Scientists Don’t Fully Understand Quantum Entanglement—but They Know That Space, Or Physical Distance,

Measuring Distances To Stars Just Got A Whole Lot Easier Thanks To This “Stellar Twin” Trick

Scientists have developed a novel method to calculate the distances to stars, and it could be useful in helping map the size of galaxies. The study is published in the Monthly Notices of the Royal Astronomical Society.

The researchers from the University of Cambridge examined what are known as “stellar twins.” These are stars that are identical, with exactly the same chemical composition, which can be worked out from their spectra – the type of light they emit. If they were both placed at the same distance from Earth, they would shine with equal brightness.

So the team realized that if the distance to just one of the stars was known, the other could be calculated relatively easily based on how brightly it was shining. The dimmer it is, the further away it is, and vice versa. The method can be used to accurately measure the distance.

“It’s a remarkably simple idea – so simple that it’s hard to believe no one thought of it before,” said lead author Dr Paula Jofre Pfeil, from Cambridge’s Institute of Astronomy, in a statement. “The further away a star is, the fainter it appears in the sky, and so if two stars have identical spectra, we can use the difference in brightness to calculate the distance.”

Read more ~ IFL Science

Photo credit: RealCG Animation Studio. Shutterstock.

Associated Press

GENEVA — Physicists on the team that measured particles traveling faster than light said Friday they were as surprised as their skeptics about the results, which appear to violate the laws of nature as we know them.

Hundreds of scientists packed an auditorium at one of the world’s foremost laboratories on the Swiss-French border to hear how a subatomic particle, the neutrino, was found to have outrun light and confounded the theories of Albert Einstein.

“To our great surprise we found an anomaly,” said Antonio Ereditato, who participated in the experiment and speaks on behalf of the team.

An anomaly is a mild way of putting it.

Going faster than light is something that is just not supposed to happen, according to Einstein’s 1905 special theory of relativity. The speed of light — 186,282 miles per second (299,792 kilometers per second) — has long been considered a cosmic speed limit.

The team — a collaboration between France’s National Institute for Nuclear and Particle Physics Research and Italy’s Gran Sasso National Laboratory — fired a neutrino beam 454 miles (730 kilometers) underground from Geneva to Italy.

They found it traveled 60 nanoseconds faster than light. That’s sixty billionth of a second, a time no human brain could register.

“You could say it’s peanuts, but it’s not. It’s something that we can measure rather accurately with a small uncertainty,” Ereditato told The Associated Press.

If the experiment is independently repeated — most likely by teams in the United States or Japan — then it would require a fundamental rethink of modern physics.

“Everybody knows that the speed limit is c, the speed of light. And if you find some matter particle such as the neutrino going faster than light, this is something which immediately shocks everybody, including us,” said Ereditato, a researcher at the University of Bern, Switzerland.

Physicists not involved in the experiment have been understandably skeptical.

Alvaro De Rujula, a theoretical physicist at CERN, the European Organization for Nuclear Research outside Geneva from where the neutron beam was fired, said he blamed the readings on a so-far undetected human error.

If not, and it’s a big if, the door would be opened to some wild possibilities.

The average person, said De Rujula, “could, in principle, travel to the past and kill their mother before they were born.”

But Ereditato and his team are wary of letting such science fiction story lines keep them up at night.

“We will continue our studies and we will wait patiently for the confirmation,” he told the AP. “Everybody is free to do what they want: to think, to claim, to dream.”

He added: “I’m not going to tell you my dreams.”

NASA Astronomy Picture of the Day 2016 February 11 

LIGO Detects Gravitational Waves from Merging Black Holes 

Gravitational radiation has been directly detected. The first-ever detection was made by both facilities of the Laser Interferometer Gravitational-Wave Observatory (LIGO) in Washington and Louisiana simultaneously last September. After numerous consistency checks, the resulting 5-sigma discovery was published today. The measured gravitational waves match those expected from two large black holes merging after a death spiral in a distant galaxy, with the resulting new black hole momentarily vibrating in a rapid ringdown. 

A phenomenon predicted by Einstein, the historic discovery confirms a cornerstone of humanity’s understanding of gravity and basic physics. It is also the most direct detection of black holes ever. The featured illustration depicts the two merging black holes with the signal strength of the two detectors over 0.3 seconds superimposed across the bottom. Expected future detections by Advanced LIGO and other gravitational wave detectors may not only confirm the spectacular nature of this measurement but hold tremendous promise of giving humanity a new way to see and explore our universe.

Looks like they could kill you but is actually a cinnamon roll: W Boson

Looks like a cinnamon roll but could actually kill you: Photon

Looks like they could kill you and can actually kill you: Z Boson

Looks like a cinnamon roll and is actually a cinnamon roll: Gluon

Spinnamon Roll: Higgs Boson

A High-Bandwidth Interplanetary Connection

(click picture for link)

“A new study suggests that by twisting laser light, scientists could pack enough information into interplanetary beams to speed up extraterrestrial communications to the multi-gigabit level.…”

The liquid oxygen/liquid methane engine, developed by Armadillo Aerospace with help from NASA, is tested in the vacuum chamber at NASA’s White Sands Test Facility, August 2009. (NASA)

7 Things to Know About Spacewalks

On Wednesday, Oct. 28 and Friday, Nov. 6, Commander Scott Kelly and Flight Engineer Kjell Lindgren will perform spacewalks in support of space station assembly and maintenance. You can watch both of these events live on NASA Television. But, before you do, here are 7 things to know:

1. What’s the Point of a Spacewalk?

Spacewalks are important events where crew members repair, maintain and upgrade parts of the International Space Station. Spacewalks can also be referred to as an EVA – Extravehicular Activity. On Wednesday, Oct. 28, Commander Scott Kelly and Flight Engineer Kjell Lindgren will complete a spacewalk. During this time they will service the Canadarm2 robotic arm, route cables for a future docking port, and place a thermal cover over a dark matter detection experiment, which is a state-of-the-art particles physics detector that has been attached to the station since 2011.

