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The new telescopes are about to transform the hunt for alien life and our understanding of the universe

From strategic points, on Earth and in space, the next telescopes will depend on next-generation technologies in their attempts to answer some of the most important questions of scientists about dark matter, the expansion of the universe and extraterrestrial life.

Some will provide 100 times more information than today’s most powerful tools for observing the heavens.

The first of these telescopes, the highly anticipated James Webb Space Telescope from NASA , will be released in 2021, and then start scanning the atmospheres of distant worlds for clues about extraterrestrial life. Already in 2022, other new telescopes in space will take unprecedented observations of the heavens, while observatories on Earth look back to the ancient universe.

This is what is in process and what these new tools could reveal.

Since its launch in 1990, NASA’s Hubble Space Telescope has discovered new planets, revealed strange galaxies and provided new insights into the nature of black holes.

It also found that the universe is expanding faster than scientists imagined.

However, many questions remain to be answered. How has the universe evolved over time? Why can’t we see 95% of it? If there are aliens, where are they?

The next generation of telescopes – in space and on land – will try to fill these gaps in our knowledge.

First, NASA is building the James Webb Space Telescope (JWST) to observe the history of the universe.

It will study how the first stars and galaxies formed, how planets are born and where there could be life in the universe.

The next telescope is fully assembled and now faces a long testing process at the Northrop Grumman facility in California before its launch on March 30, 2021.

A 21-foot-wide beryllium mirror will help the James Webb telescope observe distant galaxies in detail and capture extremely weak signals within our own galaxy.

The farther you look into space, the more the telescope will look back in time, so it could even detect the first flashes of the Big Bang.

JWST will also observe in detail young and distant galaxies that we have never seen before.

Thanks to the new infrared technology, the telescope was able to provide an unprecedented view of the supermassive black hole in the center of the Milky Way.

These images could help answer questions about how the galaxy formed and its black hole.

“Do the black hole comes first and stars form around it? Do the stars come together and collide to form the black hole? These are questions we want to answer, ”said Jay Anderson, a JWST scientist, in an October press release.

JWST will also look for signs of alien life in the atmospheres of exoplanets (the term for planets outside our solar system) – but only those larger than Earth.

By measuring the intensity of the light from the stars that crosses the atmosphere of a planet, the telescope could calculate the composition of that atmosphere.

Scientists have already identified more than 4,000 exoplanets.

But so far, they have not been able to study most of the atmospheres of these planets to look for signs of life, also known as “biosignatures.”

If an exoplanet’s atmosphere contains methane and carbon dioxide, for example, those are clues that there could be life there. JWST will look for signals like that.

Earth’s atmosphere has a lot of oxygen because life has been producing it for billions of years. Oxygen is not stable enough to last a long time on its own, so it must be constantly produced to make it so abundant.

The combination of carbon dioxide and methane (as in Earth’s atmosphere) is even more revealing, especially if there is no carbon monoxide.

This is because carbon dioxide and methane would normally react with each other to produce new compounds. So if they exist separately, something is likely to produce them constantly. That something could be a volcano, but as far as we know, only one way of life could release that amount of methane without also shedding carbon monoxide.

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Space

Asteroid as big as the pyramids on its way and could zoom past Earth on Friday

An asteroid as big as the Egyptian pyramids is zooming towards Earth and will squeeze past us on Friday – if it doesn’t smash on to our home planet’s surface.

Named 2019 WR3, NASA expects the space rock to make a “close approach” to Earth later this week.

The space agency has classified the asteroid as a “near-Earth object (NEO)” which means its orbit brings it very close – in cosmic terms – to Earth.

The asteroid was first spotted late last week.

NASA has now observed the asteroid some 74 times to better get a sense of its size and trajectory.

WR3 is believed to have a diameter of between 76m to 170m.

It is expected that on December 6, the asteroid will pass within 5.44 million km of Earth at speeds of 27,036 km/hr.

The warning comes as the European Space Agency approves a $471 million mission called Hera to examine whether a rogue asteroid on its way to Earth could be deflected out of the way.

Working with NASA, the ESA will send a pair of spacecraft to a double-asteroid system called Didymos to examine the asteroids and send valuable data back home.

The larger asteroid Didymoon is about 800m across, orbited by a moon about 160m wide.

If an asteroid the size of Didymoon were to hammer into Earth, it would be devastating.

Patrick Michel, ESA’s lead scientist for Hera, said it was vital to keep an eye on it so we can take action if needed.

“The probability is low but the consequences are high,” Michel told Space.com.

“This is why it’s relevant to take care of it. Moreover, we have the tools … We can’t lose more time.”

The Hera spacecraft will launch in 2024.

Meanwhile, Queens University Belfast professor Alan Fitzsimmons has called for amateur astronomers to assist the Hera mission’s broader goal of protecting Earth against asteroids by nominating asteroids to watch.

“We will get a serious asteroid impact sometime,” he told the BBC.

“It may not be in our lifetime, but mother nature controls when that will happen.

‘We will get a serious asteroid impact sometime.’

“We will need to do something about it. We’ll need to move that asteroid so it misses us and doesn’t hit us.

“Asteroid research is one area of astronomy where amateur observes continue to make an essential contribution,” he said.

