Can Elon Musk’s Dream Become a Reality?

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Human Habitats on Mars?, Mail & Guardian

Just last month, Elon Musk’s SpaceX used the worlds most powerful rocket, Falcon Heavy, to launch his personal red Tesla roadster into space, racing towards Mars. With a spacesuit-wearing dummy named ‘Starman’ at the wheel, the car is predicted to enter Mars’ orbit sometime in July, before exiting soon after. While Musk claims the purpose of this particularly launch was to ‘inspire humanity’, he has set a goal of having SpaceX flying people to Mars by 2024. These recent events have once again brought about the age-old curiosity of whether Mars can support human life.

While a journey to Mars could be accomplished in as little as 260 days, when the planet is at its closest point to Earth, there are many factors needing to be considered for the environment to be deemed livable for humans. For one thing, the planet’s air is mostly carbon dioxide and the level of gravity on Mar’s is only 38% of that of Earth’s. On top of this, the atmosphere is about 100 times thinner than Earth’s, which makes it far more difficult to trap heat energy. This has led to an average temperature on the planet of roughly -60˚C.  The air pressure is also significantly lower than is found even on the peak of Mount Everest. While these conditions may appear disconcerting, and a huge obstacle for any sort of human habitat on Mars, scientists have put much thought into ways around it. In fact just a couple of years ago, six companies began designing and creating possible habitat prototypes to sustain human life on the red planet.

For these habitats to prove successful, they have to overcome the perilous Mars conditions. This is not an impossible feat however, as in the same way that the various space stations orbiting Earth are sustaining life, scientists are confident in creating self sustaining habitats on Mars as well. To do so, they must ensure these environments are tightly sealed from the thin atmosphere, as well as sufficiently pressurized to mimic Earth conditions. Systems would also need to be utilized to collect solar energy to power the habitat. Another must for a sustainable habitat is a steady source of food and medical supplies, meaning scientists will have to find ways to grow produce in the low-sunlight and low-atmospheric conditions. For produce, plants can be protected from the tough conditions using pressurized green houses, as used on Earth. Farms can even be pressurized with the abundant carbon dioxide source found on the planet. The soil will need to be detoxified, however, to allow plants to receive their necessary minerals. Water is also a necessity, and so people would need to utilize the water found on Mars’ polar ice caps.  In terms of medicinal resources, artificial leaves made out of silicon have been invented to convert minimal amounts of sunlight into chemical reactions that power the creation of pharmaceutical and agricultural products.

While technology is not advanced enough yet to allow for entire human colonies to brave the Mars elements, it is seeming increasingly feasible for the creation of sustainable habitats for communities of scientists. While conditions will be very tough at first, creating a working environment for scientists would be the first step towards the realization of dreams held by those such as Elon Musk. The dream of humans stepping foot on Mars.

 

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Blog 4: The Sirens of Titan

One of my favorite novels is The Sirens of Titan by Kurt Vonnegut. As the title suggests a portion of the novel takes place on Saturn’s moon Titan, though this fiction is more concerned with the philosophical and not the realistic astronomical. I highly recommend it to fans of science fiction.

sirens
Cover Art by Jim Burns

Discovered in 1655, Titan is Saturn’s largest moon and the second largest moon in our solar system. Titan’s rotation is synchronously locked with Saturn and takes just under 16 Earth days to complete its orbit about Saturn. Its surface has been by liquid ethane and methane which make up rivers, lakes, and rain. The extreme cold, -179 degrees Celsius, means water acts like rocks and lava. The lack of craters on Titan’s surface indicate that it experiences erosive and tectonic forces similar to that on Earth.

Image result for titan's surface
Credit: ESA/NASA/JPL/University of Arizona

Titan is unique; it is the only moon in our solar system that has a thick atmosphere. Its atmospheric pressure is 60% greater than Earth’s and Titan’s smaller mass means its atmosphere extends 10 times higher off its surface. Its atmosphere is composed mostly of nitrogen and methane, which are split apart from high energy photons and particles. The split products than reform into organic molecules. Some of the heavier hydrocarbons fall to the surface becoming “sand” in Titan’s dunes.