2. What Do They Wear?

The Extravehicular Mobility Unit (EMU) spacewalking suit weighs around 350 pounds. It’s weightless in space, but mass is still very real. The EMU provides a crew member with life support and an enclosure that enables them to work outside the space station. The suit provides atmospheric containment, thermal insulation, cooling, solar radiation protection and micrometeoroid/orbital debris protection.

3. How Long Are Spacewalks?

Spacewalks typically last around 6 ½ hours, but can be extended to 7 or 8 hours, if necessary. The timeline is designed to accommodate as many tasks as possible, as spacewalks require an enormous amount of work to prepare.

4. What About Eating and Drinking?

Before a spacewalk astronauts eat light, usually something like a protein bar. The spacesuits also have a drink bag inside, and there is a bite valve that allows ready access to water.

5. What About Communication?

Spacewalkers wear a ‘comm’ cap that allows them to constantly communicate with astronauts inside the space station that are helping with the walk, and with mission control. Astronauts also wear a checklist on their left wrist called a “cuff checklist”. This list contains emergency procedures.

6. What About Light?

Something that most people don’t realize about spacewalks is that the crew will experience a sunrise/sunset every 45 minutes. Luckily, their spacesuits are equipped with lights that allow them to see in times of darkness.

7. How Do They Stay Safe?

When on a spacewalk, astronauts use safety tethers to stay close to their spacecraft. One end of the tether is hooked to the spacewalker, while the other end is connected to the vehicle. Another way astronauts stay safe is by wearing a SAFER, which is a Simplified Aid for EVA Rescue. This device is worn like a backpack and uses small jet thrusters to let an astronaut move around in space.

You can watch both of the upcoming spacewalks live on: NASA Television or the NASA App, or follow along on @Space_Station Twitter.

Wednesday, Oct. 28: Coverage begins at 6:30 a.m. EDT. Spacewalk begins at 8:10 a.m.

Friday, Nov. 6: Coverage begins at 5:45 a.m. EDT. Spacewalk begins at 7:15 a.m.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com 

Paranal red sprites

First imaged in 1989, red sprites are a ghostly phenomenon that occur at high altitudes above thunderstorms. Photographed here by ESO Photo Ambassador Petr Horálek, the unmistakable tendrils of multiple red sprites are spotted approximately 600 kilometres away from ESO’s Paranal Observatory above distant thunderclouds.

To capture multiple sprites in one image, two exposures were combined. The upper sprite occurred nearly 21 minutes before the lower one.

In the foreground sits a lone 1.8-metre Auxiliary Telescope, part of ESO’s Very Large Telescope (VLT).

Credit: P. Horálek/ESO

Quantum Vibrations Controlled For The First Time Ever, Could Help Find Gravitational Waves

A remarkable experiment has successfully seen the effects of “quantum motion” at a relatively large scale. These are essentially tiny vibrations caused on an atomic level when an object otherwise appears to be stationary. Among its many implications, the research – which was also able to temporarily stop the effect – could aid the hunt for elusive ripples in space-time called gravitational waves.

The study, published in the journal Science, was carried out by a team of researchers from the California Institute of Technology (Caltech) and collaborators. In classical physics, an object – such as a ball in a bowl – will eventually come to rest as the forces of gravity and friction act upon it. But in quantum mechanics, which governs the behavior of matter and light at an atomic scale, nothing is ever truly at rest.

This means that everything has an extremely small quantum noise, or motion; tiny vibrations at an atomic scale. In this experiment, the researchers were able to observe the effect not just at an atomic level, but at a larger micrometer-scale and, for the first time, control the effect.

To detect it, they placed a flexible aluminum plate on top of a silicon substrate. A superconducting electrical circuit was then used to vibrate the plate at 3.5 million times per second. Subsequently cooling the plate to 0.01 Kelvin (-273.14°C, -459.65°F) reduced the vibrations in a classical sense to zero, but probing it with microwave fields showed a small quantum motion – roughly the diameter of a proton, or 10,000 times smaller than a hydrogen atom.

“What we have found is that the motion of a micron scale object requires a quantum description,” co-author Keith Schwab from Caltech told IFLScience. “Classical physics just can’t capture the quantum noise we see.”

According to Schwab, the noise is an “unavoidable consequence of the Heisenberg Uncertainty Principle,” which essentially states that everything behaves like a particle and a wave at the same time. However, the team found that by carefully applying a controlled microwave field, they could reduce the motion in certain places, at the cost of making it much larger elsewhere. This technique is known as quantum squeezing.

Read more ~ IFL Science

Photo credit: agsandrew/Shutterstock.

A Pun on the Universe.