Space News/UFO's Etc...(Discussion/Pics/Vids)

Breaking News: SpaceX Falcon 9 Rocket Explodes on Launch Pad in Florida
By Tariq Malik, Space.com Managing Editor | September 1, 2016 09:38am ET

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Black plumes of smoke billow over SpaceX's Falcon 9 rocket launch site at Space Launch Complex 40 at Cape Canaveral Air Force Station, Florida on Thursday, Sept. 1, 2016 . This image was captured by a NASA Kennedy Space Center webcam.
Credit: NASA Kennedy Space Center
A SpaceX Falcon 9 rocket appears to have exploded on its Florida launch pad early Thursday (Sept. 1), just days ahead of a planned weekend liftoff of a commercial satellite.

NASA webcam images of the SpaceX rocket's launch site - Space Launch Complex 40 at the Cape Canaveral Air Force Station - showed a massive plume of black smoke over the pad Thursday morning. Other photos on Twitter by witnesses showed more smoke and flames, though exact details on what went wrong with the Falcon 9 were not immediately available from SpaceX.

The rocket incident occurs as SpaceX was preparing to launch the Amos 6 communications satellite for the Israeli company Spacecom on Saturday, Sept. 3.
 
Tour September’s Sky: Mars, Saturn & Venus
By: Kelly Beatty | August 31, 2016

Early evening features Mars and Saturn toward south, but keep an eye out for brilliant Venus climbing up from the west during twilight.

In this month's astronomy podcast, you'll learn about September's equinox, which marks the celestial end of summer and the beginning of autumn in the Northern Hemisphere. This year it occurs on the 22nd at 10:21 a.m. Eastern Daylight Time. At that moment the Sun shines directly overhead as seen from the equator.

Another celestial event is associated with this equinox: the Harvest Moon. Traditionally, it’s the name assigned to the full Moon that falls closest to the autumnal equinox, and in 2016 it falls on the night of September 16th. The Harvest Moon gets this name because around that date it never really gets dark between sunset and moonrise for several successive evenings, a boon to farmers working late to harvest their crops.

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As September begins, look for a thin crescent Moon in the west after sunset. To its lower right, hugging the horizon, are Venus and Jupiter.
Sky & Telescope diagram

As darkness falls, look for the planets Mars and Saturn in the southwest. Over in the west, use the Moon's thin, rounded crescent on the 3rd or 4th to point to its lower right, very close to the horizon, to spot bright Venus glowing in the twilight. More challenging is finding Jupiter, to the lower right of Venus.

Meanwhile, look nearly overhead to spot the three widely-separated stars of the Summer Triangle. Vega is the one farthest west, Deneb is toward northeast, and Altair is farthest south. Watch week by week as this trio gradually migrates toward the western horizon.

For more skywatching tips — including how to find Draco, the Dragon, and the lovely Corona Borealis (Northern Crown) of stars — listen to or download our monthly astronomy podcast below.

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The weird, isolated mountain on Ceres is a giant ice volcano
Mika McKinnon, Astronomy.com | Published: Friday, September 02, 2016

Ceres: a world that just keeps getting weirder and weirder.

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NASA/JPL-Caltech/UCLA/MPS/DLR/IDA/PSI

Ever since we laid robotic eyes on the lone, giant mountain on Ceres, scientist have been obsessed with a single question: How did Ahuna Mons form? New models suggest the mountain is an icy volcano, adding on to the growing body of evidence that even small worlds can be geologically active.

When NASA’s Dawn spacecraft arrived in orbit around the dwarf planet Ceres in the main asteroid belt, it found a single lone mountain in its vast, cratered plains. Since then, scientists have puzzled over its origin. After running scenarios for every formation process they could dream up, they think they’ve found an answer.

With a single spacecraft in orbit and no rovers to poke and prod directly, researchers are dependent on remote sensing to collect data, then modeling scenarios to try to make that data into a coherent story. Scientists brainstormed every process we know about that can create mountains — volcanism, tectonic movement, even buoyant displacement — and tested models to see what fits our observations.

Cryovolcanoes are a unique feature to other planets in our solar system not found on Earth. These volcanoes erupt frozen slurry of salty ices instead of molten rock. They’re increasingly common in the outer solar system, famously caught erupting on Enceladus by the Saturn-orbiting Cassini spacecraft. Now it looks like they may also exist closer to the Sun.