Credit: NASA/JPL/Space Science Institute

In 1997 NASA launched the Cassini Orbiter and Huygens Probe on a journey to Saturn. Cassini achieved orbit around Saturn in 2004 and the Huygens Probe made its descent to Titan’s surface 6 months later. The Huygens Probe was constructed by the European Space Agency. Weighing approximately 700 pounds, the probe’s payload included 6 scientific instruments designed to collect data on Titan.  NASA Jet Propulsion Laboratory published a video showing animation of the craft’s descent as well as the camera footage it captured. Finally in September of 2017, the Cassini Mission ended when the Orbiter made its final descent into Saturn’s atmosphere.

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We Are Not Alone. (Probably)

 

 

Life: one of the most unique, hard to find things in the universe. We have so much life on Earth, but it’s often something we take for granted. In the 200,000 years humans have existed on Earth, we have not found any evidence of life outside of our planet. Considering how vast and diverse the universe is, there has to be some form of life somewhere else in the universe. The question among that majority of astronomers is no longer if we will find other forms of life in our universe, but when and where we will find evidence of this life.

Since astronomers have not yet perfected a technique to look into the future, the majority of research has been focused on where we will find evidence of new life. Humanities greatest bet at finding this evidence lies in finding a planet similar to Earth.

NASA did just this in 2015 with the discovery of Kepler 452b, also known as Earth 2.0. Kepler 452b-1,400 light years away from Earth-is approximately 6 billion years old and has an average orbit of 385 days while orbiting its star at the same distance as Earth. Due to these similarities, astronomers and botanists believe that plants from Earth could survive on Kepler 452b due to similarities in the light and atmosphere of the planet with ours. The planet has many other similarities to Earth including a rocky surface and active volcanoes, leaving scientists to believe that life may have once existed on this planet. While scientists have still not found evidence of life on this planet, there have been hundreds of similar planets discovered by Kepler which may be the key to finding other forms of life in our universe. All we need is a planet that formed similarly to Earth located in the ‘Goldilocks’ zone’ (perfect distance from the Sun to have water and an atmosphere with hospitable temperatures).

The idea of finding life in our universe raises a countless amount of questions. The real question that scares and excites me is what type of life we will find. Will it be simple? Complex? Peaceful? Hostile? Only time will tell.

 

 

 

 

 

 

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Nuclear PR

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Fukushima Protesters, 2013

The ability to harness nuclear fusion could revolution human society. From the time the universe was about twenty minutes to today, nuclear fusion has only been possible in extreme of environments. The blistering cores of stars, the supernovae explosions of red giants, and a handful of other celestial events were the only things that produced the temperatures in the millions required to make fusion possible. However, this may soon change. Although the idea of harnessing fusion has been theorized since the early 20th century, the only current practical use of fusion has been in thermonuclear weapons, the first of which was successfully tested in 1952. As time has passed, our understanding has become more nuanced and nuclear scientists now believe a functioning nuclear fusion reactor could be created “within the foreseeable future.” The amount of energy that could be harnessed with this is almost unfathomable. Fusion power could create a clean energy source that would replace dirty substances like coal and oil and generate enough power to drive rapid development in even the most underdeveloped of regions. However, even if fusion could solve all of man’s problems, there’s a problem fusion has before any reactor tests go live. Nuclear fusion may be fantastic, but the word nuclear itself carries a public relations albatross that could hamper its adoption.

