Comets: A Bunch of “Dirty Snowballs”

It is only right to dedicate a blog post to the very things that inspired my username: comets! Comets are small objects that orbit the Sun and tend to have more eccentric orbits than other bodies in the solar system. A comet consists of a nucleus, coma, ion tail, and dust tail. The nucleus is solid and mostly composed of volatile ices, silicate, and organic dust particles. The coma is the bright and flowing atmosphere surrounding the nucleus that is caused when the comet gets near the Sun and its ices sublimate. The ion tail is typically blue due to the CO+ ions in it. It is created when solar wind sweeps away ionized volatile gases found in the coma; the volatile gases are ionized by ultraviolet photons coming from the Sun. The dust tail is made up of dust particles that are pushed backwards by solar radiation pressure, producing a tail that tends to be long, curved, and either yellow or white.

Additionally, comets are usually named after the people who discovered them. Sometimes, they are named after the individuals who first noticed that they had periodic orbits. A “C” before a comet’s name indicates that it has a long period while a “P” before a comet’s name indicates that it is periodic. A “D” before a comet’s name means that it is deceased or destroyed. These are just a few examples of the great detail that goes into naming a comet.

Photo of Comet West in 1976 (taken from Britannica)

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A home for future humans?

Kepler 62e and 62f compared with the Earth. UW astronomer Eric Agol discovered 62f.

Size Comparison of Kepler 62e and 62f with Earth

With the rate at which we are destroying our planet, we are likely to need a new Earth sometime in the future. Luckily for us, there are two potentially habitable planets that were discovered in the Kepler 62 System, called Kepler 62e and Kepler 62f. These planets are 60 and 40 percent larger than Earth respectively, but both are in the habitable zone of the planetary system. In this “Goldilock’s zone”, temperatures are moderate enough to support liquid water, and thus could sustain life as we know it. These planets orbit a star slightly smaller than our Sun, at the equivalent distance of Mercury and Venus in our Solar System. The only problem is that this system is 1,200 light years away. Not only does it make traveling to these planets impossible, this distance makes it extremely difficult to measure the compositions of the planets. However, Lisa Kaltenegger of Harvard-Smithsonian Center for Astrophysics and the Max Planck Institute for Astronomy modeled the conditions of these planets, and found the worlds to be humid, cloudy, and have liquid oceans. Life on these planets could potentially be aquatic, although these are educated guesses and may only be confirmed by our descendants.

The telescope that discovered these planets was the Kepler space telescope. During Kepler’s almost decade long stint in space, over 2500 planets were discovered with 678 GB of data collected. Kepler 62e and 62f represent only two of these planets and a fraction of the data collected. It will be interesting to see how our discovery of exoplanets increases as technology improves.

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The Possibility of Life on Europa

Europa, taken during NASA’s Galileo Mission

Life as we know it needs three major ingredients, at least according to NASA. Life needs water, the correct chemical makeup, and an energy source. Europa, one of Jupiter’s moons, could have all three ingredients and is a candidate for sustaining life elsewhere in the Solar System. In terms of water, Europa has oceans that may be greater in volume than Earth’s oceans. Evidence for water on Europa comes from Galileo’s flyby missions, which detected a magnetic field that could have been generated by an ocean of salty water. Europa also experiences tidal flexing, which can generate enough heat to form an ocean. In terms of chemistry, life as we know it needs the following elements: carbon, hydrogen, nitrogen, oxygen, phosphorus and sulfur. These are common elements, which may have been already on Europa since its initial formation and can arrive in the form of impacts. Lastly, in terms of energy, Europa is too far from the Sun to have life based on photosynthesis. Instead, possible life on Europa needs to rely chemical reactions. Europa gets radiation from Jupiter, which splits the oxygen and hydrogen molecules in water. Oxygen is reactive, and if it falls into the global ocean, it can be used as a chemical energy source. Thus, according to the astrobiologists at NASA, the possibility of life on Europa is realistic.

This is not to mention that these three major requirements are only for life as WE know it. It is entirely possible that in the future, we come across something that does not meet our expectations for life and requires an entirely different habitat. I personally think that because of the sheer scale of the universe and different permutations for life, it is unrealistic to believe that all life forms are carbon based. Non-carbon-based life may not need any of the three major requirements listed above.

