‘Oumuamua: An Interstellar Visitor

An artist’s rendition of what ‘Oumuamua might have looked like (The Guardian)

In 2017, a small, long object between 100 and 1,000 meters in length and between 35 and 167 meters in height and width passed through the inner solar system with a trajectory and speed only possible if it originated from beyond our solar system. This object, now known as ‘Oumuamua, is one of the first discovered to have an interstellar origin, and exhibited many unusual characteristics we have yet to explain.

‘Oumuamua passed inside of Mercury’s orbit, then traveled within 0.17 astronomical units of Earth (1 AU is the distance from Earth to the Sun) before taking a trajectory leading it outside of the solar system. When traveling away from the Sun, ‘Oumuamua’s speed increased by an amount typically indicative of comet outgassing. However, no such outgassing was observed. ‘Oumuamua also exhibited an atypical tumbling motion for objects with a high length-to-width ratio. These unusual characteristics, along with its abnormal elongated shape, have led some to theorize that the object was constructed by aliens, however most experts deem this to be very unlikely. Regardless, ‘Oumuamua is a fascinating object both in its characteristics and its extrasolar origin, and is perhaps among the first of many interstellar objects to be discovered.

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Blog#6 Red Giant and White Dwarf

Pauli Exclusion Principle (Wikipedia): every electron is indistinguishable from another. Two identical electrons cannot locate in the same volume of space with the same exact properties (energy, spin, direction) Thus, the electron has to be excluded from this space or remain at the higher energy level. 

HR diagram

When a main-sequence star (Wikipedia) comes towards the end of its life, the pressure at its core is so high that all electron states are filled. Therefore, electrons become degenerate (Wikipedia) they are forced to have higher energy than they should have at their temperatures due to Pauli Exclusion Principle. Therefore, its He core collapses, and stars climb to the red giant branch until the core temperature reaches 10^8K, then He fusion begins in the core (helium will become carbon). This process occurs at the top of the red giant branch. Moreover, the star’s core volume will be bigger due to He fusion, so there will no longer be any electron degeneracy, all energy restored due to degeneracy will be released at one, causing Helium Flash (Wikipedia)

Helium Flash

Therefore, the star will drop to a horizontal branch and becomes a red supergiant. The carbon core will slowly collapse and the H&He burning shall overcome gravity. Dust forms in outer space, light energy pushes out dust, and dust pushes gas, the outer envelope will slowly be blown away, forming a Planetary nebula (Wikipedia).

Planetary Nebula

The collapsing carbon core henceforth becomes White Dwarf (Wikipedia). Whit dwarves have balance between gravity and degeneracy and are very dense. They cannot shrink anymore. They will cool off eventually. 

White Dwarf

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Enceladus: Alien Life in Our Own Solar System?

Enceladus, one of Saturn’s moons (NASA)

Enceladus is an icy moon of Saturn, and is fairly small (or medium-sized, for a moon) with a diameter of about 500 km. For reference, the Moon has a diameter of about 3,475 km. Despite its size, however, Enceladus has been rated as among the most probable sources of life in our own solar system outside of Earth. Scientists think this might be possible because Enceladus has a large subsurface ocean below a layer of ice which is about 35 km thick. Its ocean is estimated to be about 28 km thick, which is almost eight times the average depth of Earth’s ocean. Enceladus experiences internal heating due to tidal forces from Saturn and other moons, which causes large geysers on its icy surface, and makes oceanic volcanism possible at the bottom of its massive subsurface ocean. This last point is especially significant, as life on Earth is theorized to originate from similar oceanic volcanic environments.

What bolsters this point even more is that methane, carbon dioxide, and dihydrogen have been recorded in Enceladus’ geyser plumes, which is best explained by oceanic volcanism. These chemicals were also recorded in levels that current Earth-based models cannot explain unless one factors in the role of life in generating methane at the volcanoes. This does not indicate life on Enceladus, as there could be other explanations for the levels of methane and carbon dioxide in the geyser plumes, but it is significant nonetheless that life would be the best explanation for these chemical levels if they were observed on Earth. In summary, Enceladus has both an environment that would make extraterrestrial life possible and levels of certain chemicals that would be consistent with the presence of life on the moon. Thus, Enceladus is a very interesting moon that definitely warrants further scientific study.

