GORGEOUS PHOTOS - Earth and the Night Sky: TWAN Photo Contest Winners Announced

Gorgeous Photos of Earth and the Night Sky: TWAN Photo Contest Winners Announced:

The winners of the 7th annual Earth & Sky Photo Contest have been announced, and wow, these images are absolutely stunning! The contest really highlights the beauty of the night sky, and its mission is to spread the message to cut down on light pollution while helping to preserve the last remaining natural night environments and night skies in the world. The contest was organized by The World at Night (TWAN) and other sister organizations.



"The sky above us is an essential part of our nature, a heritage for us and other species on this planet,” said TWAN founder and contest chair, Babak Tafreshi.”The contest main goal is to present the night sky in this broader context that helps preserving the natural night sky by reconnect it with our modern life."



See more winning photos below:











Just last week, a group of Italian and American scientists unveiled a new global atlas of light pollution, and sadly, they said the results show the Milky Way is “but a faded memory to one-third of humanity and 80 percent of Americans.”



“We’ve got whole generations of people in the United States who have never seen the Milky Way,” said Chris Elvidge, a scientist with NOAA’s National Centers for Environmental Information. “It’s a big part of our connection to the cosmos — and it’s been lost.”



These photos from Earth & Sky Contest really display that important connection, with people and places on Earth being a big part of many of the images – the classic definition of “TWAN-style” photography. According to the contest theme of “Dark Skies Importance,” the submitted photos were judged in two categories: “Beauty of The Night Sky” and “Against the Lights.”



“The selected images are those most effective in impressing public on both how important and delicate the starry sky is as an affecting part of our nature, and also how bad the problem of light pollution has become,” TWAN said in their press release. “Today, most city skies are virtually devoid of stars. Light pollution (excessive light that scatters to the sky instead of illuminating the ground) not only is a major waste of energy, it also obscures the stars, disrupts ecosystems and has adverse health effects.”







The winning images were chosen on their "aesthetic merit and technical excellence," said David Malin of the judging panel, who is well-known pioneer in scientific astrophotography. "We believe they accurately reflect the state of the art in TWAN-style photography. The competition encourages photographers with imagination to push their cameras to their technical limits, and to produce eye-catching images that appear perfectly natural and are aesthetically pleasing."













The contest was open to anyone of any age, anywhere in the world; to both professional and amateur/hobby photographers. It has been an annual event since 2009 (initially for the International Year of Astronomy) by TWAN, the National Optical Astronomy Observatory, and Global Astronomy Month from Astronomers Without Borders. The contest supports efforts of the International Dark Sky Association (IDA) and other organizations that seek to preserve the night sky.



The images were taken in 57 countries and territories including Algeria, Antarctica, Australia, Austria, Bahamas, Belgium, Bolivia, Brazil, Canada, China, Colombia, Croatia, Czech Republic, Egypt, England, Estonia, Finland, France, Germany, Greece, Guatemala, Guam, Hungary, Iceland, India, Indonesia, Iran, Ireland, Italy, Japan, Jordan, Kenya, Lithuania, Madagascar, Malaysia, Malta, Morocco, Norway, New Zealand, Paraguay, Peru, Philippines, Poland, Reunion (France), Romania, Russia, Scotland, Sri Lanka, South Africa, Spain, South Africa, Sri Lanka, Sweden, Switzerland, Tanzania, Thailand, Ukraine, and USA.



See all the images and more information about them at TWAN. Click on each image for larger versions. A larger version of the lead image can be found here.



You can see the global atlas of light pollution here, which was created from data from the NOAA/NASA Suomi National Polar-orbiting Partnership satellite and calibrated by thousands of ground observations.



And here's a video that includes all the winning images:





The post Gorgeous Photos of Earth and the Night Sky: TWAN Photo Contest Winners Announced appeared first on Universe Today.

PLUTO PLANET - Peering for Pluto: Our Guide to Opposition 2016

Peering for Pluto: Our Guide to Opposition 2016:

What an age we live in. This summer marks the very first opposition of Pluto since New Horizons' historic flyby of the distant world in July 2015. If you were like us, you sat transfixed during the crucial flyby phase, the climax of a decade long mission. We now live in an era where Pluto and its massive moon Charon are a known worlds, something that even Pluto discoverer Clyde Tombaugh never got to see.



Pluto in 2016



And this summer, with a little skill and patience and a good-sized telescope, you can see Pluto for yourself. Opposition 2016 sees the remote world looping through the star-rich fields of eastern Sagittarius. Hovering around declination 21 degrees south, +14.1 magnitude Pluto is higher in the June skies for observers in the southern hemisphere than the northern, but don't let that stop you from trying. Opposition occurs on July 7th, when Pluto rises opposite from the setting Sun and rides across the meridian at 29 degrees above the southern horizon for observers based along 40 degrees north latitude at local midnight.







Pluto actually crossed the plane of the galactic equator in 2009, and won't cross the celestial equator northward until 2109. Fun fact: astronomer Clyde Tombaugh discovered Pluto as it drifted through the constellation Gemini in 1930. Here we are 86 years later, and Pluto has only moved six zodiacal constellations along the ecliptic eastward in its 248 year orbit around the Sun.







