A Year in Space

Just last month Scott Kelly finished what many of us would deem unbearable: spending a year in space. For almost an entire year, Scott Kelly lived with fellow Russian Cosmonaut Mikhail Kornienko on the International Space Station in order to see the effects that long durations in zero-gravity conditions have on the human body. Prior to this mission, the longest time periods in space that scientists have extensive data on were only around six months long, so doubling that time would give scientists a much better idea of the effects of space on humans. This mission and its implications go hand in hand with
NASA’s study on the possibility of sending year-in-space-crew-scott-kelly-hdhumans to Mars. For the next couple of years, scientists will study Kelly’s body and how it reacts to readjusting to Earth’s gravitational force and atmosphere. What makes this study even more interesting, however, is the fact that Kelly has a twin brother who spent the past year living on Earth. This adds a new dimension to this study as there is someone with very similar genes and characteristics to
compare the changes to. The main goals of this mission is to see how humans can adjust to long durations in space and what scientists can do differently to mitigate the negative effects. Although Kelly has returned safely to Earth, this mission is far from over. (Source: NASA)


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Jovian Moons…Alien Life?

One question that all humans are curious to find the answer to is: Are we alone in this universe? Based on pure numbers, it is highly probable that life exists elsewhere in the universe. Despite this high likelihood for extraterrestrial life, we have yet to find any evidence of life beyond Earth. There are billions of galaxies for which life could exist; however, we may not even have to look that far. Several icy moons exist in our Solar System that are thought to have significant bodies of liquid water beneath their surfaces, potentially making them habitable environments.

Jupiter’s moon Europa and Saturn’s moon Enceladus are two of the worlds that show the most promise. Europa is primarily made of silicate rock and has a water-ice crust and probably an iron-nickel core. Additionally it has an atmosphere that is composed primarily of oxygen. Most importantly, it is believed that a water ocean exists beneath the ice surface. Like Europa, Enceladus has an ice surface with a large subsurface liquid water ocean. Additionally, Enceladus has geysers in the southern polar region that shoot out water vapor, solid material, and other minerals into space. The geysers show that Enceladus is geologically active.

These Jovian moons show the most promise for extraterrestrial life in the universe. Several missions are currently being planned or proposed that would explore Europa or Enceladus. The most concrete of these plans is The European Space Agency’s  Jupiter Icy Moon Explorer which will launch in 2022 and study three of Jupiter’s moons including Europa. Below is a video from NASA that discuses how Europa could be suitable for life.

 


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Climate Change – A Political Battle

The Earth’s climate has undergone changes throughout its 4.5 billion year history. Most of these climate changes can be attributed to small variations in Earth’s orbit that affect the amount of solar energy that the planet receives. Recently, the Earth has begun to experience climate change at levels that was previously unprecedented. 97% of climate scientists agree that climate change trends over the past 100 years are very likely human-induced.

NASA describes how the evidence for rapid climate change is compelling and can be seen in numerous areas including: sea level rise, global temperature rise, warming oceans, shrinking ice sheets, declining Arctic sea ice, glacial retreat, extreme weather/temperature events, ocean acidification, and decreased snow cover.

Despite the evidence and overwhelming scientific agreement that human-induced climate change is a very real and important problem, we have had a difficult time enacting policy measures to combat it. Climate change (as well as science in general) has unfortunately become a political battle. Rather than enact common sense measures backed by science, politicians use climate change to argue whether corporate (energy industry) profits deserve to take precedence over the health of the environment. While it is unlikely that half of Congress does not actually believe in climate change; the fossil fuel lobby has ensured that climate change legislation does not get passed.

Senator Jim Inhofe, the chairman of the Senate Environment and Public Works Committee, has long argued that climate change is a hoax and has opposed any effort to reduce carbon emissions. Below, is a clip of Senator Inhofe questioning the science behind climate change.