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Blog#5 Pluto

Pluto, formerly considered one of the nine planets, has always been controversial. Nonetheless, since the International Astronomical Union redefined the meaning of planet (A planet is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and (c) has cleared the neighborhood around its orbit) (check IAU Website for further information)

Pluto now falls into the category of a dwarf planet because of its size and the fact that it inhabits a region of other similarly sized bodies known as the Trans-Neptunian region. A dwarf planet is a celestial body that -orbits the sun, has enough mass to assume a nearly round shape, has not cleared the neighborhood around its orbit and is not a moon.

Definition of Dwarf Planet and Examples Cr. NASA

NASA’s New Horizons mission is the first mission that conducted a Pluto flyby and provided humans with a high resolute picture of Pluto. 

Pluto has one important moon: Charon. Half the size of Pluto, Cajun is the largest moon of Pluto and the largest known moon relative to its parent body. Pluto and Charon are considered binary systems and experience tidal locking. NASA’s New Horizons mission discovered that the reddish north cap of Charon is atmospheric outgassing from Pluto. 

Charon Cr. NASA
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Magnetar — A Fascinating Neutron Star

Neutron stars are the collapsed core of the massive stars (our Sun cannot qualify that). Neutron star was the smallest and densest stellar object in the universe. A city-sized neutron star can obtain the mass of the Sun. There are two types of neutron stars — magnetars and pulsars. Pulsars are neutron stars with fast rotational rates, and magnetars — as the name states — are neutron stars with extremely large magnetic fields. Magnetar — my favorite object in the whole universe —  formed from a fascinating process. During the formation when the supernova explosion happened, the magnetic field increases due to the conservation of magnetic flux. Strong magnetic fields originated from magnetar originated from the magnetohydrodynamic dynamo process before neutron stars reached equilibrium configuration. Through the dynamo process, heat and rotational energy will convert into magnetic energy. Strong magnetic fields exist and persist because of the currents in a proton-superconductor phase of matter. Giant flares, the strong eruptions caused by magnetars, burst gamma rays and give enormous information & interesting phenomenon about this mysterious star.

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Blog Post 5: Comets and their Tails

Halley’s Comet, one of the most famous comets that routinely comes back to the terrestrial worlds and can be seen. Credit to Wikipedia.

Comets are large balls of dust, rock, and ice that travel across our solar system and other solar systems. They are large like asteroids, around 10 km in diameter in our solar system. The largest one in our Solar System is Bernardinelli-Bernstein, a massive body about 85 miles in diameter. These objects can approach near Earth and can be seen in the night sky on regular intervals, due to their orbits being predictable and tracked by scientists.

The comet is made of three main parts; the nucleus, the comma, and the tails. The nucleus is the center of the comet, or the actual rock itself. It is made of dust and ice, which remains stagnant and stable in the outer solar system. However, once the comet approaches the center, the ice begins to sublimate away. This area is known as the comma. This atmospheric layer only appears when the object is getting close to the sun, making the object glow bright.

The tails extend thousands of miles behind. There are two tails, a plasma tail and a dust tail. One of them is made of plasma, which is blasted away from the sun by solar wind. The dust tail is made of physical objects, which is blasted away by the sun’s radiation pressure. Both of these tails always face away from the sun, even when moving away from the sun. The tails get larger closer to the sun, since these forces are much greater when closer.

The orbit of a comet, where the tail gets larger as it gets closer to the sun. Credit to the European Space Agency.

One of the reasons why comets are so interesting is because they come from such far distances, yet we can still observe them due to their orbits occasionally coming close to the terrestrial planets. It takes millions of dollars to get photos from an object far away such as the Kuiper Belt. Comets are opportunities for such objects to come to us instead. The comet mentioned before, Bernardinelli-Bernstein, may originate from the Oort Cloud, and will be within Saturn’s orbit by 2032. Even better, some comets come so close that we can see them as pronounced objects in the night sky. Halley’s comet comes every 75 years, and is predicted to come again around 2061.