When researchers modelled potential cryovolcanoes on Ceres, their hypothetical scenario looked similar to terrestrial volcanoes with high-viscosity magma. The peak of Ahuna Mons is riddled with fractures and tiny hills, consistent with thick, gooey material erupting, oozing in a messy spread until it cools and hardens. As it cools, the materials fractures and breaks into boulders, which tumble down the mountain to create a halo of debris. All aspects of this process common to terrestrial volcanoes with high-viscosity lava are also present on Ceres’ massive mountain, suggesting that that it formed the same way.

In order for the models to match observations, the mountain on Ceres must be quite young, and the product of a high-viscosity mix of ice and salt. But like everything else on Ceres, this is the start of a whole new round of questions. What does the interior structure of the dwarf planet look like, and how is heat involved in driving active surface processes? What salts are mixed into the ice, and how far from pure water is it? Can we find evidence of other cryovolcanic processes on Ceres, or is this mountain a unique outlier reflecting some yet-unknown localized oddity? And if we can find cryovolcanoes on dwarf planets in the main asteroid belt, where else are we going to find them?
 
Very true, asft... The image looks for all the world like an artist's rendition, but that is the real thing. It looks like what it is: an ice volcano. I guess maybe the ice slurry that erupts ends up coating the outside of the volcano.
 
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This Twitter lets you know what Hubble is staring at RIGHT NOW
Ryan F. Mandelbaum, Astronomy Magazine | Friday, September 2, 2016

Want to know what Hubble is up to right now? There's a tweet for that.

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NASA / ESA / HST

Space and science may capture the public imagination, but as laypeople we rarely get results before scientists decide to publish them. A new Twitter account lets you see the magic in action.

The account, @Hubble_Live, tweets where the Hubble Space telescope is looking… right now.

I am looking at the planet NEPTUNE for Dr. Mark R. Showalter using Wide Field Camera 3! [Address deleted - Ilan]
— Hubble Live (@Hubble_Live) September 2, 2016

Each tweet lists which scientist (or group of scientists) is using the Hubble with which specific instrument, and where the telescope is pointing and why, whether for observing or just calibrating. Some of the tweets even come with images, though the pictures aren’t actually Hubble images. Each tweet contains a link through to more information about the specific research.

The feed is run by the Space Telescope Science Institute (STScI)’s outreach site, HubbleSite.org. STSci is the operations center for the telescope’s science program.
 
Amazing Astronomy Facts
From astronomyforbeginners.com

  • When you look at the Andromeda galaxy (which is 2.3 million light years away), the light you are seeing took 2.3 million years to reach you. Thus you are seeing the galaxy as it was 2.3 million years ago.
  • Light from the sun takes 8 minutes to reach you, thus you see the sun as it was 8 minutes ago. It might have blown up 4 minutes ago and you wouldn't know about it!
  • The Earth is not a sphere! It actually is an oblate spheroid, it is squashed slightly at the poles and bulges out at the equator due to its rotation.
  • When Galileo viewed Saturn for the first time through a telescope, he described the planet as having "ears". It was not until 1655 that Christian Huygens suggested the crazy theory that they might be an enormous set of rings around the planet.
  • If you could put Saturn in an enormous bathtub, it would float. The planet is less dense than water.
  • A teaspoon-full of Neutron star would weigh about 112 million tons.
  • Jupiter is heavier than all the other planets put together.
  • Even on the clearest night, the human eye can only see about 3,000 stars. There are an estimated 100,000,000,000 in our galaxy alone!
  • The tallest mountain in the solar system is Olympus Mons, on Mars at a height of about 15 miles, three times the height of Mount Everest. It covers an area about half the size of Spain.
  • If the sun were the size of a dot on an ordinary-sized letter 'i', then the nearest star would be 10 miles away.
  • Half-a-billionth of the energy released by the sun reaches the Earth
  • Temperatures on Venus are hot enough to melt lead.
  • If you could travel at the speed of light (186,000 miles per second) it would take 100,000 years to cross our galaxy!
  • Only one side of the moon ever faces Earth. The moons period of rotation is exactly the same as it's period of orbit.
  • Betelgeuse, the bright star on Orion's top-left shoulder, is so big that if it was placed where the sun is, it would swallow up Earth, Mars and Jupiter!
  • If you stand on the equator, you are spinning at about 1,000 mph in as the Earth turns, as well as charging along at 67,000 mph round the sun.
  • On the equator you are about 3% lighter than at the poles, due to the centrigual force of the Earth spinning.
  • The atmosphere on Earth is proportionately thinner than the skin on an apple.
  • On Mercury a day (the time it takes for it to spin round once) is 59 Earth-days. Its year (the time it takes to orbit the sun) is 88 days- that means there are fewer than 2 days in a year!
  • If a piece of the sun the size of a pinhead were to be placed on Earth, you could not safely stand within 90 miles of it!
  • Its estimated that the number of stars in the universe is greater than the number of grains of sand on all the beaches in the world! On a clear night, we can see the equivalent of a handful of sand.
  • Every year the sun evaporates 100,000 cubic miles of water from Earth (that weighs 400 trillion tonnes!)
  • Jupiter acts as a huge vacuum cleaner, attracting and absorbing comets and meteors. Some estimates say that without Jupiters gravitational influence the number of massive projectiles hitting Earth would be 10,000 times greater.
  • Astronomers believe that space is not a complete vacuum - there are three atoms per cubic meter.
  • Saturn is not the only planet with rings - Neptune has it's own ring system.
 