Nuclear energy carries a massive stigma that would be hard for fusion energy to shake off. While humans have yet to harness nuclear fusion, nuclear fission has be a reliable source of energy for decades and has come under extreme scrutiny from both environmental and pacifist groups. When people hear the world nuclear, they do not think of the potential amounts of clean energy that can be created. They think of disasters of Three Mile Island, Chernobyl, Fukushima, and of course the two times that nuclear energy was used in combat, Hiroshima and Nagasaki. While it is arguable that the waste produced from fission is less destructive than our current rampant carbon dioxide emissions and that the nuclear disasters listed above are exceedingly rare, there’s no denying that nuclear energy become a polarizing topic. Fusion energy could change the world, but it going to have to defeat the public relations burdens that nuclear energy has incurred over the years.

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The Sun and the solar atmosphere.

Sun's structure
Source: Wikipedia

The solar system is special in that it only has one star, the Sun, while most other systems have at least 2 stars. Because the Sun is very important not only for maintaining the solar system, but also for providing energy to keep the lives on Earth, it is important to know what comprises of the Sun and what the solar atmosphere is.

The Sun is located at the center of the solar system, and keep other components such as planets, comets, and other mass orbiting around by the gravitational force caused by its large mass. The Sun is approximately 330,000 times heavier than Earth and its diameter is about 109 times longer than Earth’s is. The main components of the Sun is 73% of hydrogen and 25% of helium. Because the Sun employs nuclear fusions of hydrogen, which results in helium and larger energy, we can understand why the Sun is mainly comprises of hydrogen and helium, as a product of nuclear fusions.

The structure of the sun is also interesting to understand; the 6 layers of the Sun are called core, radiative zone, tachocline, convective zone, photosphere, and atmosphere. The innermost layer, the core is the place where most nuclear fusions occur, generating thermal energy to heat up outer layers of the Sun. The radiative zone is where energy from the core is transferred to outer layers through radiation. The tachocline is a transition zone between the radiative zone and the convective zone. The tachocline is hypothesized to be responsible for the magnetic fields of the Sun. The following layer is the convective zone, where the thermal energy is seized to be transferred through radiations, but rather through convective currents. The photosphere is the layer that the Sun becomes visible. Lastly, the atmosphere is where all other elements exist and very unstable as there are solar winds and flairs happening in this region.

Understanding the Sun’s structure and nature helps us understand more about the surrounding universe. The more we get to understand about the Sun, we will be more likely to understand other systems in the universe.

Source: Wikipedia

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The Sun and the solar atmosphere.

Sun's structure
Source: Wikipedia

The solar system is special in that it only has one star, the Sun, while most other systems have at least 2 stars. Because the Sun is very important not only for maintaining the solar system, but also for providing energy to keep the lives on Earth, it is important to know what comprises of the Sun and what the solar atmosphere is.

The Sun is located at the center of the solar system, and keep other components such as planets, comets, and other mass orbiting around by the gravitational force caused by its large mass. The Sun is approximately 330,000 times heavier than Earth and its diameter is about 109 times longer than Earth’s is. The main components of the Sun is 73% of hydrogen and 25% of helium. Because the Sun employs nuclear fusions of hydrogen, which results in helium and larger energy, we can understand why the Sun is mainly comprises of hydrogen and helium, as a product of nuclear fusions.

The structure of the sun is also interesting to understand; the 6 layers of the Sun are called core, radiative zone, tachocline, convective zone, photosphere, and atmosphere. The innermost layer, the core is the place where most nuclear fusions occur, generating thermal energy to heat up outer layers of the Sun. The radiative zone is where energy from the core is transferred to outer layers through radiation. The tachocline is a transition zone between the radiative zone and the convective zone. The tachocline is hypothesized to be responsible for the magnetic fields of the Sun. The following layer is the convective zone, where the thermal energy is seized to be transferred through radiations, but rather through convective currents. The photosphere is the layer that the Sun becomes visible. Lastly, the atmosphere is where all other elements exist and very unstable as there are solar winds and flairs happening in this region.

Understanding the Sun’s structure and nature helps us understand more about the surrounding universe. The more we get to understand about the Sun, we will be more likely to understand other systems in the universe.

Source: Wikipedia

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What are cosmic rays?