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TESS: The Modern Exoplanet Finder

Artist rendering of TESS (via Wikipedia)

The Kepler mission marked a significant jump in exoplanet discovery when the space telescope was launched over 10 years ago. Since then, astronomers worked hard to research, develop, and design a more modern approach to discovering these distant and unknown planets. The solution was the Transiting Exoplanet Survey Satellite (TESS). TESS’s mission was to look at the stars close to Earth that shined the brightest to find the exoplanets that orbit them. When compared to the Kepler telescope, TESS is able to perform the transit method on a significantly larger area of space than Kepler. In sum, TESS’s advanced technology including multiple modern wide-angle cameras enabled 400 times greater area of surveillance for transiting.

The surveillance covers around Earth’s entire surface facing outward, resulting in 26 different sectors of space to cover. In the two year cycle, each hemisphere of the globe is covered in one year beginning in the southern hemisphere and then moving to the northern hemisphere. TESS completed the southern hemisphere in 2019, and began the second year of the process. In fact, TESS was so successful that the mission was extended in the summer of 2020 once it completed the northern hemisphere’s mapping. The extension adds new targets for TESS to focus on filling in small gaps the first two-year cycle missed, and includes new coverage of areas around the ecliptic. After three years in the sky, TESS has amassed a collection of 2200 exoplanets discovered and will continue to add to its collection over the next year and a half. The gif below shows TESS’ orbital patterns over its lifetime.

Animation of TESS from April 18, 2018 to December 18, 2019 (via Wikipedia)
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Florida Asteroid Burning Up

On Monday April 13th, a small asteroid was spotted in the night sky off the east coast of Florida. One of my family members was all the way across the state on the western side of Florida and saw the asteroid’s fireball-like appearance as it passed by Earth over 26,000 km away. According to the Space.com, the meteor was 4 meters in diameter will continue to move through space around the sun, returning to Earth in about 2 years. The tool the National Weather Service (NWS) uses to track these occurrences is called the Geostationary Lighting Mapper that captures images of the Earth at night and finds anomalies in light coming from Earth’s surface. When the April 13th asteroid burned up, the tool took the image shown below with the asteroid being inside the red circle.

Although it would be difficult to tell the shape of the asteroid, we know that the majority of asteroids are potato-shaped since their gravity is not strong enough to shape them into spheres. They are primarily made of rock and metal as during the formation of the Solar System, they formed inside of the frost line. As this collection of rock and metal passes through Earth’s atmosphere, the asteroid begins to burn up as gasses in the atmosphere hit the front side of the rock. Then, the heat from these continual impacts causes the asteroid to heat up so dramatically that it glows in the night sky. Asteroids burning up occurs throughout the day and night, but we can only see them during the night since the sun is so bright it blinds us from the glow of an asteroid.

Here’s a link to a cool video of the event!!

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solar system superlatives: Saturn

Welcome back to solar system superlatives! Last time, we learned about Mars and the breathtaking enormity of Olympus Mons, the largest mountain in our solar system. Now, let’s take a look at my personal favorite of the giants: Saturn.

Saturn’s rings during an eclipse

Needless to say, Saturn wins the prize of “coolest rings in the solar system.” Just take a look at some of these pictures and, if you didn’t appreciate them already, hopefully you can see how beautiful they truly are. It’s hard not to be mesmerized…I just spent like 20 minutes scrolling through NASA’s gallery trying to pick some of my favorites.

Mimas and Saturn
a shadow cast by Saturn’s rings

Too bad its almost 1.5 billion kilometers away.

But let’s take a closer look to really see just how spectacular these rings are. As you can see in the picture displaying a shadow cast by Saturn’s rings, the rings are incredibly thin, so thin they almost seem to disappear when viewed head-on. As it turns out, Saturn’s rings range from about 10 meters in thickness to about 1 kilometer. Although these numbers may sound big, I assure you that they are not. In fact, let me show you why.

Saturn rings
highest resolution image of Saturn’s rings to date

Saturn’s main ring system spans about 300,000 kilometers. Therefore, if we take a width to thickness ratio, we get 0.000033. And, yes, there are five zeros. For comparison, the width to thickness ratio of a standard 28 centimeter (11 in) piece of paper is about 0.00036 (assuming a height of 0.1 mm). And, yes, there are only three zeros there. In other words, Saturn’s rings are essentially 100 times thinner than a piece of paper. A piece of paper. Also, if that’s not enough, the thickness to width ratio for Saturn was calculated by using 1 kilometer as the estimated thickness. If we drop that to the 10 meters found at the thinnest points, the ratio drops by another factor of 100.

Congratulations, Saturn. You really outdid yourself with this one.

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Going Up?

