Planet Nine

 

Planet_Nine__black_background

Planet Nine Orbit

In January of 2016, some scientists suggested that our Solar System may yet again be comprised of nine planets, but how did they come to this conclusion? Well, scientists observed that way out in our outer solar system, some Kuiper Belt objects had unusual orbits that were similar to each other. This suggests that these objects are being affected by a massive object, which led scientists to suspect that there may be another planet out there in our solar system. Scientists (creatively) named this potential planet, Planet Nine.

Okay, so we may have another planet in our solar system, but how do we know it’s not another dwarf planet like Pluto? According to scientists, the fact that many Kuiper Belt object have similar orbits suggests there is a potentially massive planet that is ten times more massive than and four times as large as Earth. Scientists ruled out that the Kuiper Belt objects’ orbit could be affected by our solar system’s gas giant planets due to the fact that they too so far away, which means the answer behind these unusual orbits may be that there is a new planet that is massive enough to affect these Kuiper Belt objects.

So the planet, if it exists is most likely not a dwarf planet. What type of planet would it be? Although it is impossible to definitively state the composition and classification of this hypothetical planet, some scientists from Switzerland conducted a study in which they determined that Planet Nine would be a cold, ice giant planet smaller than Uranus or Neptune, but the planet would also still have some internal heat, which could still be escaping through the surface. Additionally, these scientists determined that the planet’s atmosphere is mostly comprised of hydrogen and helium.

Although nothing has been definitively determined yet, it will be fascinating to see if this planet exists and if it does, what it’s characteristics would be.

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Planet Nine

 

Planet_Nine__black_background

Planet Nine Orbit

In January of 2016, some scientists suggested that our Solar System may yet again be comprised of nine planets, but how did they come to this conclusion? Well, scientists observed that way out in our outer solar system, some Kuiper Belt objects had unusual orbits that were similar to each other. This suggests that these objects are being affected by a massive object, which led scientists to suspect that there may be another planet out there in our solar system. Scientists (creatively) named this potential planet, Planet Nine.

Okay, so we may have another planet in our solar system, but how do we know it’s not another dwarf planet like Pluto? According to scientists, the fact that many Kuiper Belt object have similar orbits suggests there is a potentially massive planet that is ten times more massive than and four times as large as Earth. Scientists ruled out that the Kuiper Belt objects’ orbit could be affected by our solar system’s gas giant planets due to the fact that they too so far away, which means the answer behind these unusual orbits may be that there is a new planet that is massive enough to affect these Kuiper Belt objects.

So the planet, if it exists is most likely not a dwarf planet. What type of planet would it be? Although it is impossible to definitively state the composition and classification of this hypothetical planet, some scientists from Switzerland conducted a study in which they determined that Planet Nine would be a cold, ice giant planet smaller than Uranus or Neptune, but the planet would also still have some internal heat, which could still be escaping through the surface. Additionally, these scientists determined that the planet’s atmosphere is mostly comprised of hydrogen and helium.

Although nothing has been definitively determined yet, it will be fascinating to see if this planet exists and if it does, what it’s characteristics would be.

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Naming Exoplanets: Explained

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Artist depiction of an exoplanet

So you’ve just discovered an exoplanet via the Astrometric method, the Doppler method, the Transit method, or some other scheme. You’ve probably already discovered the star it orbits around instead. You could name it something fun like Mr. Worldwide, but that doesn’t seem quite right. Surely there is a convention that most exoplanetologists use when naming newly discovered extrasolar planets.

Luckily, you’re in luck. The International Astronomical Union agreed upon a naming standard back in 2010. An exoplanet is named by simply appending a lowercase letter to the end of the name of the parent star. The first planet discovered in the star system is assigned the letter “b”, the next discovered planet is given “c”, and so on. In the case that several planets are discovered simultaneously, the closest planet to the star is given “b”, and the subsequent letters are assigned in order of orbital size.

example: the first planet in the star system 55 Cancri is called 55 Cancri b (The lowercase “a” after the star name is implied).

