Black Holes & Co.
— filed under: g-spotlight-c2
Black holes, neutron stars and supernovae: Flight into a black hole, the black hole in the center of the Milky Way, how many different kinds of black hole are there, how black holes light up their neighbourhood
This page features an overview of all our Spotlights dealing with black holes and other compact objects, notably neutron stars. Under the heading Close encounters with black holes, a Spotlight explores what an observer on a space-ship would see as, step by step, the ship approaches a black hole. The texts in the category How to track compact objects explores the phenomena that can be used by astronomers to track black holes and other compact objects in their telescopes, from their gravitational influence on neighbouring stars to the different ways that compact objects have of lighting up their immediate cosmic neighbourhood. The category The physics of black holes is dedicated to general theorems that have been proved about these objects. The category Physics in the background explores some physics that is useful for a better understanding of the Spotlights dealing with black holes and neutron stars.
Close encounters with black holes
The story of an expedition's closer and closer approach to a black hole - too close?
How to track compact objects
More about the gravitational influence of black holes and neutron stars on their cosmic surroundings, from the orbits of nearby stars to accretion disks and the associated luminous phenomena.
Information about the closest supermassive black hole - the central object of our own galaxy
How the fact that black holes are very efficient in attracting surrounding matter leads to some of the most spectacularly luminous phenomena in the whole of the cosmos
What astronomers can see once a black hole has heated up its cosmic neighbourhood, stimulating it to emit bright radiation
The physics of black holes
Once they have settled down, there are actually only very few different kinds of black hole - find out which, and how black holes shed other distinguishing marks.
The intriguing possibility that the next generation of particle accelerators might produce - and allow the detection of - miniature black holes
How, in one sense, space and time switch their roles inside a black hole - and why this leads to a black hole's most characteristic property, namely that nothing can get out
Physics in the background
Some information about what is called the conservation of angular momentum, and its consequences for neutron stars, black holes and the matter disks around them
The connection between temperature and the emission of electromagnetic radiation, as well as the consequences for stars, matter disks around black holes, and cosmology