Image Source: MIT Technology Review

Space. Elevators. I know what you’re thinking- huh? What even are those? Those were my exact thoughts before I learned all about the concept of space elevators 10 minutes ago, and I’m going to share everything I learned with you. Rockets have been our only mode of transportation to space for quite a while, but space elevators could be the next big thing within the next century. In a space elevator, a tether is attached to both the Earth’s surface (in an equatorial region) and an object in space (most likely a geostationary satellite in Earth’s orbit), which allows for relatively simple (and cheap, compared to rockets) planet-to-space transportation. Motorized vehicles/pods could then travel freely along the tether without the help of rockets! Although this idea was first proposed in 1895 by Konstantin Tsiolkovsky, it has really only been considered feasible until recently. In fact, a Japanese company and the Chinese government are seeking to build one by 2050 and 2045, respectively. Additionally, trials are already being run to test this idea. This is a truly revolutionary concept that could potentially open up space travel to the masses, and I’m incredibly invested in its development! To wrap things up, what kind of space elevator music do you think would be playing as you go up? I personally wouldn’t mind some Jimi Hendrix or the 2001: A Space Odyssey theme song. Also, what are your thoughts on this idea? Audacious or ingenious?

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Calling All Nerds! (Just Kidding, LOTR is Cool)

Fomalhaut System (Source)

This image may look familiar to all you high fantasy fans out there as the Eye of Sauron from Lord of the Rings, but what if I told you that you didn’t have to travel to Middle-earth to see it? I know you’re all on the edge of your seats now! This is an image of the Fomalhaut System, which is located only a mere 25 lightyears away! I understand that might seem a bit far, but you can get back to me when you find out a way to get to Middle-earth that’s easier than traveling 25 lightyears (believe me, I’m open to suggestions). The above photo is actually an infrared image taken using a coronagraph (an instrument that blocks out light emitted by the star’s surface), but you might still be wondering what that brilliant ring is. That ring would be debris still left in Fomalhaut’s protoplanetary disk, where planet formation is occurring. Analysis of the debris ring has led astronomers to point to the existence of two exoplanets (or large accumulations of rubble), Dagon (already proven) and a hypothetical “Fomalhaut c.” These exoplanets shepherd the debris in a way that makes the clearly-defined edges of the ring, thus creating the distinctive Eye of Sauron shape. I’m really hoping we’ll get to learn more about this system in the near future, especially news regarding the elusive “Fomalhaut c”! Although my nerdy franchise of choice will always be Star Wars, that doesn’t stop me from appreciating a good fictional reference (especially when it’s naturally occurring). Do you know of any celestial objects that resemble iconic things of fiction?

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Makemake

Makemake was discovered in 2005 by Michael Brown, Chad Trujillo and David Rabinowitz. Makemake might be the most interesting dwarf planet with its cool name and special facts. Makemake is the second biggest dwarf planet and once it was discovered it led to the demise of the title of planet for Pluto. Because of Makemake being 2/3 the size of Pluto it led to scientists reconsidering and deciding that Pluto was actually a dwarf planet. Makemake was originally named Easter bunny, as it was discovered a few days before easter. Although Makemake might sound big being 2/3 the size of Pluto it is only 3 times as big as the Grand Canyon. Some other interesting facts about Makemake are: one year on earth is equivalent to 1/305 Makemake years, Makemake is the second brightest dwarf planet, its surface is dominated by methane which makes it extremely volatile and even though it isn’t too far away there are no plans to visit the planet soon!

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Kepler-452b

You are probably looking at the title of this post and wondering “what?” I would be too. What is Kepler-452b? Is it a theory? A concept? A principle? The correct answer is that it is a name. But a name for what? Kepler-452b is the name of an exoplanet (a planet outside our solar system). This particular exoplanet warrants a blog post because, of all the exoplanets discovered so far, this one is most similar to our Earth. Although this exoplanet is considerably more massive than Earth, its orbit lies within the habitable region of its star. We don’t quite know if Kepler-452b is a rocky terrestrial planet, but if it is, it would be highly geologically active with a ton of volcanoes. here are some facts about it!

Its orbit is 385 Earth days, so only about 20 days longer than our year.

Its equilibrium temperature is 265k, which is a little warmer than Earth’s.

It is about 5 times as massive as Earth

Its about 1,400 light years away, which may seem far to us, but in space that is pretty close to Earth.

Its star has nearly the same mass and is nearly the same size as ours!

Although Earth and Kepler-452b are not identical, they could still be considered a cousin, and they are more related than any other exoplanet. If we were to travel at the speed of the New Horizons spacecraft we just learned about, it would still take us 26 million years to get there :(. Isn’t that cool? Do you guys think we will ever be able to visit it?

Here is an image showing its orbit relative to its star and Earth’s orbit.

By NASA
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