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an artist’s depiction of cosmic rays, TED-Ed

WHAT ARE COSMIC RAYS?

One of the more mysterious subjects from our last reading was that of cosmic rays.  To be quite honest, before encountering this in our textbook I had never considered cosmic rays outside of the context of the Marvel Universe.  But it turns out that cosmic rays are more than just a cool-sounding superpower – these signals from the cosmos impact our daily lives and could provide exciting new information about the universe.

Cosmic rays are high-energy “fragments” of atoms (subatomic particles such as electrons, protons, or pieces of nucleus) that zoom through the Universe.  Accepted scientific theory tells us that powerful cosmic events such as supernovae cause atoms to fragment into their constituent particles and shoot out across space.

Cosmic rays present a very interesting opportunity to scientists wishing to learn more about specific cosmic structures or events.  Usually, the only information that the Universe offers us comes in the form of electromagnetic radiation.  However, cosmic rays pose the opportunity for researchers to analyze matter that came (more or less) directly from these events.  Although several ongoing efforts to interpret cosmic rays have made significant progress, the interpretation of cosmic rays remains mysterious.

However, scientists know a great deal about the effect of cosmic rays on our everyday activities here on Earth.  Every second, we are being bombarded by cosmic rays that rain down through our atmosphere.  Cosmic rays are the primary culprit for static/white noise on the radio and television.  They are also to blame for many GPS and phone call errors.  Yet these pesky particles effect more than our electronics.  Some scientists believe that cosmic rays are responsible for genetic mutations and cancers.  But cosmic rays aren’t all bad!  In fact, can thank cosmic rays for the aurora borealis – the Northern Lights.

If you want to detect cosmic rays for yourself, I found a really cool DIY detector by Dr. Suzy Sheehie here.

Thanks for reading!

-Justin

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What is a pulsar?

pulsargif
cool pulsar gif, Amherst College
ns_pulsar_diagram
a useful diagram from NASA

 

 

 

 

 

 

 

WHAT IS A PULSAR?

Pulsars are some of the most interesting astronomical objects out there and are the subject of intense study by teams of scientists around the world.

Pulsars are rapidly rotating neutron stars that emit beams of intense energy from their magnetic poles.  Here, it is important to bear in mind that a neutron star is actually the super dense remnant of a massive star, after said massive star has dramatically collapsed via supernova.  These neutron stars (so called because they are composed almost entirely of atomic nuclei) possess a mass similar to that of our Sun, yet the radius of a typical U.S. city.  In fact, the density of a neutron star is so great that one teaspoon of a matter from a neutron star would weigh many millions (maybe even billions!) of tons here on Earth.

It is important to note that while all pulsars are neutron stars, not all neutron stars are pulsars.  A pulsar’s most defining property comes their rapid spin period.  Many pulsars will complete over 500 full revolutions in one second!  It is largely because of this insanely fast spin that the pulsars (composed of super-dense metals) exhibit extreme magnetic properties.  This, combined with the fact that pulsars are surrounded by fields of charged particles, causes blasts of radiation to be emitted from the magnetic poles of the pulsar.  Some neutron stars may not possess this spin rate or magnetic properties and thus are not pulsars.

Pulsars are most easily viewed from Earth using radio telescopes.  These stars get their name because they appear to “pulsate” or “blink” every time that one of their magnetic poles hits Earth with a beam of electromagnetic energy.

Interestingly, pulsars are now being used to study gravitational waves! (This is a super interesting topic… maybe I will blog about it later!)

That’s all for now – thanks for reading!

-Justin

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Astronomy with a Twist of History

As an anthropology major, it is cool to see my interest in archeology and what I’m currently learning in astronomy intersect through archeoastronomy. Archaeoastronomy is defined by dictionary.com as: “the branch of archaeology that deals with the apparent use by prehistoric civilizations of astronomical techniques to establish the seasons or the cycle of the year, especially as evidenced in the construction of megaliths and other ritual structures.”