Source 7news.com.au

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An ultralight source of x-rays detected, coming from the Draco constellation

ESA / Hubble

Intriguing ultralight source of X-rays, one of the brightest ever seen. It comes from a galaxy of the Draco constellation.

The ultraluminous X sources were discovered in 1980 with the Einstein space detector. The X-rays currently detected come from a galaxy located 14.8 million light years from Earth. This type of radiation has been quite mysterious to astronomers because it is extremely bright.

These astronomical systems ULEX, for its acronym in English, UltraLuminous X-ray source, have a brightness level of more than 10 raised to 39 erg per second (Ergis are units of measure of energy). The galaxy is called UGC 6456, and, interestingly, it is found in the constellation Draco (Dragon), a constellation object of legends and mythology.

X-ray source, UGC 6456 ULX

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Ultra-light X-ray sources. Credit: NASA

The study was conducted by Russian astronomers. These electromagnetic emissions are less luminous than a galactic core, but shine more than any process of formation or evolution of stars.

The group of astronomers is led by Alexander Vinokurov, from the Special Astrophysical Observatory, located in Nizhnij Arkhyz, Russia. The study presented says:

We present preliminary results of a study of the ultra-bright X-ray source UGC 6456 ULX. (…) To identify an optical counterpart of UGC 6456 ULX, we use archive images of the Chandra X-Ray Observatory and HST.

Note: HST stands for the Hubble Space Telescope.

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Overlay of images B, V and Rc of the UGC 6456 galaxy. The box shows the HST WFPC2 / F555W image of the region around the UGC 6456 ULX source, marked by the square; the circle indicates the 0.8 inch error box, derived from the Chandra Observatory data. Credit: Vinokurov et al.

The UGC 6456 galaxy is listed as a compact blue dwarf galaxy and is one of the closest to our Milky Way. Its UGC 6456 ULX source, or ultralight X-ray source, has mysterious properties, which they had not been studied in detail.

Among the brightest ever observed

The emissions of UGC 6456 ULX have brightness changes of more than two orders of magnitude with a maximum value of 17 erg duodecillions per second in the energy range of 0.3–8 keV (electron volts).

A duodecillón is a very long numerical scale equivalent to a 10 followed by 72 zeros! An electron volt is a unit of measurement that represents the energy per motion that an electron experiences.

Map of the constellation Draco "width =" 451 "height =" 500 "srcset ="
Map of the constellation Draco. Credit: Torsten Bronger / Wikimedia commons.

The magnitude of this source in its bright state is exceeded by an amount of -7.6. That makes her one of the ultraluminous sources of X-rays brightest ever discovered in the optical range.

The study presents a correlation between X-ray flows and optical (observable) flows in UGC 6456 ULX. This could indicate that the emission of optical light is produced by the X-ray re-processing in the outer parts of the so-called «Optically thick wind».

Ultra-light X-ray font "width =" 720 "height =" 488 "srcset =" https://www.soulask.com/wp-content/uploads/2019/12/1575347443_138_They-detect-an-ultralight-source-of-x-rays-that-comes-from.jpg 720w
Illustration of the phenomenon. Credit: NASA

The detection of many hydrogen and helium emission lines could relate to the wind that emerges from the powerful and dynamic accretion disk. This disk is a structure full of powder and cosmic gas that forms around a central object.

More details are expected with the following observations of this ultra-light source of X-rays. The light and energy changes of this system are similar to that of another known source, the so-called NGC 7793 P13, which has a neutron star.

The scientific study has been published on the pre-print website arXiv.org.

References: phys.org.

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The universe can be a giant loop, evidence suggests

New evidence suggests that, instead of being flat like a leaf, the universe can actually spin on itself.

What would happen if you could go drive with your spaceship faster than light and walked away in a perfectly straight line, never slowing down and never changing direction? Would you reach the edge of the universe or end up just where you started?

The idea that the universe is curved and curves over itself has existed for a while, however, it is a theory that is not really compatible with conventional ideas about how the universe works.

Now, however, a new document has ruined the idea of ​​a curved universe, since it suggests that there may be something in the idea of ​​a curved universe after all.

The study, which is based on the research of an international team of physicists, re-examines the data of the cosmic microwave background radiation (CMB), a remnant of the birth of our universe.

The key is in the discovery of an anomaly that suggests that there are significantly more “gravitational lenses” of the CMB than expected – more than can be explained by conventional physics.

According to the team’s findings, if the universe is really curved, then the curvature is very smooth, which means that on a planetary scale or even on a galactic scale it is unlikely that we will really notice.

universe-cosmic-microwave-background-cmb-big-bang

The cosmic microwave background is the faint echo of the Big Bang (Image: ESA/Max Planck Institute)

On a cosmic scale, however, this curvature becomes increasingly frequent until someone who moves through the entire universe in a straight line finally ends just where it began.

However, there is a long way to go to prove once and for all that this is really the case.

“I don’t want to say that I believe in a closed universe,” said study co-author Alessandro Melchiorri. “I am a little more neutral. I would say wait for the data and what the new data will say. ”

“What I think is that there is a discrepancy now, that we have to be careful and try to find what is producing this discrepancy.”

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