In September of last year, the Hubble Space telescope observed what is believed to be plumes of water erupting from the surface of Jupiter’s moon, Europa. The surface of Europa is covered in a layer of ice of unknown thickness, and it is widely believed that there could be vast oceans of liquid water underneath that ice layer. These plumes support this theory, and more importantly, support the possibility of heat convection through these oceans.
That heat convection would create a very active 3-Dimensional current system in the moon’s oceans. That 3-D current could be the key to Europe supporting an ecosystem, and our first example of alien life. The possibility of alien life is, of course, exciting to many around the world, and as of 2016 there are preliminary plans to land on the surface of Europa. The opportunity to land on and study the moon provides an incredible opportunity to see the first ecosystem observed off of our own planet, but also poses unique challenges. If there is an ecosystem on Europa great care must be taken to ensure it is not disturbed by any organisms that could possible get there from Earth. (Certain organisms may be able to survive in the vacuum of space, like the tardigrade, or water-bear)
Saturn lays outside of the asteroid belt among the giant planets. With a total of 53 moons (or 62 pending a few new discoveries), Saturn is a planet that yields a huge amount of force in the Solar System. The moons orbiting Saturn are all unique and have distinct features. Titan, Saturn’s largest moon, has an atmosphere similar to that of Earth’s before the beginning of life. Among the rings, Prometheus and Pandora serve as shepherds for the material making up the rings, helping Saturn maintain its distinctive rings. Mimas is another well recognized moon, as it has such a large crater, evidence of an impact that nearly split the moon in half! There is no standard orbit for Saturn’s moons, increasing the interest astronomers have in Saturn and its moons.
Global warming is incredibly real, and an incredibly big problem. According to NASA, 9 of the 10 warmest years on record have occurred in the last 17 years, as well as the amount of arctic ice shrinking to the lowest it has ever been recorded in 2012. Our habits as a population are ever increasingly changing our world around us, with some dire consequences. A shrinking ozone layer, melting ice caps, and rising temperatures and water levels are well known and undeniable results of climate change, but a lesser discussed outcome is coral bleaching.
Coral that are stressed by a change in conditions expel algae that causes them to turn white, a process that is called coral bleaching. Coral and algae have a symbiotic relationship, meaning that they depend on each other and work together to survive. The algae gives coral its bright and vibrant colors while the coral provides the algae with shelter; each provides nutrients to the other. If the bleaching is not detrimental, coral have been shown to recover and return to its colorful and healthy state. However, if left for an extended period of time without its algae counterpart, the coral will die. Preventing coral death as much as possible is incredibly important; nearly 25% of marine life lives, interacts with, or relies on coral in some way on a daily basis.
I can personally attest that coral bleaching is a real thing affecting ecosystems across the globe. I had the opportunity to travel to Australia this summer and go snorkeling on the Great Barrier Reef. Our guides showed us pictures of the reefs we would be seeing, and in person many of the sections had turned white and had died. While still beautiful, it was very apparent that the coral was struggling to survive in its warming environment. Climate change is causing disruptions in aquatic ecosystems that will have long lasting and far reaching consequences.
We often misuse words such as meteor, meteorite, and asteroid while talking about space and not realizing that these three things are actually different! In this post I will explain the difference between all of them.
What are meteors? Meteors are objects that enter the Earth’s atmosphere from space. Sometimes they are called “shooting stars”, because they vaporize and leave the fiery trails. Meteors never reach the Earth’s surface because they burn completely in its atmosphere.
Meteorites also are objects that enter the Earth’s atmosphere, but they actually “survive” and hit its surface. The majority of meteorites are pieces of asteroids.
Asteroids are rocky bodies that are mostly found in the asteroid belt (between Mars and Jupiter). Due to a very strong Jupiter’s gravity, smaller asteroids might be pulled out of the belt, and then travel towards the inner Solar System where they can collapse with the Earth.
To sum up: asteroids are the biggest objects out of these three. They “live” very far from the Earth, and have to travel a very long distance to reach us. Meteorites are pieces of asteroids that actually go through the Earth’s atmosphere and hit the surface, while meteors are just bodies that enter our atmosphere but burn there.