And Pluto is getting tougher to catch in a backyard scope, as well. The reason: Pluto passed perihelion or its closest point to the Sun in 1989 inside the orbit of Neptune, and it's now headed out to aphelion about a century from now in 2114. Pluto is in a fairly eccentric orbit, ranging from 29.7 astronomical units (AU) to 49.4 AU from the Sun. This also means that Pluto near opposition can range from a favorable magnitude +13.7 near perihelion, to three magnitudes (16 times) fainter near aphelion hovering around magnitude +16.3. Clyde was lucky, in a way. Had Pluto been near aphelion in the 20^th century rather than headed towards perihelion, it might have waited much longer for discovery.



2016 sees Pluto shining at +14.1, one magnitude (2.5 times) above the usual quoted mean. See Mars over in the constellation Libra shining at magnitude -1.5? It's 100^3 (a 5-fold change in magnitude is equal to a factor of 100 in brightness), or over a million times brighter than Pluto.







You often see Pluto quoted as visible in a telescope aperture of 'six inches or larger,' but for the coming decade, we feel this should be amended to 8 inches and up. We once nabbed Pluto during public viewing using the 14” reflector at the Flandrau observatory.



And how about Pluto's large moon, Charon? Shining at an even fainter +16th magnitude, Charon never strays more than 0.9” from Pluto... still, diligent amateurs have indeed caught the elusive moon... as did Wendy Clark just last year.







Lacking a telescope? Hey, so are we, as we trek through Morocco this summer... never fear, you can still wave in the general direction of Pluto and New Horizons on the evening of June 21^st, one day after the northward solstice and the Full Moon, which passes three degrees north of Pluto.







And follow that spacecraft, as New Horizons is set to make a close pass by Kuiper Belt Object 2014 MU69 in January 2019 on New Year's Day.



A key date to make your quest for Pluto is June 26^th, when Pluto sits just 3' minutes to the south of the +2.9 magnitude star Pi Sagittarii (Albaldah), making a great guidepost.



Does the region of Sagittarius near Pi Sagittarii sound familiar? That's because the Wow! Signal emanated from a nearby region of the sky on August 15^th, 1977. Pluto will cross the border into the constellation Capricornus in 2024.



After opposition, Pluto heads into the evening sky, towards solar conjunction on January 7^th, 2017.



Observing Pluto requires patience, dark skies, and a good star chart plotted down to about +15^th magnitude. One key problem: many star charts don't go down this faint. We use Starry Night Pro 7, which includes online access to the USNO catalog and a database of 500 million stars down to magnitude +21, more than enough for most backyard scopes.



Don't miss a chance to see Pluto for yourself this summer!

The post Peering for Pluto: Our Guide to Opposition 2016 appeared first on Universe Today.

UNDERSTANDING THE UNIVERSE - Second Gravitational Wave Source Found By LIGO

Second Gravitational Wave Source Found By LIGO:

Lightning has struck twice – maybe three times – and scientists from the Laser Interferometer Gravitational-wave Observatory, or LIGO, hope this is just the beginning of a new era of understanding our Universe. This “lightning” came in the form of the elusive, hard-to-detect gravitational waves, produced by gigantic events, such as a pair of black holes colliding. The energy released from such an event disturbs the very fabric of space and time, much like ripples in a pond. Today’s announcement is the second set of gravitational wave ripples detected by LIGO, following the historic first detection announced in February of this year.



“This collision happened 1.5 billion years ago,” said Gabriela Gonzalez of Louisiana State University at a press conference to announce the new detection, “and with this we can tell you the era of gravitational wave astronomy has begun.”



LIGO’s first detection of gravitational waves from merging black holes occurred Sept. 14, 2015 and it confirmed a major prediction of Albert Einstein’s 1915 general theory of relativity. The second detection occurred on Dec. 25, 2015, and was recorded by both of the twin LIGO detectors.



While the first detection of the gravitational waves released by the violent black hole merger was just a little “chirp” that lasted only one-fifth of a second, this second detection was more of a “whoop” that was visible for an entire second in the data. Listen in this video:









“This is what we call gravity’s music,” said González as she played the video at today’s press conference.



While gravitational waves are not sound waves, the researchers converted the gravitational wave’s oscillation and frequency to a sound wave with the same frequency. Why were the two events so different?



From the data, the researchers concluded the second set of gravitational waves were produced during the final moments of the merger of two black holes that were 14 and 8 times the mass of the Sun, and the collision produced a single, more massive spinning black hole 21 times the mass of the Sun. In comparison, the black holes detected in September 2015 were 36 and 29 times the Sun’s mass, merging into a black hole of 62 solar masses.



The scientists said the higher-frequency gravitational waves from the lower-mass black holes hit the LIGO detectors’ “sweet spot” of sensitivity.



“It is very significant that these black holes were much less massive than those observed in the first detection,” said Gonzalez. “Because of their lighter masses compared to the first detection, they spent more time—about one second—in the sensitive band of the detectors. It is a promising start to mapping the populations of black holes in our universe.”







LIGO allows scientists to study the Universe in a new way, using gravity instead of light. LIGO uses lasers to precisely measure the position of mirrors separated from each other by 4 kilometers, about 2.5 miles, at two locations that are over 3,000 km apart, in Livingston, Louisiana, and Hanford, Washington. So, LIGO doesn’t detect the black hole collision event directly, it detects the stretching and compressing of space itself. The detections so far are the result of LIGO’s ability to measure the perturbation of space with an accuracy of 1 part in a thousand billion billion. The signal from the lastest event, named GW151226, was produced by matter being converted into energy, which literally shook spacetime like Jello.



LIGO team member Fulvio Ricci, a physicist at the University of Rome La Sapienzaa said there was a third “candidate” detection of an event in October, which Ricci said he prefers to call a “trigger,” but it was much less significant and the signal to noise not large enough to officially count as a detection.



