The faint, ephemeral glow emanating from the planetary nebula ESO 577-24 persists for only a short time – around 10,000 years, a blink of an eye in astronomical terms. ESO’s Very Large Telescope captured this shell of glowing ionized gas – the last breath of the dying star whose simmering remains are visible at the heart of this image. As the gaseous shell of this planetary nebula expands and grows dimmer, it will slowly disappear from sight.
This stunning planetary nebula was imaged by one of the VLT’s most versatile instruments, FORS2. The instrument captured the bright, central star, Abell 36, as well as the surrounding planetary nebula. The red and blue portions of this image correspond to optical emission at red and blue wavelengths, respectively.
An object much closer to home is also visible in this image – an asteroid wandering across the field of view has left a faint track below and to the left of the central star. And in the far distance behind the nebula a glittering host of background galaxies can be seen. Credit: ESO
Read more ~ phys.org
This is the 4th week of Deep, Dark, Space month!
This week’s entry is a not so “chilling” tale known as:
“The Big Crunch”
http://www.universetoday.com/37018/big-crunch/
http://www.iflscience.com/physics/big-crunch-back-possible-end-universe
Terrorism has once again shown it is prepared deliberately to stop at nothing in creating human victims. An end must be put to this. As never before, it is vital to unite forces of the entire world community against terror.
I believe that the world will know the blessing of peace only when the love for power is overthrown by the power of love.
To all the people of France, may the force be with you during these tough vicious times.
PC: shirtshovel
The Crab Pulsar (PSR B0531+21) is a relatively young neutron star. The star is the central star in the Crab Nebula, a remnant of the supernova SN 1054, which was widely observed on Earth in the year 1054. Discovered in 1968, the pulsar was the first to be connected with a supernova remnant.
The Crab Pulsar is one of very few pulsars to be identified optically. The optical pulsar is roughly 20 kilometres (12 mi) in diameter and the pulsar “beams” rotate once every 33 milliseconds, or 30 times each second.
The outflowing relativistic wind from the neutron star generates synchrotron emission, which produces the bulk of the emission from the nebula, seen from radio wavesthrough to gamma rays. The most dynamic feature in the inner part of the nebula is the point where the pulsar’s equatorial wind slams into the surrounding nebula, forming a termination shock.
The shape and position of this feature shifts rapidly, with the equatorial wind appearing as a series of wisp-like features that steepen, brighten, then fade as they move away from the pulsar into the main body of the nebula. The period of the pulsar’s rotation is slowing by 38 nanoseconds per day due to the large amounts of energy carried away in the pulsar wind.
The Crab Nebula is often used as a calibration source in X-ray astronomy. It is very bright in X-rays and the flux density and spectrum are known to be constant, with the exception of the pulsar itself.
source | A History of the Crab Nebula
images: NASA/ESA, Hubble, Cambridge University Lucky Imaging Group, NASA/CXC/ASU/J.Hester et al.
Celestial Buddy Earth peers out at Mother Earth from the ISS after hitching a ride on this weeks SpaceX Dragon test flight
“To myself I am only a child playing on the beach, while vast oceans of truth lie undiscovered before me.”
— Isaac Newton
Starry Greetings!
Seems like Planet X wanted to finish off Halloween with one… last…story…
https://cosmosmagazine.com/physics/vacuum-decay-ultimate-catastrophe
https://www.youtube.com/watch?v=ijFm6DxNVyI
http://io9.gizmodo.com/we-might-be-destroying-the-universe-just-by-looking-at-1514652112
The Space Station Transits Our Sun via NASA https://ift.tt/2RFTo9W
Seeing Titan : Shrouded in a thick atmosphere, Saturn’s largest moon Titan really is hard to see. Small particles suspended in the upper atmosphere cause an almost impenetrable haze, strongly scattering light at visible wavelengths and hiding Titan’s surface features from prying eyes. But Titan’s surface is better imaged at infrared wavelengths where scattering is weaker and atmospheric absorption is reduced. Arrayed around this centered visible light image of Titan are some of the clearest global infrared views of the tantalizing moon so far. In false color, the six panels present a consistent processing of 13 years of infrared image data from the Visual and Infrared Mapping Spectrometer (VIMS) on board the Cassini spacecraft. They offer a stunning comparison with Cassini’s visible light view. via NASA
i feel bad for math. its such a calm and friendly discipline full of beautiful and complex patterns and theres absolutely nothing inherently bad or oppressive about it but ppl treat it as though its evil and malicious. a lot of pure math lacks any kind of practical application or end goal, and just exists for the sake of stimulating peoples minds and pushing the limits of the medium as far as is possible. much like almost every kind of art
math means u no harm friends