Neptune is a fascinating system, continually forging the outer edges of our solar system. The gas giant’s orbit is littered with debris, dust and objects that travel through the Oort Cloud and into the Kuiper Belt and get caught in the gravity of the huge frozen gas giant. With a day lasting about 16 hours, … Read more
Accretion disks are one of the most fascinating and ubiquitous structures in astrophysics – swirling disks of gas, dust, and plasma that form around massive central objects like black holes, neutron stars, white dwarfs, or even baby stars.
The Properties and Characteristics of the Outer Solar System The Oort Cloud is generally considered to be at the edge of the solar system, where the gravitational influence of the Sun begins to lessen and form a vast, spherical shell of icy bodies. Neptune, the furthest planet, lies around 30 AU from the sun, about … Read more
I always like to learn about new concept and ideas, so this morning I woke up and just started to study frame dragging and relativistic effects on stars. I’ve been spending a lot of time with physics lately and have done a full Sagittarius A calculation, which turned out to be a fun way to … Read more
Presenting Elliot’s Hydrogen Fusion Simulator, V1.0.0 It is fairly well accepted that the future of energy will be nuclear. The concept of a Dyson Sphere was first developed by Olaf Stapledon in his science fiction novel Star Maker (1937). The idea was further developed by the physicist Freeman Dyson in his 1960 paper “Search for Artificial Stellar Sources of Infrared Radiation“. … Read more
Explore the nature of the solar wind through Parker’s research and NASA’s Parker Solar Probe data. Hypothesize the role of dark energy in coronal heating from 6K to 1,000K. Engage with mathematical insights and cutting-edge theories.