But still, the team said, the two confirmed detections point to black holes being much more common in the Universe than previously believed, and they might frequently come in pairs.



“The second discovery “has truly put the ‘O’ for Observatory in LIGO,” said Albert Lazzarini, deputy director of the LIGO Laboratory at Caltech. “With detections of two strong events in the four months of our first observing run, we can begin to make predictions about how often we might be hearing gravitational waves in the future. LIGO is bringing us a new way to observe some of the darkest yet most energetic events in our universe.”



LIGO is now offline for improvements. Its next data-taking run will begin this fall and the improvements in detector sensitivity could allow LIGO to reach as much as 1.5 to two times more of the volume of the universe compared with the first run. A third site, the Virgo detector located near Pisa, Italy, with a design similar to the twin LIGO detectors, is expected to come online during the latter half of LIGO’s upcoming observation run. Virgo will improve physicists’ ability to locate the source of each new event, by comparing millisecond-scale differences in the arrival time of incoming gravitational wave signals.



In the meantime, you can help the LIGO team with the Gravity Spy citizen science project through Zooniverse.



Sources for further reading:

Press releases:

University of Maryland

Northwestern University

West Virginia University

Pennsylvania State University

Physical Review Letters: GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence

LIGO facts page, Caltech



For an excellent overview of gravitational waves, their sources, and their detection, check out Markus Possel's excellent series of articles we featured on UT in February:



Gravitational Waves and How They Distort Space



Gravitational Wave Detectors and How They Work



Sources of Gravitational Waves: The Most Violent Events in the Universe



The post Second Gravitational Wave Source Found By LIGO appeared first on Universe Today.

NASA IMAGES - What Are Virtual Particles?

What Are Virtual Particles?:





Sometimes I figure out the weak spot in my articles based on the emails and comments they receive.

One popular article we did was all about Stephen Hawking’s realization that black holes must evaporate over vast periods of time. We talked about the mechanism, and mentioned how there are these virtual particles that pop in and out of existence.

Normally these particles self annihilate, but at the edge of a black hole’s event horizon, one particle falls in, while another is free to wander the cosmos. Since you can’t create particles from nothing, the black hole needs to sacrifice a little bit of itself to buy this newly formed particle’s freedom.

But my short article wasn’t enough to clarify exactly what virtual particles are. Clearly, you all wanted more information. What are they? How are they detected? What does this mean for black holes?

In situations like this, when I know the actual Physics Police are watching, I like to call in a ringer. Once again, I’m going to go back and talk to my good friend, and actual working astrophysicist, Dr. Paul Matt Sutter. He has written papers on subjects like the Bayesian Analysis of Cosmic Dawn and MHD Simulations of Magnetic Outflows. He really knows his stuff.

---

Fraser Cain:

Hey Paul, first question: What are virtual particles?

Paul Matt Sutter:

Alright. No pressure, Fraser. Okay, okay.

To get the concept of virtual particles you actually have to take a step back and think about the field, especially the electromagnetic field. In our current view of how the universe works all of space and time is filled up with this kind of background field. And this field can wibble and wabble around, and sometimes these wibbles and wabbles are like waves that propagate forward, and we call these waves photons or electromagnetic radiation, but sometimes it can just sit there and you know bloop bloop bloop, just you know pop fizzle in and out, or up and down, and kind of boil a little all on its own.

In fact all the time space is kind of wibbling/wabbling around this field even in a vacuum. A vacuum isn’t the absence of everything. The vacuum is just where this field is in its lowest energy state. But even though it’s in that lowest energy state, even though maybe on average there is nothing there. There’s nothing stopping it from just bloop bloop bloop you know bubbling around.

Credit: NASA, ESA, Q.D. Wang (University of Massachusetts, Amherst), and S. Stolovy (Caltech)

So actually the vacuum is kind of boiling with these fields. In particular the electromagnetic field which is what we are talking about right now.

And we know that photons, that light, can turn into particle, anti-particle pairs. It can turn into say an electron and a positron. It can just do this. It can happen to normal photons, and it can happen to these kind of temporary wibbly wobbly photons.

So sometimes a photon or sometimes the electromagnetic field can propagate from one place to another, and we call it a photon. And that photon can split off into a positron and an electron, and other times it can just wibble wobble kind of in place and then wibble wobble POP POP. It pops into a positron and an electron and then they crash into each other or whatever, and they just simmer back down. So, wibble wobble, pop pop, fizz fizz is kind of what’s going on in the vacuum all they time, and that’s the name we give these virtual particles are just the normal kind of background fuzz or background static to the vacuum.

Fraser:

Okay. So how do we see evidence for virtual particles?

Paul:

Yeah, great question. We know that the vacuum has an energy associated with it. We know that these virtual particles are always fizzing in and out of existence for a few reasons.

One is the transition of the electron in different states of the atom. If you excite the atom the electron pops up to a higher energy state. There is kind of no reason for that electron to pop back down to a lower energy state. It’s already there. It’s actually a stable state. There is no reason for it to leave unless there is little wibble wobbles in the electromagnetic field and it can giggle around that electron and knock it out of that higher energy state and send it crashing down into a lower state

Another thing is called the Lamb Shift, and this is when the wibbly wobbly electromagnetic field or the virtual particles interact again with electrons in say a hydrogen atom. It can gently nudge them around, and this shift effects some states of the electron and not other states. And there are actually states that you would say have the exact same say energy properties, they are just kind of identical, but because the Lamb Shift, because of this wibbly wobbly electromagnetic field interacts with one of those states and not the other, it actually subtly changes the energy levels of those states even though you’d expect them to be completely the same.