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Mars One? More like Mars WHAT

Mars One is a relatively small organization with a big idea. Based in the Netherlands, Mars One’s mission is to send a group of people from Earth on a one way trip to Mars by 2027. This mission is a nonprofit and led by Bas Lansdorp, who announced this idea in 2012. However, Lansdorp more recently stated that his goal is not simply to send people to Mars, it is to create a new civilization on Mars, essentially. I’m honestly not sure what I think about this. While having people live on Mars would be extremely rad, purely because living on a planet besides Earth would be an insane accomplishment, I’m not sure how feasible it is. Critics agree. The mission has been harshly criticized largely due to the fact that the actual plan to send the people there has several flaws. More importantly, though, in my opinion is the ethical implications of the trip. If all the technicalities of the trip work, how will the people on Mars be governed? Will they simply follow the laws on Earth? What if the people on the trip are from different countries? Which laws will they follow? Also, starting a colony on Mars would be similar to the formation of a new country. Who will be the leader? Will there be a democracy, or will it be a dictatorship? These are the questions that are currently unanswered but that need to be carefully examined before the trip occurs. The answers to them have tremendous implications that need to be realized.

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Above is a picture of what the Mars One landing could look like if the project is actualized.


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Nuclear Fusion: Our Potential Savior?

Nuclear fusion is what powers main sequence stars to shine so brightly and for so long. In the most basic sense, nuclear fusion is the process in which 2+ atomic nuclei crash together. When this occurs with nuclei of lower masses, energy is released. However, the process isn’t as simple as it sounds. An extreme amount of heat is needed to cause nuclei to crash into each other, seeing as they naturally resist each other. While this is easy to do in the core of a star due to the naturally high temperatures, it is extremely difficult this process on Earth. However, if we are able to create a way to successfully harness the power of nuclear fusion on Earth, it could mean a solution to the energy crisis. The materials needed to perform the actual process of nuclear fusion are inexpensive and very plentiful around the world. Additionally, nuclear fusion would leave little to no waste behind, an issue that we are currently facing while harnessing other types of energy. Currently, we are struggling to figure out a way to create an environment hot enough for nuclear fusion to work without the material around it melting down. Hopefully in the future we are able to create a functional way to use nuclear fusion, seeing as it has countless benefits and few costs, something we have struggled to find in past energy harnessing techniques.

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Above is a picture of the Joint European Torus, which is an attempt made by Europeans at a fusion reactor.


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Terraforming Mars: Exploring The World Of Cosmic Cosmetics

If there is anything we have learned from observing the universe, it’s that Earth is incredibly unique. Of course, we could find out soon enough how utterly ordinary we are should we discover Earth-like planets bearing life beyond our Solar System, but until, we seem to be pretty special.

Nasa’s Kepler Mission has discovered tens of thousands of planets orbiting distant stars, and given the trillions of stars in the galaxy, we are bound to discover a host of new worlds that could support life now or in the future.

Until that day, our hopes of finding a new world within flying distance are pretty slim. Unfortunately, it looks like we are all stuck here on Earth with no hope of ever living on another planet…or perhaps not.

Terraforming: The What & The Why

As of now, we have not found a planet that could support human life in it’s current state, but what if we were able to give the planet a makeover, so that it could one day be called home to humans? This is the fundamental question behind terraforming.

Terraforming is the process of making a planet more Earth-like, usually in the hopes of that planet supporting “Earthlings.” The subject has been written about in science fiction for more than a century, but terraforming has been discussed outside the realm of fiction in recent years.

Terraforming On Mars

In 1973, Carl Sagan published an article entitled Planetary Engineering On Mars, which suggested two different ways of making the red planet a world that could support human life (this was a “sequel” to his article on how to terraform Venus, published in 1961). Both theories involved melting the polar ice caps of Mars to cool the planet and ultimately make it more habitable.

In 1976, shortly after Sagan’s article, NASA published a study called “On The Habitability of Mars: An Approach to Planetary Ecosynthesis.” In addition to Sagan’s suggestion of melting the polar ice caps, NASA suggested that the introduction of greenhouse gases could both revive the planet’s atmosphere and warm the planet to livable temperatures.

Currently, NASA is hoping to get a manned mission to Mars within the 2030’s, which means we may be seeing the events of Hollywood’s recent hit, The Martian, play out in reality.

However, the day when astronauts can remove their helmets and weighty space gear is likely far off, especially in light of recent news.

