Space Physics and the Cassini Probe

Gravity is the magic super glue that keeps everything we know (and things we don’t know) together and functioning. Earth’s gravity keeps us on the ground, the moons gravity creates tides, and the sun’s gravity keeps us from flying away into oblivion. But why did Earth and the rest of the planets stay orbiting around the sun in the first place?

In order for an object to be captured in an orbit, it must face precisely the right conditions. Let’s talk in terms of an asteroid and a planet. If the asteroid passes too far away from the planet, the planet’s gravity will pull on the asteroid and change its path, but it will not capture the asteroid. If the asteroid passes too close to the planet, it will either make contact with the planet or experience something called a gravity assist. A gravity assist (recently seen in the movie The Martian) would pull the asteroid very close to the planet and slingshot it off at a speed much faster than its initial velocity. This method is frequently used in space missions to conserve fuel while increasing speed. A diagram below shows how a planetary/gravity assist was used to get the Cassini probe to Saturn.

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Planetary Assist

The Cassini probe was launched and used four different planetary assists to increase speed and alter its direction to reach Saturn. It passed by Venus twice, then Earth, and finally Jupiter over the course of three years. The probe did not reach a velocity high enough to escape Venus’s orbit until it passed by Earth, which gave it enough juice to break the cycle and head towards Jupiter. The fact that scientists and astronomers were able to figure out that the planets would be the exact positions they needed to be in for this to work over a decade in advance astounds me. What do you think is the coolest thing astronomers have accomplished?


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Rogue Planets

All of the planets that we know and love in our solar system follow a pretty regular life. They spin about an axis, revolve around the central Sun, and go about their business in the small, but vast, family of the solar system.

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We are most familiar with “planets” as being what is similar to our solar system. Bodies of rock or gas caught in the pull of a massive star, following an orbit dictated by the laws of gravity.

However, not all planets are like this. It is too easy to get caught in the bias that everything we see on Earth is representative of the universe; the truth is that the universe is a vast, mysterious, and strange place. In addition to the usual planets familiar to us, there exist billions of rogue planets, who live quite different lives to the celestial bodies near us. Instead of orbiting around a central star (or anything at all), they drift aimlessly in space, only the occasional one lucky enough to get caught by a star, becoming “adopted” in sense.

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An artist’s perception of a rogue planet

Rogue planets weren’t always rogue, however. Most rogue planets are believed to have been ordinary members of a solar system, until a cataclysmic event resulted in one or several planets being completely knocked out of orbit. Possibilities include a massive collision with the planet, a massive collision with the central star, or even just another large body passing close enough to completely throw off the gravitational balance that makes up the serene solar system.

As if being an orphaned planet wasn’t sad enough, the surface of the planet is most likely equally desolate and miserable as its abandonment. Without a star to provide it light energy, liquid water would freeze into ice quickly, and any hope of civilization on the surface would be gone forever. Interestingly, if a “blanket” of ice forms properly and thickly enough, it could theoretically insulate the ocean of water underneath, similarly to how a bed of snow can actually insulate the grass underneath. There’s not much hope for advanced life on such a planet, but scientists do believe there is a slim chance extremophiles could find a way to adapt to such an environment.


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The EM Spectrum

When most people think of the word “light” they are probably talking about visible light, but the electromagnetic spectrum is much bigger and more diverse than that. Visible light is actually a very small part of the electromagnetic spectrum. Lets break down the spectrum in terms of wavelength. Visible light has a wavelength of 390 to 700 nanometers. X-rays and gamma rays, on the other hand, have wavelengths from 1 nm to 1 pm (1×10^-12). AM radio waves have a wavelength of 200-600 meters. In other words the wavelength of AM radio waves is about 1 trillion times as long as the wavelength of visible light. Light waves can have very different wavelength, so they can also have very different energy. Waves with shorter wavelength have higher energy. This is why some light is so dangerous and some is not. Gamma rays and even x-rays can be lethal, while radio waves and visible light are around us all the time.

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Photo source: Wikipedia

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The EM Spectrum

When most people think of the word “light” they are probably talking about visible light, but the electromagnetic spectrum is much bigger and more diverse than that. Visible light is actually a very small part of the electromagnetic spectrum. Lets break down the spectrum in terms of wavelength. Visible light has a wavelength of 390 to 700 nanometers. X-rays and gamma rays, on the other hand, have wavelengths from 1 nm to 1 pm (1×10^-12). AM radio waves have a wavelength of 200-600 meters. In other words the wavelength of AM radio waves is about 1 trillion times as long as the wavelength of visible light. Light waves can have very different wavelength, so they can also have very different energy. Waves with shorter wavelength have higher energy. This is why some light is so dangerous and some is not. Gamma rays and even x-rays can be lethal, while radio waves and visible light are around us all the time.

