Looks like perfectly habitable planet with water, lush green rainforests teeming with life.
Looks like perfectly habitable planet with water, lush green rainforests teeming with life.
Actual time lapse of an alien solar system (Composite, not sure if they've modelled anything)
Linky - http://www.manyworlds.space/index.p...stem-in-orbit-directly-imaged-and-remarkable/
That's incredible. Who'd have thought stars actually look like that.
That's incredible. Who'd have thought stars actually look like that.
That's incredible. Who'd have thought stars actually look like that.
Loving how good we as a species are getting really good at science... However should we be messing with other planets when we can't even look after our own?
Are we gonna be the 'bad guy aliens' from the movies, who strips a planet of all its resources, then moves on to the next?
Aye, and luckily for the black hole, it's located in the midst of a very, very active stellar nursery:That thing must have eaten a good part of a galaxy. Some aliens probably went with it.
Just the sheer dimension of its event horizon is disconcerting...The colossal galaxy cluster is also the brightest in X-ray light, and the galaxy at its heart apparently gives birth to more than 700 stars per year – hundreds of times as fast as our Milky Way forms stars, researchers say.
The diameter of the black hole's immense event horizon is on the order of 118 billion kilometres, 19 times the distance from the Sun to Pluto
A Nasa ultra HD shot of a small part of the Andromeda galaxy. 1 Trillion stars. Click on the image and zoom in. Its mindboggling.
https://www.nasa.gov/sites/default/files/thumbnails/image/hs-2015-02-a-hires_jpg.jpg
Yep, we have recently discovered that galaxy is teaming with badly animated life
The ultimate limits of the relativistic rocket equation. The Planck photon rocket
In this paper we look at the ultimate limits of a photon propulsion rocket. The maximum velocity for a photon propulsion rocket is just below the speed of light and is a function of the reduced Compton wavelength of the heaviest subatomic particles in the rocket. We are basically combining the relativistic rocket equation with Haug's new insight on the maximum velocity for anything with rest mass. An interesting new finding is that in order to accelerate any subatomic“fundamental” particle to its maximum velocity, the particle rocket basically needs two Planck masses of initial load. This might sound illogical until one understands that subatomic particles with different masses have different maximum velocities. This can be generalized to large rockets and gives us the maximum theoretical velocity of a fully-efficient and ideal rocket. Further, no additional fuel is needed to accelerate a Planck mass particle to ist maximum velocity; this also might sound absurd, but it has a very simple and logical solution that is explained in this paper.
That's incredible. Who'd have thought stars actually look like that.
Atmosphere found around Earth-like planet GJ 1132b
Image caption Artist's impression of GJ 1132b: The planet's thick atmosphere may contain water or methane
Scientists say they have detected an atmosphere around an Earth-like planet for the first time.
They have studied a world known as GJ 1132b, which is 1.4-times the size of our planet and lies 39 light years away.
Their observations suggest that the "super-Earth" is cloaked in a thick layer of gasses that are either water or methane or a mixture of both.
The study is published in the Astronomical Journal.
Discovering an atmosphere, and characterising it, is an important step forward in the hunt for life beyond our Solar System.
But it is highly unlikely that this world is habitable: it has a surface temperature of 370C.
Dr John Southworth, the lead researcher from Keele University, said: "To my knowledge the hottest temperature that life has been able to survive on Earth is 120C and that's far cooler than this planet."
Chemical signatures
The discovery of planet GJ 1132b was first announced in 2015. It lies in the Vela constellation in the southern hemisphere.
One possibility is that it is a 'water world' with an atmosphere of hot steam
While it is a similar size to Earth, the star it orbits is much smaller, cooler and dimmer than our Sun.
Using a telescope at the European Southern Observatory in Chile, the researchers were able to study the planet by watching how it blocked some of the light of its host star as it passed in front of it.
"It makes the star look a little bit fainter - and it's actually a very good way of finding transiting planets - it's how this one was found," said Dr Southworth.
But different molecules in a planet's atmosphere - if it has one - absorb light in different ways, allowing scientists to look for their chemical signatures when the world transits its star.
The observations of planet GJ 1132b suggest that it has a thick atmosphere containing either steam and/or methane.
"One possibility is that it is a 'water world' with an atmosphere of hot steam," said Dr Southworth.
The researchers say while it is unlikely that any life-forms could survive on this world, the discovery of an atmosphere is encouraging in the hunt for extraterrestrial life.
Dr Southworth said: "What we have shown is that planets around low mass stars can have atmospheres and because there are so many of those in the Universe, it makes it that much more likely that one might have life."
