The Northern Lights

Aurora Borealis, or the Northern Lights, is a natural phenomena that is observable at the North and South poles. Named by Galileo and meaning “Dawn of the North”, Aurora Borealis is  a visualization of the reaction between electrons from the Sun and our atmosphere. Due to our magnetosphere, most of the electrons are rejected, but some get through at the magnetospheres weakest points (the North and South poles). Once they are through the magnetosphere, the electrons begin reacting with the nitrogen and oxygen in the Earth’s atmosphere, where energy is transferred to the gasses atoms. After this transfer, the gas atoms discard the extra energy in the form of photons, creating a brilliant display of colorful light. Oxygen and Nitrogen react differently, and since they’re at different levels of the atmosphere, it becomes easy to determine where the reaction takes place. For example, when the electrons interact with oxygen, which is located in the first 150 miles of the atmosphere, the lights are more yellow. Beyond 150 miles, the color is more red, and below the 60 mile mark, which is the location of nitrogen in the atmosphere, the lights appear more blue.

 

The Northern Lights are a phenomena which have puzzled ancient civilizations and were mentioned numerous times throughout Norse folklore. The vikings were under the impression that the lights were the bridge to Asgard, some thought they were reflections from the shields of the Valkyrie, and in Finland they were thought to be the result of a battle between the Archangel Michael and Beelzebub. Due to the almost ethereal nature of the lights it becomes easy to determine how ancient civilizations, incapable of advanced astronomical research, were able to comes to the conclusions they did. Even now, with a scientific understanding of their origins, the Aurora Borealis remain one of the Earth’s most beautiful and fascinating natural occurrences.

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The Northern Lights

Aurora Borealis, or the Northern Lights, is a natural phenomena that is observable at the North and South poles. Named by Galileo and meaning “Dawn of the North”, Aurora Borealis is  a visualization of the reaction between electrons from the Sun and our atmosphere. Due to our magnetosphere, most of the electrons are rejected, but some get through at the magnetospheres weakest points (the North and South poles). Once they are through the magnetosphere, the electrons begin reacting with the nitrogen and oxygen in the Earth’s atmosphere, where energy is transferred to the gasses atoms. After this transfer, the gas atoms discard the extra energy in the form of photons, creating a brilliant display of colorful light. Oxygen and Nitrogen react differently, and since they’re at different levels of the atmosphere, it becomes easy to determine where the reaction takes place. For example, when the electrons interact with oxygen, which is located in the first 150 miles of the atmosphere, the lights are more yellow. Beyond 150 miles, the color is more red, and below the 60 mile mark, which is the location of nitrogen in the atmosphere, the lights appear more blue.

 

The Northern Lights are a phenomena which have puzzled ancient civilizations and were mentioned numerous times throughout Norse folklore. The vikings were under the impression that the lights were the bridge to Asgard, some thought they were reflections from the shields of the Valkyrie, and in Finland they were thought to be the result of a battle between the Archangel Michael and Beelzebub. Due to the almost ethereal nature of the lights it becomes easy to determine how ancient civilizations, incapable of advanced astronomical research, were able to comes to the conclusions they did. Even now, with a scientific understanding of their origins, the Aurora Borealis remain one of the Earth’s most beautiful and fascinating natural occurrences.

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Climate Change: 2018 4th Warmest Year

The Article

Climate change is one of the biggest threats mankind has to face, and it’s an issue that only grows in intensity over time. Last month, NASA and the National Oceanic and Atmospheric Administration highlighted the severity of this issue in a research article meant to explain the real dangers of climate change. NASA gathered data from all over the planet while researching this issue. They used 6,300 weather stations to measure surface temperatures in various locations. They also used ships and buoys to measure oceanic temperatures to see how they have changed overtime. The Arctic areas were heavily focused on as temperatures gathered in Arctic regions were found to be affected most. This large shift in Arctic temperatures has led to an increased rate of ice and glacial melting, causing an increase in sea levels. Along with an increase in sea levels, climate change can also cause an increase in natural fires, extreme weather events, and other natural disasters. The techniques used to gather and monitor temperature readings has changed throughout the years, but NASA is confident that their data is accurate, within 0.1 degree Fahrenheit.

 

The issue of climate change is one that doesn’t just affect this generation. It’s an issue that will worsen and cause irreversible problems for future generations. The rise in sea level experienced today could mean large scale displacement and flooding, spelling disaster for any coastal populations. In the past few years we have already witnessed the harsh effects of hurricanes and wildfire activity. It is important that the public is aware of climate change to work now to prevent it from worsening. This education also comes with the premise of voting for officials that are passionate about making a positive change in the way of taking care of our environment. This is an issue that cannot be ignored or swept under the rug,

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Climate Change: 2018 4th Warmest Year

The Article

Climate change is one of the biggest threats mankind has to face, and it’s an issue that only grows in intensity over time. Last month, NASA and the National Oceanic and Atmospheric Administration highlighted the severity of this issue in a research article meant to explain the real dangers of climate change. NASA gathered data from all over the planet while researching this issue. They used 6,300 weather stations to measure surface temperatures in various locations. They also used ships and buoys to measure oceanic temperatures to see how they have changed overtime. The Arctic areas were heavily focused on as temperatures gathered in Arctic regions were found to be affected most. This large shift in Arctic temperatures has led to an increased rate of ice and glacial melting, causing an increase in sea levels. Along with an increase in sea levels, climate change can also cause an increase in natural fires, extreme weather events, and other natural disasters. The techniques used to gather and monitor temperature readings has changed throughout the years, but NASA is confident that their data is accurate, within 0.1 degree Fahrenheit.