Remember, comets, just like Tails the fox, have two tails. Credit to Wikipedia.
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Asteroid Mining

Picture of Asteroid

With the current rise of privatized space travel, one industry that may very well likely be popularized within our lifetimes is asteroid mining. However the initial investment cost of getting to a profitable asteroid will be enormous, the payoff of mining and bringing back the metals that these asteroids contain would be more than worth it. We are currently aware of 5 different asteroids that are worth multiple quintillion dollars at the current market rate of the metals that are contained.

However, to play devils advocate, the pure profit from these asteroids would likely be much lower if they were actually brought back to Earth, thanks to the laws of supply and demand. The price for the metals contained in these asteroids would plummet do to the massively increased supply.

Still, that does not mean it would not be fiscally worth it to go after these asteroids. It may be probable that industry would increase with the lowered price of these metals, allowing humanity to advance without resource limitation.

Source : Asteroid Mining

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Possibility of Life on Europa

Picture from European Space Agency

As of now scientists believe there are three requirements for a planet to develop and sustain life. Liquid water, the appropriate chemical elements, and an energy source. Europa has more than enough water, as it is believed that below the roughly 15 miles of solid ice, lies twice as much water as in Earth’s ocean, even though Europa is a fraction of Earth’s size.

As of now the most likely way to get more information about possible life at Europa is to sample water from water vapor fumes shooting through the ice. We would have to send a spacecraft to Europa with capabilities of finding and sampling these fumes.

Europa is currently the best chance of finding life outside of Earth, and it is important to explore this possibility as it would significantly alter how we view the development of life in the universe. If life has developed on two separate bodies in the solar system, life may no longer be viewed as a freak of nature, but as a result of the right combination and not wholly uncommon features in nature.

Source – Europa : Ocean Moon

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Chicxulub Impactor Found?

A diagram of the Chicxulub impact and how ejecta could have reached the Upper Midwest, where the impactor samples were found.

In class, we discussed the Chicxulub impact, which is highly likely to have triggered the extinction event that killed the dinosaurs. Despite the large size of the impactor, the catastrophic impact and 65 million years of geological processes have hidden the exact nature of the impactor from scientists. While iridium deposits in sedimentary rock layers point towards a more metallic asteroid, there isn’t direct evidence of the composition of the impactor and if it was an asteroid or a comet. Recently, paleontologists discovered what they believe to be shards of the Chicxulub impactor preserved in amber from the moments after the impact. Some fragments in the sample are characteristic of Earth’s crust, but others contain more iron, chromium, and nickel. These elements are signs that these may be tiny pieces of the impactor, and point towards an asteroid as the culprit. While these results have not been thoroughly reviewed yet, this would bring us a step closer to understanding both the Chicxulub impact itself as well as the types of impacts and impactors we see on Earth.

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The Future of Exoplanet Analysis

Researchers were able to accurately map oceans, land, and vegetation from a pixelated image of Earth. This technology could be applied to exoplanets in the near future.

The search for extrasolar planets and alien life is a fascinating research focus that sits at the intersection of astronomy, physics, planetary science, and biology. As we have discussed in class, discovering exoplanets is a very difficult task, but we have discovered roughly 5,000 exoplanets to date and are making significant progress in that area. We currently analyze these planets at a surface level and try to make conclusions about their habitability based on their size, mass, the star they orbit, and the distance of that orbit. A potential next step would be to gather visual data about these planets, and a recent study suggests that we could detect the existence of surface features such as land and oceans with only a few pixels of information. Using new machine learning techniques, the researchers were able to correctly map out land and oceans on a blurry image of Earth. Future telescopes, like the next round of planned ground-based telescopes, could be able to produce images of exoplanets, so analysis technology like this could be used soon. 

As I mentioned in class, it seems to me that our rate of discovery of potentially habitable worlds in and outside of our solar system is accelerating significantly. I think it is more likely than not that we discover evidence of alien life within my lifetime— do you agree or disagree?

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