For about 4 billion years, Earth has rather peacefully orbited the Sun along with its seven fellow planets. While this may feel how it has always been, this was not the case. The creation of our planet and Solar System involved intense, powerful forces at work. The video clip from Stephen Hawking’s Into the Universe series, “Formation of the Solar System,” shows how it might have looked.
Ironically, the birth of our Solar System might have begun with the deaths of many stars. At the onset of the Big Bang, hydrogen and helium were released in a vast cloud of gas and dust called a nebula. These nebulae created stars, which contained heavier elements and scattered their materials into new clouds when they died. Our Solar System began with a solar nebula from a star’s supernova. This solar nebula contained nitrogen, oxygen, iron, silicon, and many other elements, which we now see on Earth and throughout the Solar System. Then, the cloud collapsed into itself due to gravity.
During the collapse, the solar nebula’s temperature increased as gas particles crashed into each other and produced thermal energy. While gravity pulled the cloud’s material inward from all directions, the nebula rotated at an accelerated pace, keeping the material from being all drawn to the center at once. The particle collision and rotation caused the cloud to flatten. The spinning, heated particles of rocks, metals, and minerals collided and clumped together into huge, rotating masses which would soon become planets. Although the video does not explain the process, it shows how the solar nebula’s heating, spinning, and flattening created Earth.
In the center of the nebula, the temperatures became so great that the atoms began to fuse into the Sun. When it was created, the Sun released a huge solar wind which blew the remaining gas particles into the outer edges of the Solar System. These gas particles would get trapped by gravitational pulls of the planets Jupiter, Saturn, Uranus, and Neptune, which are now known as gas giants. Meanwhile, the rocky terrestrial planets of Mercury, Venus, Earth, and Mars lie near the center orbiting the Sun. Thus, our Solar System came into being.
Source: The video shows a simulated formation of the Solar System as seen in Stephen Hawking’s Into the Universe series, clips of which can be seen in this playlist.
The Cosmic Perspective: The Solar System- Jeffery Bennett, Megan Donahue, Nicholas Schneider, Mark Voit
“Out to sea, the calm lagoon waters were darkening, while the comets overhead glowed brighter, omens in the gloaming.” ― Julian May, Perseus Spur
A comet is an icy small body in the solar system that when passing close to the Sun, it produces a visible atmosphere or coma from a process called outgassing — Wikipedia. I always hope to see the comet steaming away into the space and passing the night sky with a beautiful tail. Although most people may not get the chance to witness their beauty themselves, some pictures and scientific facts about famous comets will help us understand more about those mysterious objects traveling in the solar system.
HALLEY’S COMET
Halley’s Comet is probably the most famous comet in history. It was named after the astronomer Edmund Halley who found out its 76-year orbit. “Halley is the only known short-period comet that is regularly visible to the naked eye from Earth, and the only naked-eye comet that might appear twice in a human lifetime.” — Wikipedia. Comet Halley will return to the inner Solar System in the year 2061.
Hale–Bopp was discovered on July 23, 1995 prior to it becoming naked-eye visible on Earth. One if its outstanding traits is its intense brightness, which is due to the exceptionally large size. Comet Hale-Bopp was estimated to have a nuclei about 40 km across, which is way larger than most comets. And Comet Hale-Bopp holds the record for a 19 months period of naked-eye visibility, which is amazing!
Comet Hyakutake was first discovered by an amateur astronomer called Yuji Hyakutake from southern Japan on January 30, 1996 using a pair of binoculars. Then in the spring of that year, this small bright comet with a nucleus of 1.6 to 3,2 km made a close flyby of Earth — sporting one of the longest tails ever observed. — Wikipedia.
Everyone got some basic knowledge about planets, stars, and asteroids at school, but not many people actually know much about comets. How are these things formed? Why do they have tails? How big are they? Stay with me if you want to find out.
Our entire Solar System was created by the collapse of a giant, diffuse cloud of gas and gas 4.6 billion years ago, and comets are simply some leftovers from the formation of the planets. Comets mainly contain dust, ice (the temperature in space is cold enough to produce ice), carbon dioxide, ammonia, methane, and are often called “dirty snowballs” by scientists.