 

The issue of climate change is one that doesn’t just affect this generation. It’s an issue that will worsen and cause irreversible problems for future generations. The rise in sea level experienced today could mean large scale displacement and flooding, spelling disaster for any coastal populations. In the past few years we have already witnessed the harsh effects of hurricanes and wildfire activity. It is important that the public is aware of climate change to work now to prevent it from worsening. This education also comes with the premise of voting for officials that are passionate about making a positive change in the way of taking care of our environment. This is an issue that cannot be ignored or swept under the rug,

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Expanding a Trillion Dollar Industry

Many are familiar with mining on Earth to obtain resources that we use for all sorts of things on the planet. What many don’t know is that this process can be, and most likely will be, expanded beyond the planet. Asteroids contain many of the resources found on Earth since they are basically leftover material from the Solar System’s formation. Asteroid mining is an idea that is currently being explored by scientists and engineers in order to exploit the resources that can be found on these asteroids. Their size and type can vary, and the amount of resources that can be obtained is dependent upon these factors as well as their accessibility.

Image result for asteroid mining
Source: SYFY – Artist conception of asteroid mining

It will take a lot of money (billions) to even begin attempting this project. However, asteroid mining has the potential to be very lucrative as it is estimated that a relatively small asteroid can contain over $20 billion in just platinum. Since many asteroids cross Earth’s orbit during their journey through the Solar System and around the sun, they can be approached using a relatively low amount of fuel from our planet’s orbit. The first missions are loosely projected to be sometime during the 2020s. Planetary Resources is a company that “aims to be the leading provider of resources for people and products in space through its goal of identifying, extracting, and refining resources from near-Earth asteroids” and more information about their plans can be found on their website here.

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Mars: Investigating the Red Planet

In his hit song “Rocket Man”, musical legend Elton John aptly remarks that “Mars ain’t the kind of place to raise your kids / In fact it’s cold as hell.” The average surface temperature of Mars is 220 Kelvin, or about -64 degrees Fahrenheit. Now, I’m not sure about hell, but that’s definitely too cold to be raising any kids.

Gif Source: Giphy

For centuries, us humans have wondered about our next-door neighbor in the solar system: the red planet of Mars. Mars’ semi-major axis is about 1.5 times that of Earth, and Mars’ radius is only slightly more than half the size of Earth’s radius. Mars is the last of the four inner planets and the five terrestrial worlds; however, Earth is ten times more massive than Mars.

Mars is a truly fascinating world; from humongous volcanoes to polar caps of dry ice, the planet is a wonder to behold. Mars is too cold for liquid water today, but we have found evidence to suggest that Mars was a wet planet at some point in its history. Even if water was still around, human beings could not survive on Mars without a spacesuit due to low air pressure, freezing temperatures, little breathable oxygen, and the lack of an atmospheric ozone layer.

Though no human has step foot on Mars (yet), we have “visited” our neighboring planet with help from exploration rovers. There have been four successful rovers; in fact, the Opportunity mission was only recently terminated after working for 15 years and covering a total distance of just over 25 miles. As of now, the Curiosity rover is still active, and NASA is planning to launch a new mission in 2020.

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Oops, I accidentally welded!

Welding is the use of high heat to melt two metal pieces together so they fuse into one. It’s tricky and not a relaxing hobby done on the sofa while watching TV. It’s something that people take classes for and get certified for. In other words, it’s definitely a skill to be learned.

But sometimes it happens on accident. Let me introduce you to cold welding.

Image result for galileo high gain antenna
Galileo High Gain Antenna

This diagram shows the antenna of Galileo, which NASA launched in 1989 to gather data about Jupiter. Its special high gain antenna would transmit 134 kilobits per second back to Earth, and was tucked into an umbrella structure so it would be small and convenient for transportation. However, once it arrived at Jupiter, the antenna didn’t release as expected. Of the 18 ribs, only 15 released.

When a team went to work trying to figure out what happened, they discovered that some the rods were cold welded. The umbrella shaped antenna was packaged away before take-off, but some of the rods fused once they were in space.

Image result for galileo high gain antenna
What a fully deployed antenna would look like

Cold welding was first recognized in the 1940s. It’s the fusing of two pieces of metal without any applied heat, and happens when two flat metal pieces come in contact in a vacuum. It happened on Galileo because space is a vacuum.