And another piece of evidence is in photon photon scattering usually two photons just, phweeet, fly by each other. They are electrically neutral, so they have no reason to interact, but sometimes the photons can wibble wobble into say electron/positron pairs, and that electron/positron pair can interact with the other photons. So sometimes they bounce off each other. It’s super rare because you have to wait for the wibble wobble to happen at just the right time, but it can happen.

Credit: NASA/Dana Berry/SkyWorks Digital

Fraser:

So how do they interact with black holes?

Paul:

Alright, this is the heart of the matter. What do all of these virtual particles or wibbly wobbly electromagnetic fields have to do with black holes, and specifically Hawking radiation? But check this out. Hawkings original formulation of this idea that black holes can radiate and lose mass actually has nothing to do with virtual particles. Or it doesn’t speak directly about virtual particle pairs, and in fact no other formulations or more modern conceptions of this process talk about virtual particle pairs.

Instead, they talk more about the field itself and specifically what’s happening to the field before the black hole is there, what’s happening to it as the black hole forms, and then what happens to the field after it’s formed. And it kind of asks a question: What happens to these wibbly wobbly bits of the field, these like transient kind of boiling nature of the vacuum of the electromagnetic field? What happens to it as that black hole is forming?

Well what happens is that some of the wibbly wobbly bits just get caught near the black hole, near the event horizon as it is forming, and they spend a long time there, and eventually they do escape. So it takes awhile, but when they escape because of the intense curvature there, the intense curvature of space-time, they can get boosted or promoted. So instead of being temporarily wibbly wobbly’s, in the field they get boosted to become “real” particles or “real” photons. So it’s really like an interaction of the formation of the black hole itself with the wibbly wobbly background field, that eventually escapes because it’s not quite trapped by the black hole.

Eventually it escapes and gets turned into real particles, and you can calculate like what happens with say the expected number of particles near the event horizon of the black hole. The answer is the negative number, which means the black hole is losing mass and spitting out particles.

Now this popular conception of virtual particle pairs popping into existence and one getting caught inside the event horizon. That’s is not exactly tied to the mathematics of Hawking radiation but it’s not exactly wrong either. Remember the wibbly wobbly’s in the electromagnetic field are related to these pairs of particles and anti-particles that are constantly popping in and out of existence. They kind of go hand in hand. So by talking about wibbly wobbly’s in the field you’re also kind of talking about the production of virtual particles. And it’s not exactly the math, but you know close enough.

An artist’s conception of a supermassive black hole’s jets. Image Credit: NASA / Dana Berry / SkyWorks Digital

Fraser:

Okay, and finally, Paul. I need you to just randomly blow the minds of the viewers. Something about virtual particles that is just amazing!

Paul:

Alright. So you want to bend people’s minds? All right. I was saving this for the last. Something juicy, just for you, Fraser.

Check this out, it’s one other big piece of evidence we have for the existence of these background fluctuations and the existence of virtual particles, and that’s something we call the Casimir Effect, or Casimir Force.

You take two neutral metal plates, and what happens is this field that permeates all of space-time is inside the plates and it’s outside the plates. Inside the plates, you can only have certain wavelengths of modes. Almost like the inside of a trumpet can only have certain modes that make sound. The ends of the wavelengths must connect to the plates, because that’s what metal plates do to electromagnetic fields.

Outside the plates you can have any wavelength you want. It doesn’t matter.

So it means outside the plates you have an infinite number of possible wavelengths of modes. Every kind of possible kind of fluctuation, wibble wabble in the electromagnetic field is there, but inside the plates it’s only certain wavelengths that can fit inside the plates.

Now, outside there’s an infinite number of modes. Inside, there is still an infinite number of modes, just slightly fewer infinite number of modes. And you can take the infinity on the outside, and subtract the infinite infinity on the inside, and actually get a finite number, and what you end up with is a pressure or a force that brings the plates together. And we have actually measured this. This is a real thing, and yes, I am not kidding around, you can take infinity minus a different infinity, and get a finite number. It’s possible. One example is the Euler Mascheroni Constant. I dare you to look it up!

---

So there you go, now I hope you understand what these virtual particles are, how they’re detected, and how they contribute to the evaporation of a black hole.

And if you haven’t already, make sure you click here and go to his channel. You’ll find dozens of videos answering equally mind-bending questions. In fact, send your questions and he might just make a video and answer them.

The post What Are Virtual Particles? appeared first on Universe Today.

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GALAXIES AND STARS - The Fornax Cluster of Galaxies

The Fornax Cluster of Galaxies:

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

2016 June 11

Explanation: Named for the southern constellation toward which most of its galaxies can be found, the Fornax Cluster is one of the closest clusters of galaxies. About 62 million light-years away, it is almost 20 times more distant than our neighboring Andromeda Galaxy, and only about 10 percent farther than the better known and more populated Virgo Galaxy Cluster. Seen across this two degree wide field-of-view, almost every yellowish splotch on the image is an elliptical galaxy in the Fornax cluster. A standout barred spiral galaxy NGC 1365 is visible on the lower right as a prominent Fornax cluster member. The spectacular image was taken by the VLT Survey Telescope at ESO's Paranal Observatory.