For a planet that orbits a star in a binary system, its name is the combination of the capital letter that designates the star, immediately followed by the lowercase letter as with before. The star designation is only necessary when more than one star is circled by its own planets.

example: Pitbull B is the second brightest star in a binary system. The first exoplanet discovered shall be named Pitbull Bb

Here is the naming standard from the International Astronomical Union:

In the WMC naming system, the brightest member of a star system receives the letter “A”. Distinct components not contained within “A” are labeled “B”, “C”, etc. Subcomponents are designated by one or more suffixes with the primary label, starting with lowercase letters for the second hierarchical level and then numbers for the third. For example, if there is a triple star system in which two stars orbit each other closely with a third star in a more distant orbit, the two closely orbiting stars would be named Aa and Ab, whereas the distant star would be named B. For historical reasons, this standard is not always followed: for example Alpha Centauri A, B and C are not labelled Alpha Centauri Aa, Ab and B.

If anyone can figure out what this means please let me know.

Source

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The Dragon Storm

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Source

In a world where the Sun is but a mere speck in the sky, where one day is 10 Earth hours, there exists a storm unlike any other. Jupiter’s Red Spot contains a storm that has lasted for centuries. Neptune’s Great Dark Spot is host to an anticyclonic storm. None can compare to the storm on Saturn known as The Dragon Storm.

Storms are not uncommon in the gas giants. Their turbulent atmospheres are prime for storms that last much longer than those here on Earth. Saturn’s atmosphere is no different; scientist refer to a region in the Southern Hemisphere as “storm alley” based on its high level of storm activity. This is where the Dragon Storm lies. As Cassini circled Saturn, it noticed a strong source of radio emissions between July and September of 2004. Scientists soon linked the radio emissions to the storm after months of observing their coincident behavior. These radio waves were of interest to NASA scientists because they resemble the bursts of static created by lighting on Earth. Ultimately, they deduced that the Dragon Storm is a giant lightning storm that can be explained using Earth weather.

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Dragon Storm in action

The Dragon Storm helped to characterize the behavior of weather on gas giants. Thunderstorms spawn regional storms which combine together to feed more powerful currents that sweep the face of the planet.

yay space

 

Source

 

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Dirty Snowballs

comet
The Hale-Bopp comet seen in Croatia in 1977

Comets are often referred to as “dirty snowballs“. That is because they are made up of a lot of many components that a dirty snowball would also consist of, and more! Many comets consist of dust, ice, carbon dioxide, ammonia, methane, and many more other components. When a comet gets close to the sun, some components of the go from being a solid state to a gas state. They leave a little trail behind them, which is the trail that we see when we see comet in the sky. Comets also consist of a comma, or the head of it which contains the rest of the components that are probably still in a solid state. If a comet gets too close to the sun though, it may crash, or just break up because all of its components evaporate.

Comets often get mixed up with asteroids, but asteroids do not contain a tail. Comets are thought to be leftovers from the formation of the universe, and can provide key clues to the history and formation of our universe. Asteroids are very much worth studying, and can provide us with a lot of key information if we take the time to take a look!

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Dirty Snowballs

comet
The Hale-Bopp comet seen in Croatia in 1977

Comets are often referred to as “dirty snowballs“. That is because they are made up of a lot of many components that a dirty snowball would also consist of, and more! Many comets consist of dust, ice, carbon dioxide, ammonia, methane, and many more other components. When a comet gets close to the sun, some components of the go from being a solid state to a gas state. They leave a little trail behind them, which is the trail that we see when we see comet in the sky. Comets also consist of a comma, or the head of it which contains the rest of the components that are probably still in a solid state. If a comet gets too close to the sun though, it may crash, or just break up because all of its components evaporate.

Comets often get mixed up with asteroids, but asteroids do not contain a tail. Comets are thought to be leftovers from the formation of the universe, and can provide key clues to the history and formation of our universe. Asteroids are very much worth studying, and can provide us with a lot of key information if we take the time to take a look!

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Are We Alone?

 

I’ll actually take the liberty of answering that. Of course not! How, in our exponentially infinite and ever expanding universe, could it have been us that just happened to luck out on the single life supporting planet? There is certainly other life out there, it’s just a matter of where and what type. Operating from our Earthly point of view and assuming all life in the universe operates as life on Earth does (which is a reasonable assumption, considering none of the other planetary climates in our solar system have been proven to sustain life) we must consider three necessary ingredients for life to be sustained on any planet.

First, a source of nutrients from which to build living cells. On Earth, this is nitrogen. Also necessary is a form of energy that can be harnessed to fuel said cells- on Earth, this energy takes the form of sunlight, chemical reactions, and even heat. Finally, liquid water is the last necessary ingredient for life on this Earth.