“When the atoms in contact are all of the same kind, there is no way for the atoms to “know” that they are in different pieces of copper.” – Richard Feynman

Basically, it happens because the pieces are pressed so closely together that they fuse. Unlike traditional forms of welding, it requires no heat. It also requires the surfaces to be extremely clean. If any dirt, foreign atoms, or air molecules stand in the way, the metal pieces won’t join.

The European Space Agency published a 2009 paper declaring that spacecraft designers must consider this issue while working. There a number of possible preventative measures to take: selecting materials that won’t cold-weld, coating surfaces, lubricating moving materials, and reducing contact surfaces.

It’s a problem that aerospace engineers have to think about, but not anything to lose sleep over. It’s just something that designers have to keep in mind. Either way, it’s pretty cool that space can squeeze things together so hard that they become one!

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Hypervelocity Stars

In 2005, the first hypervelocity star (HVS) was discovered by Smithsonian astronomers. These objects are defined as stars with very high velocities compared to normal star velocities in a galaxy. Some of them have velocities that exceed the escape velocity of the galaxy. They are thought to originate from encounters of binary stars with the supermassive black hole at the center of the Milky Way Galaxy. One of the partners of the binary star is “captured” by the black hole, entering orbit around it, while the other partner escapes with a high velocity to become an HVS. In addition to the black hole origin of HVSs, it is also thought that HVSs can be induced by supernovas. In this case, a HVS is ejected from a binary system when the other partner undergoes a supernova explosion.

Diagram Showing Star Ejection from a Galaxy

As of 2014, there are 20 known HVSs. These HVSs all have masses a few times that of the Sun, though dwarf HVS candidates have also been discovered. There are so few confirmed HVSs because they are pretty difficult to track down. It’s not easy to search through a billion stars and find a couple that are moving abnormally. In order to locate them successfully, astronomers have used a specific type of telescope to focus on a large group of stars on the edges of the Milky Way’s black hole that had traveled a notable distance. They then were able to narrow down this large group to stars that were travelling at speeds consistent with ejection from the center of the Milky Way. Once we learn more about HVSs, we can use information about them to learn about stars that form in the centers of galaxies and the sizes of black holes at the centers of galaxies.

This link from Harvard contains a complete collection of links to general information, podcasts, scientific publications, and other links about hypervelocity stars. This article serves as a good introduction to the topic.

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The Sun – the heart of our solar system

the sunn

Planetary System

The star at the center of the solar system plays a special role for us here on earth. It was formed about 4.5 billion years ago, in the Orion spur (in the milky way galaxy). It was born from the collapse of a cloud and dust called the “solar nebula”. It then condensed into a burning ball of gas, called the sun.

What makes the sun the heart of our solar system?

  1. Its magnetic field
  2. Its gravitational pull.

The sun’s magnetic and gravitational impacts are largely due to its size. It is large enough to hold the solar system intact, it is about 100 earths wide, and it could theoretically fit all 8 planets nearly 600 times. Additionally, it contains about 99.8% of all the mass in the solar system.

If you are guessing that this is why planetary bodies orbit it, you are right. Because of its mass, it has a great pull on the fabric of space, creating a gravitational force that causes nearby bodies to be drawn towards it. Without this pull, the other planets will vanish into deep space.

The magnetic field of the sun is called the heliosphere, and it encapsulates the entire solar system. It protects the planets form harmful cosmic radiation. It is caused by the sun’s plasma, and it causes the pushing of particles towards its poles.

Will the sun last forever? Unfortunately not. It is expected to collapse into a white dwarf in about 6.5 billion years, after it runs out of its hydrogen fuel. That’s such a depressing thought. I hate to imagine what will happen to our existence as a result of this. Maybe we should think of ways to refuel the sun? Or maybe we should just refrain from worrying about things we cannot change. In the meantime, let’s enjoy the sun’s magnetic field, gravitational pull and vast amounts of energy.

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Radioactivity 101. Is the sun radioactive?

sun radio

sun spots and solar flares

Chemical reactions occur because atoms strive for stability. Just like the outer electrons require a certain number of electrons to become stable, the nucleus requires a certain number of protons and neutrons to achieve this stability. The decomposition (breaking down) of the nucleus to achieve this stability is what we call Radioactive Decay. An unstable nucleus can be referred to as a Radionuclide.

Why do atoms decay in the first place? Each nucleus contains protons and neutrons. If there are too many or too few of the neutrons, the core of the atom becomes unstable, leading to the decay of the radionuclide. 

How do we measure the rate of decay? We measure this by measuring the time it takes for exactly one-half of the radioactive substance’s nucleus to decay.  There are three types of decay, and each one is based off the radiation emitted through radioactivity. The three types are: alpha, beta or gamma decay. Our very own sun emits gamma rays, but unlike that of unstable nuclei, its rays are from solar flares.

 

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