One of my personal favorite examples of archeoastronomy is Stonehenge, mainly because it is still such a mystery.

 

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My best friend Caroline who took this photo when she visited Stonehenge two summers ago

Originally built around 5,000 years ago, today we know very little about who, why, or how it was built. However, one thing that is clear that Stonehenge is aligned with the movements of the sun – many people speculate that could be a major part of the role it played as a perhaps a religious epicenter but the truth is we just don’t know. That’s what makes it so fascinating – if only we could go back in time and ask!

 

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1 Shift, 2 Shift, Redshift, Blueshift

Space is vast. In fact, vast enough to contains many million, billions, and trillions of galaxies and other celestial objects. So the ultimate question is, how do scientists keep track of all of the celestial bodies? How do we know that the Andromeda galaxy is coming toward us if we can’t tell if it is growing in size by using naked eye observation? These burning questions, my friend, can be answered thanks to the rise of technology and advancements in practices.

From physics, we know that:

Velocity = Distance / Time

Therefore, if we were astronomers in the past, all we would have to do is determine the distance that a a star or a celestial object travels, and records the times at which we determined these distances, and, by subtracting the difference between the final and initial distance and final and initial time to find the velocity. For those of you who have taken calculus, this may look like:

velocity

Now that we have established what velocity is (and learned a bit of calculus), how is it that astronomers collect data on an object’s position in space?

In astronomy, there is something that is famously known as the Cosmic Distance Ladder. That is, given how far away an object or body is estimated to be, a certain method or device will be used to try and accurately gauge its distance. The distance ladder is shown below

distance ladder
Sourced from The University of California, Berkeley

If we look at the figure then we can see that, for example, we can accurately tell how far away an object in our solar system is by using RADAR and LIDAR. By using this method, scientists shoot radio waves into space and check how long it takes for them to bounce back. They then take the time and multiply it by the speed of light (since radio waves travel at the speed of light) to determine an object’s distance. So, if we really wanted to determine an object’s velocity in the solar system relative to us, we could use this technology to determine the distance away an object is to us at several different times. We would then use this to determine whether an object is moving toward or away from us, as well as how fast it is moving. If an asteroid is in the solar system, this could really help in determining whether or not it will strike Earth!

asteriod
Yikes! Sourced from the Dailystar

However, what happens when we just want to know velocity? Well, we look at a celestial object’s absorption spectra. An absorption spectra is all of the visible light that an object absorbs in space, thus why it is called an absorption spectra. The absorption spectra for the Sun looks something like this:

sun
Sourced from bhs4

Those black lines tell us all of the wavelengths that our Sun absorbs. We can use these lines to then determine if an object is moving toward or away from us. If an object is moving toward us, the lines will all shift the same distance to the right. This is known as RedshiftIf an object is moving away from us, then these lines move to the left the same distance. This is known as a Blueshift. We can then determine if an object has it’s spectral lines moved left or right by finding its absorption spectra when its not moving. Since elements each have their own absorption spectra, if we know the elements a object is made out of, then we can determine the absorption spectrum for that element when it is not moving. A visual example of red and blue shift looks something like this:

redshift
Sourced from the California Institute of Technology

Finally, why does this shift in spectra even happen? Well, if you’ve ever heard an angry person honk their horn continuously while passing you on the freeway, you’ve probably experienced something known as a Doppler Effect. The Doppler Effect essential states that anything wave at a velocity greater than 0 relative to you will slightly bend. Thus, when that person passes you, the sound waves get bent and the sound gets distorted. There is a great video by altshift that explains this better visually. Therefore, since light is a wave, light that is moving toward or away from us will become distorted and essentially change in wavelength. Thus, that is why we see the shift in wavelength to the left or right with Redshift and Blueshift.

Note, however, that objects on Earth move too slow for us to see this distortion of light. However, we can still hear distorted sounds thanks to the Doppler Effect. And so, I leave you with this: Video on Doppler Effect Using Trumpets

Featured Image Sourced From news.softpedia

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