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Best Picture Yet Of Milky Way’s Formation 13.5 Billion Years Ago
Evan Gough, UniverseToday | Article Updated: 8 Sep , 2016

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The Milky Way is like NGC 4594 (pictured), a disc shaped spiral galaxy with around 200 billion stars. The three main features are the central bulge, the disk, and the halo. Credit: ESO
Maybe we take our beloved Milky Way galaxy for granted. As far as humanity is concerned, it’s always been here. But how did it form? What is its history?

Our Milky Way galaxy has three recognized stellar components. They are the central bulge, the disk , and the halo. How these three were formed and how they evolved are prominent, fundamental questions in astronomy. Now, a team of researchers have used the unique property of a certain type of star to help answer these fundamental questions.

The type of star in question is called the blue horizontal-branch star (BHB star), and it produces different colors depending on its age. It’s the only type of star to do that. The researchers, from the University of Notre Dame, used this property of BHB’s to create a detailed chronographic (time) map of the Milky Way’s formation.

This map has confirmed what theories and models have predicted for some time: the Milky Way galaxy formed through mergers and accretions of small haloes of gas and dust. Furthermore, the oldest stars in our galaxy are at the center, and younger stars and galaxies joined the Milky Way over billions of years, drawn in by the galaxy’s growing gravitational pull.

The team who produced this study includes astrophysicist Daniela Carollo, research assistant professor in the Department of Physics at the University of Notre Dame, and Timothy Beers, Notre Dame Chair of Astrophysics. Research assistant professor Vinicius Placco, and other colleagues rounded out the team.

“We haven’t previously known much about the age of the most ancient component of the Milky Way, which is the Halo System,” Carollo said. “But now we have demonstrated conclusively for the first time that ancient stars are in the center of the galaxy and the younger stars are found at longer distances. This is another piece of information that we can use to understand the assembly process of the galaxy, and how galaxies in general formed.”

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This dazzling infrared image from NASA’s Spitzer Space Telescope shows hundreds of thousands of stars crowded into the swirling core of our spiral Milky Way galaxy. Credit: NASA/JPL-Caltech
This dazzling infrared image from NASA’s Spitzer Space Telescope shows hundreds of thousands of stars crowded into the swirling core of our spiral Milky Way galaxy. Credit: NASA/JPL-Caltech

The Sloan Digital Sky Survey (SDSS) played a key role in these findings. The team used data from the SDSS to identify over 130,000 BHB’s. Since these stars literally “show their age”, mapping them throughout the Milky Way produced a chronographic map which clearly shows the oldest stars near the center of the galaxy, and youngest stars further away.

“The colors, when the stars are at that stage of their evolution, are directly related to the amount of time that star has been alive, so we can estimate the age,” Beers said. “Once you have a map, then you can determine which stars came in first and the ages of those portions of the galaxy. We can now actually visualize how our galaxy was built up and inspect the stellar debris from some of the other small galaxies being destroyed by their interaction with ours during its assembly.”

Astronomers infer, from various data-driven approaches, that different structural parts of the galaxy have different ages. They’ve assigned ages to different parts of the galaxy, like the bulge. That makes sense, since everything can’t be the same age. Not in a galaxy that’s this old. But this map makes it even clearer.

As the authors say in their paper, “What has been missing, until only recently, is the ability to assign ages to individual stellar populations, so that the full chemo-dynamical history of the Milky Way can be assessed.”

This new map, with over 130,000 stars as data points, is a pretty important step in understanding the evolution of the Milky Way. It takes something that was based more on models and theory, however sound they were, and reinforces it with more constrained data.
 
