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Tag Archives: blog4
Kepler Supernova
The image above is of Kepler’s Supernova, which Johannes Kepler is credited with discovering with his description of the stellar object in his De Stella Nova. As stars progress through their main sequence lifetime and beyond and use up more of their hydrogen in nuclear fusion, they can fuse heavier and heavier elements. More massive […] Continue reading
Legacy Survey of Space and Time: The future of astronomical observation is here…. almost!
Just two years from now, the Vera C. Rubin Observatory will commence operations, beginning its mission to image nearly 40 billion celestial objects over 10 years! These observations will be made with the world’s largest digital camera and an enormous 8.4 meter (in diameter) telescope, ensuring that its images will be of the highest quality. […] Continue reading
Posted in Instruments, Observables, Science, Stars
Tagged astro2110, blog4, technology
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The Martian: Scientifically Accurate?
The Martian is one of my favorite books, and the movie adaptation was fantastic as well (mild spoilers ahead). As someone who enjoys science and science fiction, I loved the realism and accurate technical problems that Mark Watney faces. The fundamentals of life on Mars—the time needed to travel there, delays and difficulties communicating withContinue reading “The Martian: Scientifically Accurate?” Continue reading
Time Dilation
As with most impressionable children growing up, the fascination of space and the many wonders it holds stems from watching certain movies or television shows that help portray these wonders. I was no exception to this as I was completely awestruck when I watched Christopher Nolan’s brilliant film, Interstellar. Despite containing a masterfully crafted story […] Continue reading
The Likelihood of Getting Hit with a Gamma-Ray Burst
A gamma ray burst is expected to hit Earth every 10,000 years to 1,000,000 years. How would this affect human society as we know it, why are gamma rays so dangerous, and can we do anything to stop it? Gamma ray bursts are extremely energetic spouts of energy, and similar to visible light, are part […] Continue reading
What was Theia?
Theia was about the size of Mars. It orbited with Earth. It crashed into the Earth and the debris helped create the moon. The core of Theia combined with the core of Earth. Scientists disagree on this and some believe that it formed into multiple moons. It is hypothesized to have orbited in the L4 […] Continue reading
Posted in Class, General, Historical
Tagged astro2110, blog4, Moon, Solar System, Uncategorized
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Blog #4: Coronal Mass Ejections
Coronal Mass Ejections are ejections of solar wind and plasma from our Sun’s corona. The blast from a Coronal Mass Ejection (CME), carries about a billion tons of material away from the sun at speeds ranging from 250 km/s to almost 3000 km/s. (NOAA) If they are directed toward Earth when they are ejected from […] Continue reading
Binary Star Collision
Binary stars were stars orbiting each other, and they might eventually collide due to the stellar mass loss or gravitational radiation which caused the decay of orbits. Stellar collisions could be amazing and rare, which happened once every 10000 years in our globular clusters. It was very likely, from scientists’ approximation, that a binary star […] Continue reading
Posted in Class
Tagged astro2110, binary stars, blog4, Observation
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Blog Post 4 Chicxulub Impact
The Chicxulub Impact happened approximately 66 million years ago, defining the end of the Cretaceous Period and the beginning of the Paleocene, as well as the end of the Mesozoic Era and the beginning of the Cenozoic Era. This impact not only managed to eradicate the dinosaurs as the dominant lifeform on the planet but […] Continue reading
Proxima: Our Cosmic Neighbor
The closest star to our solar system is one named Proxima Centauri. Proxima Centauri is a relatively small star, as it is a red dwarf star with about 12.5% the mass of the Sun and only about 0.17% as bright as the Sun. Proxima Centauri resides about 4.25 light years away from Earth, and is […] Continue reading