Commenting on the research Marek Kukula, the public astronomer at the Royal Observatory Greenwich, said: "This is a nice proof of concept.
"If the technology can detect an atmosphere today, then it bodes well for being able to detect and study the atmospheres of even more Earth-like planets in the not-too-distant future."
http://www.bbc.co.uk/news/science-environment-39521344
Prolly get to Mars for that by then.If someone puts $10k in a passive global fund today, if *should* turn into $100k in todays money before 40 years time.
Probably the cost of a trip to LEO will have also come down to that price.
One last hurrah?
https://www.nasa.gov/feature/goddard/2016/a-dead-stars-ghostly-glowA Dead Star's Ghostly Glow
The eerie glow of a dead star, which exploded long ago as a supernova, reveals itself in this NASA Hubble Space Telescope image of the Crab Nebula. But don't be fooled. The ghoulish-looking object still has a pulse. Buried at its center is the star's tell-tale heart, which beats with rhythmic precision.
The "heart" is the crushed core of the exploded star. Called a neutron star, it has about the same mass as the sun but is squeezed into an ultra-dense sphere that is only a few miles across and 100 billion times stronger than steel. The tiny powerhouse is the bright star-like object near the center of the image.
This surviving remnant is a tremendous dynamo, spinning 30 times a second. The wildly whirling object produces a deadly magnetic field that generates an electrifying 1 trillion volts. This energetic activity unleashes wisp-like waves that form an expanding ring, most easily seen to the upper right of the pulsar.
The nebula's hot gas glows in radiation across the electromagnetic spectrum, from radio to X-rays. The Hubble exposures were taken in visible light as black-and-white exposures. The Advanced Camera for Surveys made the observations between January and September 2012. The green hue that gives the nebula a Halloween theme, represents the color range of filter used in the observation.
NASA will discuss new results about ocean worlds in our solar system from the agency’s Cassini spacecraft and the Hubble Space Telescope during a news briefing 11 a.m. PDT (2 p.m. EDT) on Thursday, April 13. The event, to be held at NASA Headquarters in Washington, will include remote participation from experts across the country.
The briefing will be broadcast live on NASA Television and the agency's website.
These new discoveries will help inform future ocean world exploration -- including NASA’s upcoming Europa Clipper mission planned for launch in the 2020s -- and the broader search for life beyond Earth.
The news briefing participants will be:
- Thomas Zurbuchen, associate administrator, Science Mission Directorate at NASA Headquarters in Washington
- Jim Green, director, Planetary Science Division at NASA Headquarters
- Mary Voytek, astrobiology senior scientist at NASA Headquarters
- Linda Spilker, Cassini project scientist at NASA’s Jet Propulsion Laboratory in Pasadena, California
- Hunter Waite, Cassini Ion and Neutral Mass Spectrometer (INMS) team lead at the Southwest Research Institute (SwRI) in San Antonio
- Chris Glein, Cassini INMS team associate at SwRI
- William Sparks, astronomer with the Space Telescope Science Institute in Baltimore
Members of the public can ask questions during the briefing using #AskNASA.
The event will also be streamed live at:
YouTube.com/nasajpl/live
http://www.cbc.ca/news/technology/dark-matter-detected-1.4068001Researchers at the University of Waterloo have created the first map showing how our universe's elusive dark matter interacts with galaxies. Dark matter makes up about 25 per cent of our universe. However, it's invisible: its presence is only detectable through its gravity and how it interacts with galaxies. One way astronomers can "see" dark matter is through something called gravitational lensing. Because of its extreme gravity, dark matter bends light, in keeping with Einstein's theory of general relativity. This phenomenon is depicted below in an animation created with Hubble Space Telescope imagery.
It's been theorized that galaxies are connected through dark matter in a type of cosmic web. However, until now there has never been quantitative evidence. Using the Canada-France-Hawaii Telescope, the researchers were able to detect the dark matter through weak gravitational lensing. This lensing effect only changes about one per cent of a galaxy's shape. The image created is a composite using images from more than 23,000 pairs of galaxies located about 4.5 billion light-years away. What's seen is the bridge connecting galaxies.
"It's opening up essentially a new window to understanding where the dark matter is in the universe and how much of it there is and how it's distributed in space," said Mike Hudson, co-author of the paper published in the Monthly Notices of the Royal Astronomical Society. "This is a step forward in convincing us that, yes, it's really there," Hudson said. The next step is to look at more galaxies that are farther away to get a better picture of how dark matter evolved over time.