Newly Discovered Asteroid Has a Close Encounter with Earth
Nancy Atkinson, UniverseToday.com | Article Updated: 7 Sep , 2016

Quite a bit closer than I had thought. - Ilan

As NASA prepares to send a spacecraft to a distant asteroid, another space rock made a surprise visit to Earth’s vicinity. The newly discovered small asteroid, named 2016 RB1, passed safely by Earth, coming within approximately 23,900 miles (38,463 km) of our planet, or just outside the orbit of many communications satellites.

The asteroid passed by Earth at 1:28 p.m. Eastern Time (1728 UT).

2016rb1_anim_06sept2016.gif

Credit: Gianluca Masi/Virtual Telescope Project.

The asteroid was discovered on Monday, September 5 by the Mt. Lemmon Survey telescope in Tucson, Arizona. 2016 RB1 is estimated to be between 24 to 52 feet (7.3 – 16 meters) across, which is just a bit smaller than the Chelyabinsk meteor that exploded over northern Russian in February 2013, which was estimated to be around 56 ft (17 meters) wide.

On Thursday, September 8, NASA hopes to launch its OSIRIS ReX mission to study asteroid Bennu and conduct a sample return, with the sample coming back to Earth by 2023. With the mission, scientists hope to learn more about the formation and evolution of asteroids and of the Solar System as a whole.

Here’s a graphic comparing the small asteroid 2016 RB1 to other objects, compiled by Mikko Tuomela and Massimo Orgiazzi.

CrvjgS9WYAADyBw.jpg-large-580x435.jpg

Objects on Earth and in space compared to the newly found asteroid
2016 RB1 (center of graphic). Compiled by Mikko Tuomela and
Massimo Orgiazzi. Used by permission.


A few observers were able to track the asteroid, including Gianluac Masi of the Virtual Telescope project, and Ernesto Guido of the Remanzacco Observatory.

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An image of 2016 RB1 taken on September 7, 2016, remotely
from the Q62 iTelescope network (Siding Spring, Australia).
Credit: Ernesto Guido.


2016 RB1 is the third asteroid so far in September 2016 that traveled between the Earth and the Moon. Asteroid 2016 RR1 passed by at 0.32 lunar distances on September 2, and just a few hours later, asteroid 2016 RS1 passed by at 0.48 times the Earth-moon distance. But this latest asteroid pass is the closest, at 0.10 lunar distances.

From its orbit, astronomers have determined 2016 RB1 is likely an Aten asteroid, a group of Near-Earth Objects that cross the orbits of Earth, Venus and even Mercury.
 
Newly Discovered Asteroid Has a Close Encounter with Earth
Nancy Atkinson, UniverseToday.com | Article Updated: 7 Sep , 2016

Quite a bit closer than I had thought. - Ilan

As NASA prepares to send a spacecraft to a distant asteroid, another space rock made a surprise visit to Earth’s vicinity. The newly discovered small asteroid, named 2016 RB1, passed safely by Earth, coming within approximately 23,900 miles (38,463 km) of our planet, or just outside the orbit of many communications satellites.

The asteroid passed by Earth at 1:28 p.m. Eastern Time (1728 UT).

2016rb1_anim_06sept2016.gif

Credit: Gianluca Masi/Virtual Telescope Project.

The asteroid was discovered on Monday, September 5 by the Mt. Lemmon Survey telescope in Tucson, Arizona. 2016 RB1 is estimated to be between 24 to 52 feet (7.3 – 16 meters) across, which is just a bit smaller than the Chelyabinsk meteor that exploded over northern Russian in February 2013, which was estimated to be around 56 ft (17 meters) wide.

On Thursday, September 8, NASA hopes to launch its OSIRIS ReX mission to study asteroid Bennu and conduct a sample return, with the sample coming back to Earth by 2023. With the mission, scientists hope to learn more about the formation and evolution of asteroids and of the Solar System as a whole.

Here’s a graphic comparing the small asteroid 2016 RB1 to other objects, compiled by Mikko Tuomela and Massimo Orgiazzi.

CrvjgS9WYAADyBw.jpg-large-580x435.jpg

Objects on Earth and in space compared to the newly found asteroid
2016 RB1 (center of graphic). Compiled by Mikko Tuomela and
Massimo Orgiazzi. Used by permission.


A few observers were able to track the asteroid, including Gianluac Masi of the Virtual Telescope project, and Ernesto Guido of the Remanzacco Observatory.

