Star clusters provide insight into stellar evolution. Open clusters contain a few dozen to hundreds of younger, hot stars loosely spaced in a galaxy's disk. Globular clusters contain tens to hundreds of thousands of older, metal-poor stars in a spherical distribution in a galaxy's halo. Measuring a cluster's main-sequence turn-off point allows determining its age. Some globular clusters exhibit evidence of black holes at their centers from observations of white dwarf concentrations.
This document provides an overview of exoplanets, which are planets that orbit stars outside of our solar system. It discusses some of the key research that has been done to discover exoplanets, examples of notable exoplanets that have been found, and different types of exoplanets. The document also explores possibilities about whether life could exist on exoplanets and if humans will ever be able to travel to exoplanets. It presents the results of a survey conducted with 10th grade students about their interest in astrophysics and exoplanets.
1. The document discusses three main types of galaxies: irregular galaxies, spiral galaxies, and elliptical galaxies. 2. Irregular galaxies have no regular structure and contain regions of gas and young stars. 3. Spiral galaxies have a central bulge, disk with spiral arms, and halo, while elliptical galaxies are shaped like elongated spheres with smooth light and no axis of rotation.
There are several types of galaxies including spiral, elliptical, irregular, and barred galaxies. Spiral galaxies are the most common type and have tightly or loosely wound spiral arms. The Milky Way is a typical spiral galaxy located in the outer range of the galaxy. Other galaxy types include whirlpool galaxies like M51a, barred galaxies like NGC 1365, and elliptical galaxies which can be very large or small dwarf galaxies. Irregular galaxies have no distinct shape.
Black holes are regions of space where gravity is so strong that nothing, not even light, can escape. They form when massive stars over 8 times the sun's mass die in supernova explosions. Billions of black holes exist between galaxies and millions exist within our own Milky Way galaxy. Black holes can be detected by their gravitational effects on nearby stars and the intense light produced from material falling into supermassive black holes at galaxy cores. Orbiting black holes is possible only at precise speeds - too slow will lead to spiraling in, too fast will escape, and intermediate speeds result in complex rosetta orbits.
1) Black holes are formed when massive stars over 10 times the mass of the Sun collapse in on themselves due to nuclear fusion and strong gravitational forces. 2) We can detect the presence of black holes through the X-rays emitted when matter around the black hole is heated and through gravitational lensing effects on light passing by. 3) If you fell into a black hole, the extreme tidal forces would spaghettify and kill you before you reached the central singularity, and from your perspective you would see the universe compressed into a brief flash of light before destruction.
Mercury is the smallest planet in the solar system and orbits the Sun every 88 Earth days. It rotates slowly, with a day lasting almost 60 Earth days. Mercury has almost no atmosphere and its surface is heavily cratered due to meteor impacts. It is named after the Roman messenger god Mercury and is the closest planet to the Sun, with surface temperatures varying greatly between very hot and very cold.
A presentation I gave to the Brighton Astronomy Society in Jan 2016 - http://brightonastro.com/ , https://www.facebook.com/brightonastro/ Annoyingly that's removed the videos from the slides, so here are links to those: https://www.youtube.com/watch?v=e-P5IFTqB98&t=18s (This Youtube channel "In a nutshell" is absolutely fantastic by the way and I highly recommend a look through their other videos!) https://www.youtube.com/watch?v=duoHtJpo4GY https://vimeo.com/8723702 I've also made my notes from preparing the slides available here as well: https://docs.google.com/document/d/1gqgsAbvoCB_7-_gPToqOuSixc02YnU-ajf-uT60R1vc/edit?usp=sharing -- there are LOTS of further links to interesting videos in there as well, that I didn't use on the night so worth a scan through. Any further questions, feel free to ask in comments on here
The document provides information about astrophysics and the universe. It discusses the solar system including the sun and planets. It then discusses galaxies including spiral, elliptical, and irregular galaxies. It also covers constellations, nebulae such as the Eagle Nebula and Crab Nebula, and supernovas.
Observations from the Hubble Space Telescope in 1998 showed that the universe was expanding more slowly in the past than it is today, contrary to expectations. This led scientists to propose either modifications to Einstein's theory of gravity, such as the introduction of dark energy, or the existence of an unknown type of matter, dubbed dark matter, that cannot be detected directly. Dark matter is inferred to make up about 27% of the universe based on its gravitational effects, but its exact nature remains unknown.
The Milky Way Galaxy is a spiral galaxy that contains the solar system and Earth. It is estimated to be 100,000 light years in diameter and contains millions to billions of stars. The galaxy is composed of a disk, halo, and central bulge. Spiral arms in the disk contain dense clouds of gas and dust where new stars are forming. The sun orbits near the edge of the disk at a distance of about 8.2 kiloparsecs from the galactic center. All elements heavier than hydrogen and helium were produced through nuclear fusion in earlier generations of stars within the Milky Way over billions of years.
All stars begin as clouds of dust and gas called nebulae. When gravity causes the nebula to collapse, a protostar forms at the center. The protostar grows in size and temperature through nuclear fusion reactions until it becomes a stable main sequence star. Small stars like our Sun will eventually expand into red giants and shed their outer layers, leaving behind dense white dwarf cores. Larger stars may explode as supernovae, collapsing into neutron stars or black holes. The life cycle of a star depends on its initial mass, with smaller stars ending as white dwarfs and more massive stars ending as black holes or neutron stars.
The document discusses lunar and solar eclipses. It explains that lunar eclipses occur when the Earth passes between the Sun and Moon, casting its shadow on the Moon. Solar eclipses occur when the Moon passes between the Earth and Sun, casting its shadow on parts of Earth. For an eclipse to occur, the Sun, Moon and Earth must be aligned on the same plane. The document provides details on the conditions required to view lunar and solar eclipses and why the Moon appears red during a lunar eclipse.
Hey I'm DIVYA SHREE NANDINI. I'm here with my new presentation on Black Hole. I'm sure you'll find it interesting. well first thing what is black hole- "Black hole, cosmic body of extremely intense gravity from which nothing, not even light, can escape. A black hole can be formed by the death of a massive star. When such a star has exhausted the internal thermonuclear fuels in its core at the end of its life, the core becomes unstable and gravitationally collapses inward upon itself, and the star’s outer layers are blown away. The crushing weight of constituent matter falling in from all sides compresses the dying star to a point of zero volume and infinite density called the singularity." wanna know more about it then come with me. :)
Detail about Black holes. It's definition, components and then history of black hole and General theory of relativity. Life cycle of a star and formation of black hole in space. Different types of choice after star's life end. Different types of Black hole on basis on mass of Parent star. and classification of black holes on basis of charge and rotational motion of black holes. Quantum theory of physics. Study of Black holes using Quantum mechanics by Steaphen Hawking. Current research on black holes.
There are four main types of galaxies: spiral, elliptical, lenticular, and irregular. Spiral galaxies have a central bulge and rotating spiral arms containing young stars. Elliptical galaxies are spherical and contain mostly older, redder stars. Lenticular galaxies resemble ellipticals but have a disk of gas and dust. Irregular galaxies do not fit into the other categories and often have regions of intense star formation. The Milky Way is classified as a barred spiral galaxy while Andromeda is a spiral galaxy as well.