In the outer Solar System comets remain frozen, and it is impossible to see them from the Earth due to their small size. “As a comet approaches the inner Solar System, solar radiation causes the volatile materials within the comet to vaporize and stream out of the nucleus, carrying dust away with them. The streams of dust and gas thus released form a huge, extremely tenuous atmosphere around the comet called the coma, and the force exerted on the coma by the Sun’s radiation pressure and solar wind cause an enormous tail to form, which points away from the Sun,” – Wikipedia.
The solid nucleus of comets is usually less than 50 km, but the coma may be larger than the SUN! Comet’s tail might extend up to 3.8 astronomical units (570 Gm). A comet can lose its tail only if magnetic reconnection occurs. This means that if at some point where the ion tail is sufficient, and the magnetic field lines are squeezed together, the tail “disconnects”.
So, to sum up… Comets are “dirty snowballs” made of dust, ice and some gases, their bodies might be tiny for cosmos, but their tails are suuuuper long! We do not see them too often, and they still remain a bit mysterious… In Russia we say that you need to make a wish when you see a comet in the sky!
In August of 2016, a team of astronomers discovered Proxima Centauri b, an exoplanet orbiting the red dwarf star Proxima Centauri. This finding was greatly exciting for several reasons. Not only is Proxima Centauri the closest star to our solar system besides the Sun at 4.2 light-years away, but its planet is in orbit within the star’s habitable zone, or the distance at which the planet could potentially support liquid water on its surface. The planet is only slightly more massive than Earth, indicating that it is likely a rocky planet like our own. However, Proxima Centauri b may have several hazards preventing it from being habitable by life as we know it. Below is an infographic about some of Proxima b’s characteristics:
Because the planet is in orbit around a small red dwarf, it is quite close to its star, orbiting in only about 11.2 days. Because of this, it may be tidally locked, meaning that one side would always face the star, creating harsh conditions everywhere except perhaps the border between the light and dark sides. It’s proximity to its star also leaves it prone to devastating solar flares and other radiation, making it unlikely that the star has a thick atmosphere or the potential for life. Nevertheless, knowing that planets quite similar to our own are this close should inspire us to continue searching for new and exciting worlds.
Discovered in 1930 by Clyde Tombaugh, Pluto was long regarded as the ninth planet of our solar system. However, after astronomers deepened their exploration of the intriguing worlds in the Kuiper belt, the icy Pluto was reclassified by IAU as a dwarf planet in 2006. Because additional objects in Kuiper belt has been discovered including Eris, which is 27% more massive than Pluto.
Then more accurate description of Pluto should be: the second largest known dwarf planet and tenth largest objects orbiting the Sun.
Pluto is only half as wide as the United States and its diameter is only about two-thirds as wide as Earth’s moon. Pluto is about 40 times farther from the sun than Earth is. Thus, it takes 248 Earth years to go around the sun and its surface is mostly covered with methane and nitrogen ice. Pluto is about 230 degrees below zero Celsius, much colder than Antarctica.
Pluto has five moons: Charon, Styx, Nix, Kerberos and Hydra, with Charon being the closet to Pluto and Hydra the most distant. Since Charon and Pluto are similar in size, Pluto and Charon orbit a point in space that lies between them and they continuously face each other as they travel through space.
With the successful flyby of the New Horizons mission launched by NASA in 2015, for the first time we get to know Pluto and its moons through clear pictures. And information about Pluto and its moons provide astronomers insights into the history of the solar system and how dwarf planets are formed.
In most the field of astronomy, the periodic table is far simpler than the one you had to learn about in school. There are only three elements: hydrogen, helium, and metals. This does not mean that all of the other elements you know aren’t real, but because there is so much hydrogen and helium in our universe, they completely dwarf all of these other elements on large scales. In our entire solar system, the Sun comprises 99.86% of its total mass, and of that mass, about 98% of it is hydrogen and helium. Jupiter and Saturn alone make up 90% of what is left, and they too are made up of mostly hydrogen and helium. Virtually all of the other elements that make up basically everything you know are present in only trace amounts. The image below shows the relative abundances of all of the elements, and as you can see, most elements are too comparatively rare to even appear on the diagram.