The Snag(s) In An Already Daring Plot

If changing the livability of an entire planet did not seem daunting enough, recent research of Mars suggests that making the planet inhabitable may be even harder than expected. Until recently, scientists suspected that a large portion of the CO2 that previously occupied Mars’ atmosphere was absorbed by rocks on the surface. However, recent MAVEN data suggests that once the magnetic field of the Red Planet disappeared some 4.2 billion years ago,  solar winds stripped Mars’ atmosphere of most of its CO2, hurling the gases into space never to return.

With little to no CO2 to harvest from the crust of Mars, we would have to explore other ways of getting that much gas into the atmosphere. Science aside, putting astronauts in space is expensive enough, let alone sending them to Mars. It’s questionable whether all the money in the world could purchase the resources necessary to rebuild a planet.

Fear not would-be colonists. Although terraforming is difficult, it is not impossible. The human population has already influenced Earth’s atmosphere to a certain extent, so we know that terraforming is possible in some capacity. Because terraforming Mars has turned out to be trickier than previously thought, others have advocated for seeking other options for our next planetary home, namely Venus. While Venus does show some promise, such as a pre-existing atmosphere and a closer gravitational force to our own, the planet does present its own set of challenges.

Conclusion

While terraforming seems almost as difficult as finding an inhabitable planet, the field does show promise. Although we may not be the generation to leave our world to inhabit another, terraforming, at the very least, is being discussed seriously in the scientific community, and perhaps one day, those discussions will lead to mankind leaving this world for another.

For further reading, check out The Definitive Guide To Terraforming. A lot of the information and inspiration for this post was derived from this article.

Featured image courtesy of Pics About Space. Artist credit: Daein Ballard, CC BY-SA


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Plate Tectonics on Mars?

Active tectonic activity, as opposed to past and currently extinct activity, was thought to be limited to Earth among the terrestrial worlds. Tectonic plates on Earth cause activity such as earthquakes and volcanoes as well as mountain-building as they move atop the asthenosphere and recycle geological materials. However, UCLA scientist An Yin discovered evidence of plate tectonics on Mars.

Yin analyzed satellite images captured by the Mars Odyssey spacecraft’s Thermal Emission Imaging System (THEMIS) and the Mars Reconnaissance Orbiter’s High Resolution Imaging Science Experiment (HRISE). He analyzed one hundred satellite images and found characteristics indicative of tectonic plate activity such as flat canyon walls and cliffs that resembled those generated by faults on Earth.

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An image of Valles Marineris composed by Robert L. Hunt. Valles Marineris, a long trough system on Mars, appears to have been formed through geological processes connected to tectonic plates such as rifting and strike-slip faulting. 

However, compared to the activity on Earth, the plates appear to be much less active. Mars’ small size and less thermal energy contributes to this significantly slower tectonic activity. And while Earth has seven major tectonic plates, Yin believes that Mars has only two plates.


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Olympus Mons

mars-olympus-mons

Mars is the home of the largest volcano in the Solar System: Olympus Mons. It stands 22km above the surface of Mars, and is it so wide it takes up an incredible 300,000 square kilometers of land. In comparison, Mt. Everest is only 8.8km tall, and Olympus Mons is approximately the size of Italy. As seen in the picture above, Mars is home to many large volcanos that are all at least one hundred times larger than any volcano on Earth. The main reason for this is because Mars does not have mobile tectonic plates, meaning that these volcanoes have sat over hot spots filled with lava for hundreds of millions of years, and as a result have grown to enormous sizes. Scientists have determined that the last time Olympus Mons erupted was about 25 million years ago. While its last eruption happened while dinosaurs still roamed the Earth, scientists are still unsure of Olympus Mons is dormant or not, and thus it may still erupt again in the future.

It is interesting to think about the effects that the last eruption had on Mars, or even what the next eruption might do to those on Earth if it happened tomorrow. Could it have wiped out any life that may have been on Mars? Did it set off the nearby volcanoes in a catastrophic chain reaction? If it erupted tomorrow would any of the debris reach us? Olympus Mons may have played a role in eliminating life on Mars millions of years ago, and it is equally  interesting and terrifying to think about what sort of effect this massive volcano could have on Earth if it is, in fact, still active. (Source of Information: Wikipedia)


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Radioactivity and Practicality

Radiation-Symbol

Radioactivity has several negative associations: cancer, the atomic bomb, Chernobyl, etc. However, there are several practical uses for radioactivity across multiple disciplines.