What personally gives me hope that not all life in the universe is Earth-like (and would therefore be more plentiful, given that the aforementioned requirements would not necessarily be satisfied) is the presence of bacteria on our own planet living in environments not conducive to life, as well as deep-sea creatures surviving under exorbitant amounts of pressure.57b7681edb5ce94b088b7e07-1334-1001

In our search for life in the universe, we are mainly focusing on the search for liquid water, as that seems to be the unifying factor to sustain life as we know it. This leads us to look towards planets in what is known as the “Goldilocks Zone”, which would be a Earth-like distance proportional to a planet’s Star (given it’s size).For example, if the star was larger and hotter, the special zone in which liquid water could exist on a planet would be further than our given distance of 1AU.
All of these ideas are summed up in the Drake equation (which I actually blogged about on my other blog) which takes into account all the aforementioned discussed factors for life and attempts to calculate the number of intelligent civilizations in the universe. With all these factors, combined with the billions of solar systems out there, one thing remains certain: we are not alone.

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Metal. Fire. Splash.

 

 

Beijing, we have a problem. At least that’s what I imagined Tiangong 1 broadcasted back to China as it re-entered Earth’s atmosphere and careened into the central South Pacific Ocean. Officials had no idea where exactly the station would re-enter and end up crashing, making the South Pacific a welcome relief for many. The initial estimated chances of a person on Earth being hit by the debris was less than one in a trillion due to the low percent of the space station which would survive re-entry.

The space station, first launched in 2011, lost contact with Earth in June of 2016 even though Chinese officials would not initially confirm this. The station’s main purpose was to serve as a manned laboratory and as an experiment for orbital rendezvous and docking capabilities. One of the station’s claims to fame was hosting a crewed mission which included China’s first female astronaut. Worry not though because Tiangong 2 replaced Tiangong 1 in 2016 and is currently orbiting Earth as China’s main research station.

China also currently has a planned launch for a permanent space station set for 2022 and another mission to land a rover on Mars to bring back samples for 2020. Experiments will continue to take place in outer space, furthering galactic research and the furthering of the human race.

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Pluto Reclassified as Planet

 

 

History was made on Sunday, April 1, 2018, as the International Astronomical Union (IAU) has decided to reclassify Pluto as a planet.

Pluto, discovered in 1930 as the ninth planet of the solar system, is a tiny world smaller than Earth’s moon. Pluto was stripped of its planetary status in 2006 and demoted to a dwarf planet. Unlike normal planets, dwarf planets have not cleared their neighboring region of other objects. Even though Pluto has multiple moons, it had failed to become gravitationally dominant in its vicinity in space. In order to be considered a full-sized planet, the object must have sufficient mass that its shape was formed by gravitational forces and must orbit the Sun in addition to clearing ‘its neighborhood’. Pluto had failed to differentiate itself from other Kuiper Belt objects in its near vicinity, which is why it was downgraded to a dwarf planet.

Over the past year, Pluto has been slowly shedding itself from the Kuiper Belt and as of Sunday, finally became gravitationally dominant in its spacial neighborhood. This recent development was discovered by Harvard astronomer David Fules. As is tradition with the discovery of new planets, the naming process is usually heavily influenced by the person who discovers the planet. As a result of his discovery and the time of the event, a large movement has gained traction to rename Pluto to “April Fules”.

🙂

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Many interesting exoplanets.

Even though we are mostly familiar with planets within our solar system, there have been many discoveries of exoplanets with the development of scientific technology and the improvement of our understanding of the Universe. Among these exoplanets, there are some interesting and habitable planets outside our solar system.

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source: NASA

First of all, “Kepler-186f” was found to be a rocky planet in the habitable zone, which is the region with right temperature for water from the star of the system. “Kepler-186f” has a very similar size as Earth and has a high chance of being a habitable planet. However, due to the lack of advanced technology, it’s hard to know what is going on at the surface and atmosphere of this planet.

Kepler16b
Source: NASA

Second interesting exoplanet is named as “Kepler-16b,” which is a circumbinary planet that oribits two different stars. Because it orbits two different stars, this planet would have a very different orbit from the orbits of planets in the solar system.

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Source: NASA

This “Kepler-444 system” is known to be the oldest solar system in our galaxy that existed since the creation of our galaxy.

There are many other exoplanets with its distinctive characteristics such as habitable environment, rocky surface etc. These exoplanets are important for us to study because they provide information that we can use to apply to our solar system. For example, the discovery of planetary systems within our galaxy helped us understand it is fairly common to have a solar system with many planets orbiting the star.

Source: NASA

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