2016_RB1_07_Sep_2016_Q62-467x580.jpg

An image of 2016 RB1 taken on September 7, 2016, remotely
from the Q62 iTelescope network (Siding Spring, Australia).
Credit: Ernesto Guido.


2016 RB1 is the third asteroid so far in September 2016 that traveled between the Earth and the Moon. Asteroid 2016 RR1 passed by at 0.32 lunar distances on September 2, and just a few hours later, asteroid 2016 RS1 passed by at 0.48 times the Earth-moon distance. But this latest asteroid pass is the closest, at 0.10 lunar distances.

From its orbit, astronomers have determined 2016 RB1 is likely an Aten asteroid, a group of Near-Earth Objects that cross the orbits of Earth, Venus and even Mercury.

We are not alone
 
NGC 6101: Star Cluster with Hundreds of Black Holes?
Sep 9, 2016 by SciNews Staff | Sep 9, 2016

Computer simulations of a globular cluster called NGC 6101 reveal that it contains several hundreds of stellar-mass black holes, until now thought impossible.

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This Hubble image shows the globular cluster NGC 6101. Globular clusters are spherical collections of old stars (10-13 billion years old) which orbit around a galactic center. Image credit: NASA / ESA.
NGC 6101 is a globular star cluster in the constellation Apus. It is located at a distance of about 47,600 light-years from the Sun and about 36,500 light-years from the Galactic center.

Also known as Dun 68, GCL 40 and ESO 69-SC4, this grouping of stars was discovered on June 1, 1826 by the Scottish astronomer James Dunlop.

Using advanced computer simulations, astronomers at the University of Surrey, UK, were able to see the un-seeable by mapping NGC 6101, from which the existence of black holes within the system was deduced.

These black holes are a few times larger than the Sun, and form in the gravitational collapse of massive stars at the end of their lives.

It was previously thought that these black holes would almost all be expelled from their parent cluster due to the effects of supernova explosion.

“Due to their nature, black holes are impossible to see with a telescope, because no photons can escape”, said Dr. Miklos Peuten, a researcher in the Department of Physics at the University of Surrey and the lead author on a paper published in the Monthly Notices of the Royal Astronomical Society (arXiv.org preprint).

“In order to find them we look for their gravitational effect on their surroundings. Using observations and simulations we are able to spot the distinctive clues to their whereabouts and therefore effectively ‘see’ the un-seeable.”

In 2013, astronomers found individual black holes in globular clusters via rare phenomena in which a companion star donates material to the black hole.

The current study has shown that in NGC 6101 there could be several hundred black holes, overturning old theories as to how black holes form.

“Our work is intended to help answer fundamental questions related to dynamics of stars and black holes, and the recently observed gravitational waves,” said co-author Prof. Mark Gieles.

“These are emitted when two black holes merge, and if our interpretation is right, the cores of some globular clusters may be where black hole mergers take place.”

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The scientists chose to map NGC 6101 due to its recently found distinctive makeup, which suggested that it could be different to other clusters.

Compared to other globular clusters this one appears dynamically young in contrast to the ages of the individual stars.

Also NGC 6101 appears inflated, with the core being under-populated by observable stars.

Using computer simulation, the astronomers recreated every individual star and black hole in the cluster and their behavior.

Over the whole lifetime of 13 billion years the simulation demonstrated how NGC 6101 has evolved.

It was possible to see the effects of large numbers of black holes on the visible stars, and to reproduce what was observed for NGC6101.

From this, the team showed that the unexplainable dynamical apparent youth is an effect of the large black hole population.
 
Astronomers unveil most detailed map of the Milky Way to date
Hannah Devlin, The Guardian | 14 September 2016 9:54 EDT


The map, based on observations from the European Space Agency’s Gaia probe, will transform what we know about the galaxy, say scientists

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To see the video of the European Space Agency's release of a highly detailed map of the Milky Way
Please see URL in CODE at bottom


Astronomers have unveiled the most detailed map to date of the Milky Way, after charting the positions of more than 1bn stars with stunning precision.

The map, based on observations from the European Space Agency’s Gaia probe, still only represents about 1% of the Milky Way’s stars, but is already 20 times more complete than any previous observations of the night sky.

Speaking at a briefing in London on Wednesday, Gerry Gilmore, the mission’s UK principle investigator, said that the mission was already transforming what we know about our home galaxy. “We don’t actually know what the Milky Way looks like,” he said. “It’s astonishingly difficult, when you’re inside something, to find out what it looks like.”