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WONDERFUL NEBULA IN THE SPACE - The Horsehead Nebula in Infrared from Hubble

The Horsehead Nebula in Infrared from Hubble:

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

2016 June 8

Explanation: While drifting through the cosmos, a magnificent interstellar dust cloud became sculpted by stellar winds and radiation to assume a recognizable shape. Fittingly named the Horsehead Nebula, it is embedded in the vast and complex Orion Nebula (M42). A potentially rewarding but difficult object to view personally with a small telescope, the above gorgeously detailed image was taken in 2013 in infrared light by the orbiting Hubble Space Telescope in honor of the 23rd anniversary of Hubble's launch. The dark molecular cloud, roughly 1,500 light years distant, is cataloged as Barnard 33 and is seen above primarily because it is backlit by the nearby massive star Sigma Orionis. The Horsehead Nebula will slowly shift its apparent shape over the next few million years and will eventually be destroyed by the high energy starlight.

PLUTO PLANET - Pluto at Night

Pluto at Night:

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

2016 June 9

Explanation: The night side of Pluto spans this shadowy scene. The spacebased view with the Sun behind the distant world was captured by New Horizons last July. The spacecraft was at a range of over 21,000 kilometers, about 19 minutes after its closest approach. A denizen of the Kuiper Belt in dramatic silhouette, the image also reveals Pluto's tenuous, surprisingly complex layers of hazy atmosphere. The crescent twilight landscape near the top of the frame includes southern areas of nitrogen ice plains informally known as Sputnik Planum and rugged mountains of water-ice in the Norgay Montes.

NASA IMAGE - NGC 6888: The Crescent Nebula

NGC 6888: The Crescent Nebula:

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

2016 June 10

NGC 6888: The Crescent Nebula

Image Credit & Copyright: Michael Miller, Jimmy Walker


Explanation: NGC 6888, also known as the Crescent Nebula, is a cosmic bubble about 25 light-years across, blown by winds from its central, bright, massive star. This sharp telescopic portrait uses narrow band image data that isolates light from hydrogen and oxygen atoms in the wind-blown nebula. The oxygen atoms produce the blue-green hue that seems to enshroud the detailed folds and filaments. Visible within the nebula, NGC 6888's central star is classified as a Wolf-Rayet star (WR 136). The star is shedding its outer envelope in a strong stellar wind, ejecting the equivalent of the Sun's mass every 10,000 years. The nebula's complex structures are likely the result of this strong wind interacting with material ejected in an earlier phase. Burning fuel at a prodigious rate and near the end of its stellar life this star should ultimately go out with a bang in a spectacular supernova explosion. Found in the nebula rich constellation Cygnus, NGC 6888 is about 5,000 light-years away.

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DEVICE FROM ALIENS ? Mysterious Greek Device Found To Be Astronomical Computer

Mysterious Greek Device Found To Be Astronomical Computer:

Thanks to a decade worth of high-tech imaging, the use of the ancient device called the Antikythera Mechanism can now be confirmed. The device, which was discovered over a century ago in an ancient shipwreck near the Greek island of Antikythera, was used as an astronomical computer.



Archaeologists long suspected that the device was connected to astronomy, but most of the writing on the instrument was indecipherable, which left some question. But a thorough, decade long effort using high-tech scanning methods has revealed much more of the text on the instrument.



The Antikythera Mechanism has about 14,000 characters of text on its mangled, time-weary body. Since its discovery over 100 years ago, very little of that text was readable, only a few hundred characters. It hinted at astronomical use, but detail remained frustratingly out of reach.



Now, the team behind this effort confirms that the mechanism was an astronomical calendar. It showed the position of the planets, the position of the Sun and Moon in the zodiac, the phases of the Moon, and it also predicted eclipses.



According to the team, it was like a teaching tool, or a kind of philosopher's guide to the galaxy.







The characters were engraved on the front and back sections of the device, and on the inside covers. Some of the writing was very small, only about 1.2 mm (1/20th of an inch) tall. The device itself was about the size of an office box file. It was contained in a wooden box, and was operated with a handle crank.



At the time that it was found, the device was largely an afterthought. The real find at the time was luxury glassware and ceramics, and statues made of bronze and marble found at the shipwreck by sponge divers. But the device attracted attention over the years as different scholars hypothesized what the mechanism was for and how the gears worked.



Professor Mike Edmunds, of Cardiff University, is the Chair of the Antikythera Mechanism Research Project. He said, "This device is just extraordinary, the only thing of its kind. The design is beautiful, the astronomy is exactly right. The way the mechanics are designed just makes your jaw drop. Whoever has done this has done it extremely carefully."



In fact, a device of this complexity did not appear anywhere for another thousand years.



The device itself is incomplete. The fragments that were found came from a shipwreck discovered in 1901. That ship was a mid-1st century BC ship, a large one for its time at 40 meters (130 ft) long. It's hoped that additional fragments of the device can be found by architects visiting the original shipwreck. But event though it's incomplete, most of the inscriptions are there, as are 20 gears that displayed planets.



According to the team responsible for imaging the text on the device, almost all of the text on the device's 82 fragments has been deciphered. It remains to be seen if any other surviving fragments, if found, will contain more text, and if that text will shed any more light on this remarkable device.



The post Mysterious Greek Device Found To Be Astronomical Computer appeared first on Universe Today.

SENDING COLONISTS TO MARS - These are the 40 Who Might Die on Mars

These are the 40 Who Might Die on Mars:

If there were an Olympics for ambition, the Dutch-based non-profit organization Mars One would surely be on the podium.