330px-em_spectrum_properties_edit-svg

Photo source: Wikipedia


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Feb 27 Solar Eclipse

On February 27, 2017 there will be an annular solar eclipse visible in parts of the South America and Southern Africa. A solar eclipse happens when the moon gets between the earth and the sun. An annular solar eclipse is like a total solar eclipse but instead of blocking all the visible light from the Sun it blocks all of the light except a ring around the outside. But what causes a solar eclipse to be annular? The moon’s orbit is elliptical, so it is sometimes closer to the Earth and sometimes further. When the moon is at or near apogee (the point in its orbit that takes it farthest from Earth) it appears smaller to an observer on Earth. Therefore when the moon eclipses the sun at apogee it does not appear to cover the entire sun. Instead it only covers part. When it lines up correctly, the relatively distant and apparently smaller moon creates an annular eclipse on the sun. solar-eclipse-annular

Photo cred: timeanddate.com

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Feb 27 Solar Eclipse

On February 27, 2017 there will be an annular solar eclipse visible in parts of the South America and Southern Africa. A solar eclipse happens when the moon gets between the earth and the sun. An annular solar eclipse is like a total solar eclipse but instead of blocking all the visible light from the Sun it blocks all of the light except a ring around the outside. But what causes a solar eclipse to be annular? The moon’s orbit is elliptical, so it is sometimes closer to the Earth and sometimes further. When the moon is at or near apogee (the point in its orbit that takes it farthest from Earth) it appears smaller to an observer on Earth. Therefore when the moon eclipses the sun at apogee it does not appear to cover the entire sun. Instead it only covers part. When it lines up correctly, the relatively distant and apparently smaller moon creates an annular eclipse on the sun. solar-eclipse-annular

Photo cred: timeanddate.com


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Star Trails

Star trails are probably some of the most well-known and well-received type of astrophotography out there, as the beautiful circular patterns the stars make as Earth rotates are truly mesmerizing and sometimes even inspirational. I know I always find time to look up at night and appreciate the night sky and the stars and even wonder about life and my place in this world. Anyways, I digress. There are two main ways to create a star trail image, one is through a long exposure, where the camera shutter stays open for a long time and essentially records all light, and then there is the stacking of multiple shorter long-exposure images. I have tried both and I have to say, the latter definitely seems to work better.

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A stacked star trail (came out pretty well!)

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A single long exposure star trail (not as well)

First, I usually have my camera set to a lower ISO, such as 400, to reduce the noise, then I generally use as wide of an aperture as I can get paired with a wider angle lens to also capture some of the landscape. I use a Nikon 18 – 55mm kit lens, so I set it to f/3.5 and 18mm. Lastly, I set the focus to infinity (since the stars are so far away) and try several exposure times— usually eight to ten seconds work well. I use an intervalometer to continually capture images for a set period of time, anywhere from half an hour to 3+ hours.

Once I have all the raw images, I import them into a free software called StarStax, and choose the gap-filling mode. Then the magic happens and you get to see the stars moving as the images are stacked, leaving a circular trail behind them. This is a very primitive guide, but really, there isn’t very much effort required if you are already familiar with a camera and its settings. A more in depth guide can be found here if you want it though. Mostly, I wanted to share the program StarStaX because it is completely free! Meaning if you already own a decent camera and tripod, anyone can do this type of photography as long as they can see the night sky! Go try it out 🙂


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Planetary Defense System

Earth sees its own fair share of incoming projectiles from space, but it’s extremely rare to find an event that poses any real threat to Earth or its life.  Most of this safety comes from that fact that space is inconceivably large; the possibility of being hit by an asteroid that could do any real damage is astronomically low (yeah, pun intended).

In a 1994 paper, planetary scientist George Wetherill postulated that Jupiter’s immense size could be partially to thank for keeping large bodies from reaching the inner planets of the solar system and possibly colliding with Earth.  Recently, however, Kevin Grazier of NASA’s Jet Propulsion Laboratory ran simulations of the solar system and found strong evidence that we may have Saturn to thank as well for keeping us safe.

His tests showed that the most asteroids were deflected out of our system only when both Saturn and Jupiter were in the solar system.  A solar system with either Jupiter or Saturn in it would produce a much larger asteroid belt and would keep many of these smaller bodies in closer, more dangerous proximity to our home rather than being flung into space due to the larger, combined gravity of both giant planets.

 

Photo courtesy of NASA and seeker.com

Saturn Could Be Defending Earth From Massive Asteroid Impacts


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Rogue Radio Burst Leads to Discovery of Billion-Year-Old Galaxy

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©2008 John P Warren

The detection of fast radio bursts, one of the universe’s most mysterious and rare occurrences, took place in early January of this year when signals from a dwarf galaxy over 2.5 billion light years away were first recorded.

Fast radio bursts (FRBs) are an incredibly rare phenomenon usually occurring in a millisecond or so, each containing energy amounts equivalent to almost 500 million of our Suns. While such a signal has only ever been recorded 18 times prior, it is suspected that ten thousand of these bursts could be sent each day.

Scientists have speculated neutron stars to be the source of these bursts, while some point to origins within our own galaxy.

For more information on past occurrences, read here.


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Want to discover a new planet?

Are you curious about what’s out there in our universe? Have you been wanting to do your own astronomical research? Has it been a dream of yours to discover a new planet? Fear no more! A team of astronomers led by MIT and the Carnegie Institution for Science is now giving the public the opportunity to engage in research of exoplanets, or planets that orbit the Sun outside the solar system.

HD 209458 b (“Osiris”)

The team released datasoftware package, and a tutorial for the public to use. There is already data about which stars the team believes may have exoplanets. It is our job to help find those exoplanets. So what are you waiting for!


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