The robotic Gaia spacecraft, which launched in 2013, is fitted with a 1bn pixel camera – the largest ever in space – complete with more than 100 electronic detectors. The precision of the measurements is equivalent to measuring the width of your fingernail – but if you were in London and your finger was in Australia.

The observations have already hinted at scientific discoveries that may lie ahead - including the possibility that the Milky Way may contain more stars than the current estimate of 100bn.

Scientists originally calculated that Gaia would see about 1bn stars by the end of 2017, but this number has now been revised upwards.

Floor van Leeuwen, of the University of Cambridge, who manages Gaia’s data processing, said: “It looks very much like we underestimated the number of stars. We think we will see 2-2.5bn stars.”

However, he added that it is not obvious how this relates to the number of stars in the entire galaxy.

The camera has now made observations of the precise position and brightness of more than 1.1bn stars. Astronomers are steadily converting the data into a 3D map of the galaxy - in effect, a cosmic version of Google maps.

“Every mission to come will use this map,” said Gilmore, adding that it would also help direct ground telescopes towards objects of interest in the cosmos.

By scanning each star about 70 times, astronomers have also calculated the sideways motion of 2m stars, showing how they drift and “wobble” in the night sky. This motion information will be crucial to building up a picture of the mass distribution in the galaxy – in particular the nature of the halo of dark matter that scientists believe surrounds the visible disk of the galaxy.

“We don’t know how massive the dark matter halo is and we will know that very much more accurately,” said Gilmore. “Knowing the velocities of objects far out in the galaxy will help determine that. That will be a complete revolution.”

Gaia astronomers will also be able to spot which stars have planets, by observing the characteristic wobble of the star caused by the gravitational pull of its neighbouring planet. Scientists estimate that Gaia could identify around 70,000 new exo-planets – planets outside of our solar system – by the end of the mission, which would be a dramatic increase on the 3,500 already known, most of which were identified by Nasa’s Kepler spacecraft.

“For the first time, we’ll be able to look at the distribution of planets based on the position of parent stars,” said Gilmore. “That will be a huge step forward in understanding planetary formation.”

Alvaro Giménez, ESA’s Director of Science, said: “Today’s release gives us a first impression of the extraordinary data that await us and that will revolutionise our understanding of how stars are distributed and move across our galaxy.”

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Alien Megastructure In Space Theory Reignited
Source: UFO-Blogger

Three months ago, news broke that a giant "alien megastructure" could exist around a bizarre-looking star 1,500 light-years away.

The first signs of this space oddity came from NASA’s planet-hunting Kepler space telescope, which continually watched the star’s region of the sky between 2009 and 2013. Most planet-hosting stars show small, regular dips in light when their planets pass in front of them. But Tabby’s star dipped erratically throughout the four years, sometimes losing as much as 20 per cent of its brightness.

In September 2015, a team led by Tabetha Boyajian of Yale University, who lends the star its informal name, tried to make sense of this unusual signal. Ultimately they determined that dust from a large cloud of comets was the best explanation.

A month later, the star made headlines across the globe thanks to a paper by Jason Wright of Pennsylvania State University and his colleagues, who suggested that “alien megastructures”, such as satellites designed to collect light from the star, could be responsible for the signal.

alien_megastructures_orbiting_star.jpg


While the prospect of aliens was first launched by Penn State astronomer Jason Wright, almost everyone in the astronomy community agreed that the chances that this was the case were "very low."

Now, the latest investigations into this strange star by Louisiana State University astronomer Bradley Schaefer have reignited the alien theory, New Scientist reported.

Now Bradley Schaefer of Louisiana State University has discovered that the mystery goes even further. When Boyajian’s team studied the star, they looked at data from a Harvard University archive of digitally scanned photographic plates of the sky from the past century or so to see if the star had behaved unusually in the past, but found nothing.

Schaefer decided this unusual star deserved a second look. He averaged the data in five-year bins to look for slow, long-term trends, and found that the star faded by about 20 per cent between 1890 and 1989. “The basic effect is small and not obvious,” he says.

To confirm the fade was real, Schaefer went to Harvard to look at the original photographic plates and inspected them by eye for changes, a skill few astronomers possess these days. “Since no one uses photographic plates any more, it’s basically a lost art,” says Wright. “Schaefer is an expert at this stuff.”

Schaefer saw the same century-long dimming in his manual readings, and calculated that it would require 648,000 comets, each 200 kilometres wide, to have passed by the star – completely implausible, he says.

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What makes this most interesting to me is the fact that researchers were willing to include an alien-based source in their speculations. - Ilan
 
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