If you haven't heard of them, (and we expect you have,) they are the group that plans to send colonists to Mars on a one-way trip, starting in the year 2026. Only 24 colonists will be selected for the dubious distinction of dying on Mars, but that hasn't stopped 200,000 people from 140 countries from signing up and going through the selection process.



There are 100 people who have made it through the selection process so far. Another five day testing phase will knock that number down to 40, out of which 24 will be chosen as the lucky ones. The latest testing will start soon. According to Mars One, most of their testing is the same as the testing that NASA does on their astronauts.



At least some of the candidates have serious backgrounds. One, Zachary Gallegos, is a geologist and field chemist who works with the Mars Science Laboratory. Here's what he has to say:



[embed]https://www.youtube.com/watch?v=qEWzUGNnkNY#t=129[/embed]



All of this testing and narrowing down is partially funded by a reality show, which adds to the sort of carnival atmosphere around the whole thing, and makes it hard to take it seriously.



But, some people are serious about it.



In a statement, Mars One commented on the upcoming testing:



"Over the course of five days, candidates will face various challenges. It will be the first time all candidates will meet in person and demonstrate their capabilities as a team."



"In this round the candidates will play an active role in decision making/group formation. Mars One has asked the candidates to group themselves into teams with the people they believe they can work well with."



A human presence on Mars is a great idea, of course. But it seems fatalistic, and pointless, to choose to die there. And rest assured, these colonists are meant to die there.



Mars One addresses this kind of thinking on their website:

"For anyone not interested to go to Mars, moving permanently to Mars would be the worst kind of punishment. Most people would give an arm and a leg to be allowed to stay on Earth so it is often difficult for them to understand why anyone would want to go."



"Yet many people apply for Mars One’s mission and these are the people who dream about someday living on Mars. They would give up anything for the opportunity and it is often difficult for them to understand why anyone would not want to go."

Fair enough. Maybe these are the types of people who really contribute in driving humanity forward.



NASA is planning to get humans to Mars in the 2030s, and Elon Musk says he'll do it even earlier. But they plan to bring people back. If they can provide return trips, it seems a wasteful sacrifice to die on Mars when they don't have to. Couldn't successful colonists contribute a lot to humanity if they were to return to Earth after their successful missions?



Mars One seems to gloss over a lot of problems. Here's some more from their website:

A new group of four astronauts will land on Mars every two years, steadily increasing the settlement’s size. Eventually, a living unit will be built from local materials, large enough to grow trees.



As more astronauts arrive, the creativity applied to settlement expansion will certainly give way to ideas and innovation that cannot be conceived now. But it can be expected that the human spirit will continue to persevere, and even thrive in this challenging environment.

"A living unit will be built from local materials, large enough to grow trees." A simple sentence, which obscures so much complexity. Will they mine and refine iron ore? What do they have in mind?



I don't want to be a Debbie Downer about it. I love the spirit behind the whole thing. But it takes so much rigorous planning and execution to establish a colony on Mars. And money. How will it all work?



In the end, the whole thing is a long shot. Mars One says they have visited and talked to engineering and technological suppliers globally, and that their timeline and planning is based on this feedback. For example, they say they intend to use a Falcon Heavy rocket from SpaceX to launch their ship. But so much detail is left out. The Falcon Heavy doesn't even exist yet, and Mars One has no control or input into the rocket's development.







Take a look at the two sentences describing how they will communicate with Earth:

"The communications system will consist of two communications satellites and Earth ground stations. It will transmit data from Mars to Earth and back."

Does this type of brevity inspire confidence?



For at least 200,000 people, the answer is "yes."





The post These are the 40 Who Might Die on Mars appeared first on Universe Today.

ALIENS MESSAGES - Crop Circles - Hyperspace Gateways - Feature Length

MESSAGES FROM ALIENS - Undeniable Evidence - The Message (Colin Andrews) {1998}

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MILKY WAY - Metropolitan Milky Way

Metropolitan Milky Way:

This article was written by contributing author Janik Alheit, and is used by permission from the original at PhotographingSpace.com.

When it comes to my style of photography, preparation is a key element in getting the shot I want.

On this specific day, we were actually planning on only shooting the low Atlantic clouds coming into the city of Cape Town. This in itself takes a lot of preparation as we had to keep a close eye on the weather forecasts for weeks using Yr.no, and the conditions are still unpredictable at best even with the latest weather forecasting technology.



We set out with cameras and camping gear with the purpose of setting up camp high up on Table Mountain so as to get a clear view over the city. The hike is extremely challenging at night, especially with a 15kg backpack on your back! We reached our campsite at about 11pm, and then started setting up our cameras for the low clouds predicted to move into the city at about 3am the next morning. For the next 2 hours or so we scouted for the best locations and compositions, and then tried to get a few hours of sleep in before the clouds arrived.



At about 3am I was woken up by fellow photographer Brendon Wainwright. I realised that he had been up all night shooting timelapses, and getting pretty impressive astro shots even though we were in the middle of the city. I noticed that the clouds had rolled in a bit earlier than predicted and had created a thick blanket over the city, which was acting as a natural light pollution filter.



I looked up at the skies and for the first time in my life I was able to see the core of the Milky Way in the middle of the city! This is when everything changed, the mission immediately became an astrophotography mission, as these kind of conditions are extremely rare in the city.

Composition

After shooting the city and clouds for a while, I turned my focus to the Milky Way. I knew I was only going to have this one opportunity to capture an arching Milky Way over a city covered with clouds, so I had to work fast to get the perfect composition before the clouds changed or faded away.