  1. Agriculture:
    – Fertilizers are labeled with isotopes of nitrogen and phosphorous in order to figure out how much of the nutrients the plants take up and how much is lost to the environment
    – Before genetic engineering, gamma or neutron irradiation was used to alter a plant’s DNA as a way to introduce more genetic variability and new genetic lines of crops
  2. Pest Control: Some farms are using a sterile insect technique (SIT) to reduce the populations of pest insects in certain areas. Large numbers of insects are reared in a facility and before they are hatched, the eggs are irradiated with gamma rays in order to sterilize the insects. When these insects are released into the world and attempt to mate, no offspring are produced.
  3. Food Preservation: Some raw foods are exposed to high levels of gamma radiation in order to kill harmful organisms or bacteria – this keeps the food from spoiling for longer.
  4. Medicine:
    – Radioisotopes are used in combination with imaging devices to give medical professionals better insight into dynamic bodily processes, allowing for better diagnosis
    – Radio-immuno-assays are used in the laboratory to measure levels of hormones, enzymes, and drugs in a patient’s blood
  5. Industry:
    – Radioactive tracers can be used to detect leaks in machinery by examining the mix and flow rates of various materials
    – Instruments or gauges often contain radioactive sources that are used to detect certain levels of gases, liquids or solids by measuring the amount of radiation absorbed
    – The heat emitted by isotopes as they decay can be harnessed for industrial purposes (ex. The heat from the decay of plutonium-238 has powered several space vehicles)

As you can see from this list, not all radioactive decay is detrimental, and we will likely discover more applications for this technology in the future.


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Space: The Final Frontier…

Launched on January 19th, 2006 the New Horizons Space Probe was the first mission since Voyager to launch to an unexplored planet!

Designed, built and operated by the Johns Hopkins University Applied Physics Laboratory (APL), New Horizons also features instruments from: SwRI (Southwest Research Institute), NASA’s Goddard Space Flight Center, the University of Colorado, Stanford University and Ball Aerospace Corporation.

Labeled Instruments Antenna Ralph—telescope and color camera New Horizons at the Kennedy Space Center in 2005 LORRI—long-range camera VBSDC—Venetia Burney Student Dust Counter SWAP—Solar Wind At Pluto

(Images from: WordPress and Wikipedia)

New Horizons is comparable to the size of a piano. It is 27 inches tall,  83 inches long and measures 108 inches at its widest. It weighs about 1,054 pounds.

New Horizons made a brief swing by Jupiter in February 2007 to pick up some data and a bit of a gravity boost (Juno-the second New Frontiers mission- launched on August 5, 2011, is focused on finding more in-depth data about Jupiter) before continuing with its “required” objectives in the Pluto System.

On July 14, 2015, New Horizons made its closest approach to Pluto (7,750 miles away from the surface). It’s primary objectives were to:

  • Characterize the global geology and morphology of Pluto and Charon
  • Map chemical compositions of Pluto and Charon surfaces
  • Characterize the neutral (non-ionized) atmosphere of Pluto and its escape rate

and while we’ve gotten a lot of data, New Horizons could take as long as 16 months to get all of the data back to us (it can only transmit 1 to 2 kb/s)-that means we won’t have it all until November of this year! And then of course there is the time it takes for analysis.

But never fear, in the mean time, New Horizons is continuing onward ( at 9.02 miles/s)  in the direction of the Sagittarius constellation. The hope is that New Horizons will be able to get observations of a Kuiper Belt Object- PT1 (2014 MU-69) in January 2019.

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New Horizons’ Trajectory (Wikipedia)

More Info:

See Where New Horizons Currently Is

More About New Horizons (from NASA)

NASA Fact Sheet about NH

NASA Press Kit on NH

New Horizons (Wikipedia)

New Frontiers (Wikipedia)


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