiation (specifically particle radiation that consists of protons and electrons) and are accompanied by geomagnetic storms. Both can have effects on satellites, spacecraft, and astronauts. Large CMEs can even interact with Earth’s magnetosphere, which would send some of the particle radiation into our upper atmosphere, causing dramatic auroras. (UCAR)

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Binary Star Collision

Picture of Star Collision from NASA

Binary stars were stars orbiting each other, and they might eventually collide due to the stellar mass loss or gravitational radiation which caused the decay of orbits. Stellar collisions could be amazing and rare, which happened once every 10000 years in our globular clusters. It was very likely, from scientists’ approximation, that a binary star system called KIC 9832227 would merge and explode in 2022. The mergence and collision would create the brightest light in the night. And the phenomenon would be visible with naked eyes, which could be spectacular! This phenomenon was predicted by Prof. Lawrence Molnar from Calvin College, who found that the period of variations in the binary stars was growing shorter in 2013 and made the prediction.

Let’s wait to watch that in three years~!!

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Composition of Planets within the Solar System

Picture of Solar System from The Nine Planets

Different elements were occupied in different planets within the solar system. Mercury, Venus, Earth, and Mars were terrestrial planets made of rocks, which were composed of diverse metal elements including magnesium and aluminum. Specifically, mercury obtained a thin exosphere of oxygen, sodium, hydrogen, helium, and potassium. Venus consisted of an iron core and a carbon-dioxide atmosphere. Our planet — Earth — was mostly (90%) made of silicon, iron, oxygen, and magnesium, which was similar to the composition of Mars as well. 

Jupiter and Saturn were gas giants, which mostly contained helium, hydrogen, and water. Simultaneously, Uranus and Neptune were ice giants, possessing water, methane, and ammonia fluid. In these two ice giant planets, it rained diamonds due to the separation of elements made of polystyrene, resulting in carbon dioxide atoms. Carbon was converted into diamonds at extremely high pressure within two planets.

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Blog Post 4 Chicxulub Impact

The Chicxulub Impact happened approximately 66 million years ago, defining the end of the Cretaceous Period and the beginning of the Paleocene, as well as the end of the Mesozoic Era and the beginning of the Cenozoic Era. This impact not only managed to eradicate the dinosaurs as the dominant lifeform on the planet but also managed to kill off 50 percent of all biodiversity.

Triceratops, one of my favorite dinosaurs, and an unfortunate victim to the mass extinction event at the end of the Cretaceous period. Credit to Fossil Facts and Finds.

This impact was caused by an asteroid that was approximately 10 kilometers wide and hit the Earth at 30 kilometers per second, producing 3*10^23 joules of force. The impact was so large that it kicked up debris across the entire world, producing ash clouds that blocked the sun for years before the emissions of CO2 put the world into a massive temperature spike.

Impact Crater at the Yucatan Peninsula in Mexico, credit to Wikipedia

It is theorized that this asteroid originated from the from the asteroid belt, although from where is up to debate. Some suggested but discredited theories on where it originated from were from the Baptistina group of asteroids in the asteroid belt or from the remnants of a comet. The most modern theory of the asteroid originating from the main asteroid belt was determined from simulations, probability, and high deposits of chromium and platinum isotopes at the impact crater.

The idea that the dinosaurs went extinct by an asteroid hitting them is a relatively new idea. In Disney’s Fantasia, it shows the dinosaurs dying off by heat wave, exhaustion, and climate change. This was the common theory until this impact crater was discovered. Initially found by Walter Alverez and his father Luis Walter Alverez, the high levels of iridium in the clay in the late 1970s. An oiling company hired Glen Penfield and Antonio Carmago as geologists to scout the area, where they noticed the ridge present near the town of Chicxulub extended into the ocean creating a circle. Further research in the area revealed pink granite and other igneous rock that only form deep inside the Earth, brought up to the surface.

Despite being the most recent mass extinction event, as well as being one of the most sudden and impactful (literally), the Earth’s natural forces of erosion, plant growth, and oceans had covered up one of the larger craters on its surface. There was even a town in the center of the crater without anyone realizing it. It was so well hidden that it took until 1991 for a paper to be published declaring it to be an impact crater. Unlike other planets like Mars and Mercury, Earth’s changing atmosphere and lifeforms can erode and erase crater impacts with little evidence left.

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