I set my tripod on top of a large rock that gave me a bit of extra height so that I could get as much of the city lights in the shot as possible. The idea I had in my mind was to shoot a panorama from the center of the city to the Twelve Apostles Mountains in the southwest. This was a pretty large area to cover, plus the Milky Way was pretty much straight above us which meant I had to shoot a massive field of view in order to get both the city and the Milky Way.



The final hurdle was to get myself into the shot, which meant that I had to stand on a 200m high sheer cliff edge! Luckily this was only necessary for one frame in the entire panorama.

Gear and settings

I usually shoot with a Canon 70D with an 18mm f/3.5 lens and a Hahnel Triad 40Lite tripod. This particular night I forgot to bring a spare battery for my Canon and by the time I wanted to shoot this photo, my one battery had already died!



Luckily I had a backup camera with me, an Olympus OMD EM10 mirrorless camera. I had no choice but to use this camera for the shot. The lens on that camera was an Olympus M.Zuiko 14-42mm f/3.5 kit lens, which was not ideal, but I just had to make it work.



I think this photo is a testament to the fact that your gear is not nearly as important as your technique and knowledge of your surroundings and your camera.



I started off by shooting the first horizontal line of photos, in landscape orientation, to form the bottom edge of the final stitched photo. From there I ended up shooting 6 rows of 7 photos each in order to capture the whole view I wanted. This gave me 42 photos in total.



For the most part, my settings were 25 seconds, f/3.5, ISO 2000, with the ISO dropped on a few of the pictures where the city light was too bright. I shot all the photos in raw as to get as much data out of each frame as possible.

Editing

Astrophotography is all about the editing techniques.



In this scenario I had to stitch 42 photos into one photo. Normally I would just use the built-in function in Lightroom, but in this case I had to use software called PTGui Pro, which is made for stitching difficult panoramas. This software enables me to choose control points on the overlapping images in order to line up the photos perfectly.



After creating the panorama in PTGui Pro, I exported it as a TIFF file and then imported that file into Lightroom again. Keep in mind that this one file is now 3GB as it is made up of 42 RAW files!



In Lightroom I went through my normal workflow to bring out the detail in the Milky Way by boosting the highlights a bit, adding contrast, a bit of clarity, and bringing out some shadows in the landscape. The most difficult part was to clear up the distortion that was caused by the faint clouds in the sky between individual images. Unfortunately it is almost impossible to blend so many images together perfectly when you have faint clouds in the sky that form and disappear within minutes, but I think I did the best job I could to even out the bad areas.

A special event

After the final touches were made and the photo was complete, I realized that I had captured something really unique. It's not every day that you see low clouds hanging over the city, and you almost never see the Milky Way so bright above the city, and I managed to capture both in one image!



The response to the image after posting it to my Instagram account was extremely overwhelming. I got people from all over the world wanting to purchase the image and it got shared hundreds of time across all social media.



It just shows you that planning and dedication does pay off!

The post Metropolitan Milky Way appeared first on Universe Today.

DISCOVER THE COSMOS - The Supernova and Cepheids of Spiral Galaxy UGC 9391

The Supernova and Cepheids of Spiral Galaxy UGC 9391:

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

2016 June 6

The Supernova and Cepheids of Spiral Galaxy UGC 9391

Image Credit: NASA, ESA, and A. Riess (STScI/JHU) et al.


Explanation: What can this galaxy tell us about the expansion rate of the universe? Perhaps a lot because UGC 9391, featured, not only contains Cepheid variable stars (red circles) but also a recent Type Ia supernova (blue X). Both types of objects have standard brightnesses, with Cepheids typically being seen relatively nearby, while supernovas are seen much farther away. Therefore, this spiral is important because it allows a calibration between the near and distant parts of our universe. Unexpectedly, a recent analysis of new Hubble data from UGC 9391 and several similar galaxies has bolstered previous indications that Cepheids and supernovas are expanding with the universe slightly faster than expected from expansion measurements of the early universe. Given the multiple successes of early universe concordance cosmology, astrophysicists are now vigorously speculating about possible reasons for this discrepancy. Candidate explanations range from the sensational, such as the inclusion of unusual cosmological components types such as phantom energy and dark radiation, to the mundane, including statistical flukes and underestimated sources of systematic errors. Numerous future observations are being planned to help resolve the conundrum.

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Tomorrow's picture: news from venus

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DISCOVER THE COSMOS - Inside a Daya Bay Antineutrino Detector

Inside a Daya Bay Antineutrino Detector:

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

2016 May 23

Inside a Daya Bay Antineutrino Detector

Image Credit & Copyright: DOE, Berkeley Lab - Roy Kaltschmidt, photographer


Explanation: Why is there more matter than antimatter in the Universe? To better understand this facet of basic physics, energy departments in China and the USA led in the creation of the Daya Bay Reactor Neutrino Experiment. Located under thick rock about 50 kilometers northeast of Hong Kong, China, eight Daya Bay detectors monitor antineutrinos emitted by six nearby nuclear reactors. Featured here, a camera looks along one of the Daya Bay detectors, imaging photon sensors that pick up faint light emitted by antineutrinos interacting with fluids in the detector. Early results indicate an unexpectedly high rate of one type of antineutrino changing into another, a rate which, if confirmed, could imply the existence of a previously undetected type of neutrino as well as impact humanity's comprehension of fundamental particle reactions that occurred within the first few seconds of the Big Bang.

