Space Science

A Nepalese official says five climbers are missing and feared dead on the world's third highest mountain.

Police say actress Amanda Bynes has been arrested in midtown Manhattan after she heaved a marijuana bong out of a window.

An Interstate 5 bridge over a river north of Seattle collapsed Thursday evening, dumping several vehicles into the water as authorities investigated the cause of the collapse that cut off the state's main north-south thruway and sent three people to the hospital.

An Interstate 5 bridge over a river north of Seattle collapsed Thursday evening, dumping vehicles and people into the water, the Washington State Patrol said.

An earthquake has struck Northern California's Plumas County with a preliminary magnitude of 5.7.

Scott Walker tried to introduce himself to Iowa Republicans Thursday as so many would-be presidential candidates often do — one of their own.

Dan Brown's description of Manila as "the gates of hell" in the American novelist's latest book has not gone down well with officials in the Philippine capital.

Astronomers catch two giant galaxies merging in images from Europe's Herschel space telescope - The Verge. #space

A study notes "a lot of excitement and interest from various companies" for such ventures.

“Because dark energy makes up about 70 percent of the content of the universe, it dominates over the matter content. That means dark energy will govern expansion and, ultimately, determine the fate of the universe.” -Eric Linder It’s been a while since we’ve spoken about dark energy, and we were just talking about Einstein’s greatest blunder, so let’s just dive right in. Image credit: S. Beckwith & the HUDF Working Group (STScI), HST, ESA, NASA. This is our observable Universe, as unveiled by the Hubble Space Telescope. With hundreds of billions of galaxies stretched out some 41 billion light years in all directions, finding out about what our Universe was like in the distant past, the recent past, and what it’s like today is limited only by our willingness to look. In particular, there are three great sets of observations that tell us ever so much about the Universe on the largest scales. Image credit: Northern Galactic Cap from the SDSS-III release, via http://www.sdss3.org/. 1.) The way galaxies cluster together on the largest scales. By looking at huge, tremendous surveys of galaxies, we can see how the visible matter in the Universe has clustered, clumped, and grouped together, as well as where it hasn’t, and has left us great cosmic voids. By putting various ingredients into a model Universe governed by General Relativity, we can also simulate how structure should form in our Universe. Where the simulations and the observations match up, that tells us what’s in our Universe. Image credit: ESA and the Planck Collaboration. 2.) The temperature fluctuations in the cosmic microwave background. By looking at the temperature fluctuations — the hot-and-cold spots — in the CMB, we can know what the Universe looked like in terms of overdensities, underdensities, and how they’re clustered with respect to one another all the way back at a time when the Universe was just some 380,000 years old! Because the light has had to travel for nearly the entire 13.8 billion years that the Universe has been around (it’s been traveling for 99.997% of the Universe’s history), we can find out information about what the Universe was like back then, but also how it’s expanded since then. This pattern of fluctuations also tells us what the various combinations of ingredients are in our Universe. Image credit: Kowalski et al., Ap.J., 2008. 3.) Direct observations of well-understood objects at various distances/redshifts in the Universe. Everything from variable stars to properties of galaxies to distant supernovae help us get a handle on this, the cosmic distance ladder. This tells us how the Universe has been expanding since as far back as we can measure until the present day. When these three data sets are combined — and we can combine others, too, but these three are the best data sets we have — they tell us that there’s matter in the Universe, about 31-32% of the Universe is matter (most of which is dark matter), and that there’s another type of energy, dark energy, that makes up the rest. Image credit: Planck Collaboration: P. A. R. Ade et al., 2013, A&A Preprint; annotations by me. So, you ask, just what is dark energy, and how do we know? In principle — and by in principle, I mean in General Relativity — matter, energy, topological defects, and pretty much anything else that you throw into your Universe is going to affect how your Universe expands because of two properties inherent to it: it’s energy density and its pressure. Image credit: Large Synoptic Survey Telescope, NSF, DOE, and AURA. Because of the way the Universe is observed to expand, and because of the known way that matter (yes, even dark matter, according to General Relativity) behaves, we can infer something about the energy density and pressure of dark energy. In particular, we know that dark energy’s pressure is negative, and that it’s quite negat