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Tomorrow's picture: diagonal peaks

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SATURN RING - Up and Over

Up and Over: Cassini orbited in Saturn's ring plane -- around the planet's equator -- for most of 2015.

Original enclosures:

FANTASTIC UNIVERSE - Comet PanSTARRS and the Helix Nebula

Comet PanSTARRS and the Helix Nebula:

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

2016 June 5

Comet PanSTARRS and the Helix Nebula

Image Credit & Copyright: Fritz Helmut Hemmerich


Explanation: It's rare that such different objects are imaged so close together. Such an occasion is occurring now, though, and was captured two days ago in combined parallel exposures from the Canary Islands of Spain. On the lower right, surrounded by a green coma and emanating an unusually split blue ion tail diagonally across the frame, is Comet C/2013 X1 (PanSTARRS). This giant snowball has been falling toward our Sun and brightening since its discovery in 2013. Although Comet PannSTARRS is a picturesque target for long-duration exposures of astrophotography, it is expected to be only barely visible to the unaided eye when it reaches its peak brightness in the next month. On the upper left, surrounded by red-glowing gas, is the also-picturesque Helix Nebula. At 700 light years distant, the Helix is not only much further away than the comet, but is expected to retain its appearance for thousands of years.

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HUBBLE TELESCOPE - The Hubble Constant Just Got Constantier

The Hubble Constant Just Got Constantier:

Just when we think we understand the Universe pretty well, along come some astronomers to upend everything. In this case, something essential to everything we know and see has been turned on its head: the expansion rate of the Universe itself, aka the Hubble Constant.



A team of astronomers using the Hubble telescope has determined that the rate of expansion is between five and nine percent faster than previously measured. The Hubble Constant is not some curiousity that can be shelved until the next advances in measurement. It is part and parcel of the very nature of everything in existence.



"This surprising finding may be an important clue to understanding those mysterious parts of the universe that make up 95 percent of everything and don't emit light, such as dark energy, dark matter, and dark radiation," said study leader and Nobel Laureate Adam Riess of the Space Telescope Science Institute and The Johns Hopkins University, both in Baltimore, Maryland.







But before we get into the consequences of this study, let's back up a bit and look at how the Hubble Constant is measured.



Measuring the expansion rate of the Universe is a tricky business. Using the image at the top, it works like this:

1. Within the Milky Way, the Hubble telescope is used to measure the distance to Cepheid variables, a type of pulsating star. Parallax is used to do this, and parallax is a basic tool of geometry, which is also used in surveying. Astronomers know what the true brightness of Cepheids are, so comparing that to their apparent brightness from Earth gives an accurate measurement of the distance between the star and us. Their rate of pulsation also fine tunes the distance calculation. Cepheid variables are sometimes called "cosmic yardsticks" for this reason.
2. Then astronomers turn their sights on other nearby galaxies which contain not only Cepheid variables, but also Type 1a supernova, another well-understood type of star. These supernovae, which are of course exploding stars, are another reliable yardstick for astronomers. The distance to these galaxies is obtained by using the Cepheids to measure the true brightness of the supernovae.
3. Next, astronomers point the Hubble at galaxies that are even further away. These ones are so distant, that any Cepheids in those galaxies cannot be seen. But Type 1a supernovae are so bright that they can be seen, even at these enormous distances. Then, astronomers compare the true and apparent brightnesses of the supernovae to measure out to the distance where the expansion of the Universe can be seen. The light from the distant supernovae is "red-shifted", or stretched, by the expansion of space. When the measured distance is compared with the red-shift of the light, it yields a measurement of the rate of the expansion of the Universe.
4. Take a deep breath and read all that again.

The great part of all of this is that we have an even more accurate measurement of the rate of expansion of the Universe. The uncertainty in the measurement is down to 2.4%. The challenging part is that this rate of expansion of the modern Universe doesn't jive with the measurement from the early Universe.



The rate of expansion of the early Universe is obtained from the left over radiation from the Big Bang. When that cosmic afterglow is measured by NASA’s Wilkinson Microwave Anisotropy Probe (WMAP) and the ESA's Planck satellite, it yields a smaller rate of expansion. So the two don't line up. It's like building a bridge, where construction starts at both ends and should line up by the time you get to the middle. (Caveat: I have no idea if bridges are built like that.)







"You start at two ends, and you expect to meet in the middle if all of your drawings are right and your measurements are right," Riess said. "But now the ends are not quite meeting in the middle and we want to know why."



"If we know the initial amounts of stuff in the universe, such as dark energy and dark matter, and we have the physics correct, then you can go from a measurement at the time shortly after the big bang and use that understanding to predict how fast the universe should be expanding today," said Riess. "However, if this discrepancy holds up, it appears we may not have the right understanding, and it changes how big the Hubble constant should be today."



Why it doesn't all add up is the fun, and maybe maddening, part of this.



What we call Dark Energy is the force that drives the expansion of the Universe. Is Dark Energy growing stronger? Or how about Dark Matter, which comprises most of the mass in the Universe. We know we don't know much about it. Maybe we know even less than that, and its nature is changing over time.



"We know so little about the dark parts of the universe, it's important to measure how they push and pull on space over cosmic history," said Lucas Macri of Texas A&M University in College Station, a key collaborator on the study.



The team is still working with the Hubble to reduce the uncertainty in measurements of the rate of expansion. Instruments like the James Webb Space Telescope and the European Extremely Large Telescope might help to refine the measurement even more, and help address this compelling issue.

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