Traveling Across the Tarantula Nebula on a Runaway Star

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This image of the 30 Doradus nebula, a rambunctious stellar nursery, and the enlarged inset photo show a heavyweight star that may have been kicked out of its home by a pair of heftier siblings. In the inset image at right, an arrow points to the stellar runaway and a dashed arrow to its presumed direction of motion. The image was taken by the Wide Field and Planetary Camera 2 (WFPC2) aboard NASA’s Hubble Space Telescope. The heavyweight star, called 30 Dor #016, is 90 times more massive than the Sun and is traveling at more than 250,000 miles an hour. In the wider view of 30 Doradus, the homeless star, located on the outskirts of the nebula, is centered within a white box. The box shows Hubble’s field of view. The image was taken by the European Southern Observatory’s (ESO) Wide Field Imager at the 2.2-meter telescope on La Silla, Chile. Credits: NASA/ESA/Hubble

Traveling at 250,000 mph would be a windy, visually spectacular ride to hell 

Space news (Astrophysics: stellar nursery dynamics; runaway stars) – 170,000 light-years from Earth, near the edge of the Tarantula Nebula – 

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Hubble/WFPC2 and ESO/2.2-m Composite Image of 30 Dor Runaway Star. Credits: NASA/ESA/Hubble

If you want to travel through the galaxy, hitch a ride on a runaway star like the one astronomers have been tracking since it came screaming out of 30 Doradus (Tarantula Nebula) in 2006. Data collected by the newly installed Cosmic Origins Spectrograph on the Hubble Space Telescope suggests a massive star, as much as 90 times the mass of Sol, was knocked out of the nebula by gravitational interactions with even more massive suns. Traveling at around 250,000 mph, voyaging through the cosmos on this runaway star would be an adventure to write home about.  

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ESO 2.2-m WFI Image of the Tarantula Nebula. Credits: NASA/ESA/Hubble

The trail leads back to a star-forming region deep within the Tarantula Nebula called R136, where over 2,400 massive stars near the center of this huge nebula produce an intense wind of radiation. Astronomers think interactions with some of the 100 plus solar mass stars detected in this stellar nursery resulted in this runaway star being flung over 375 light-years by its bigger siblings.  

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Massive Star is Ejected from a Young Star Cluster. Credits: NASA/ESA/Hubble

These results are of great interest because such dynamical processes in very dense, massive clusters have been predicted theoretically for some time, but this is the first direct observation of the process in such a region,” says Nolan Walborn of the Space Telescope Science Institute in Baltimore and a member of the COS team that observed the misfit star. “Less massive runaway stars from the much smaller Orion Nebula Cluster were first found over half a century ago, but this is the first potential confirmation of more recent predictions applying to the most massive young clusters.”   

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Nolan Walborn. Credits: NASA/ESA/Hubble Heritage Site

Astrophysicists studying the runaway star and the region in the Tarantula region where the trail ended believe it’s likely a massive, blue-white sun at least ten times hotter than Sol and only a few million years old. It’s far from home and in a region of space where no clusters with similar stars are found. It’s also left an egg-shaped cavity in its wake with glowing edges pointing in the direction of the center of 30 Doradus and the region of R136. A flaming trail you would see behind the star as you traveled across the cosmos and onto eternity.  

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Compass/Scale Image of 30 Dor Runaway Star. Credits: NASA/ESA/Hubble

 “It is generally accepted, however, that R136 is sufficiently young, 1 million to 2 million years old, that the cluster’s most massive stars have not yet exploded as supernovae,” says COS team member Danny Lennon of the Space Telescope Science Institute. “This implies that the star must have been ejected through dynamical interaction.” 

This runway star continues to scream across the cosmos, nearing the outskirts of 30 Doradus a star-forming region in the Large Magellanic Cloud, it will one day end its existence in a titanic explosion or supernova, and possibly leave behind one of the most mysterious and enigmatic objects discovered during the human journey to the beginning of space and time, a black hole.  

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Hubble Observations of Massive Stars in the Large Magellanic Cloud. Credits: NASA/ESA/Hubble

Imagine riding this runaway star until it contracted into a black hole and left our universe altogether. Where would we travel? To a random location in spacetime? To another reality or universe? The possibilities abound and far exceed our ability to imagine such a reality. Scientists tell us such a journey wouldn’t be possible, but they’re just stumbling around in the dark looking for ideas to grasp. For handholds on the dark cliff we climb as we search for answers to the mysteries before us.  

What’s next?

Astronomers continue to study the Tarantula Nebula and the star-forming region R136 looking for signs of impending supernovae among the zoo of supermassive stars within. They also continue to track this runaway star and two other blue hot, supermassive stars outside the boundary of 30 Doradus that appear to have also been ejected from their host systems. We’ll update you with any news on it, and other runaway stars as it continues to scream across the cosmos. 

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Read and learn more about ancient navigators “The Incredible Polynesian Navigators Followed the Stars“.

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Read about astronomers observe the shock wave of a supernova in visible light for the first time.

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WISE & Spitzer Detect Faintest, Coolest Brown Dwarf Star to Date

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WISE J085510.83-071442.5 is the coolest, faintest brown dwarf star located and it’s also only 7.2 light-years away from Earth. Credits: NASA/ESA/Spitzer/WISE

A frosty, chilly star about the same temperature as the North Pole, minus 54 and 9 degrees Fahrenheit (minus 48 to minus 13 degrees Celsius)

Space news (astrophysics: faint, cool stars; brown dwarfs) – the fourth closest detected star system to Earth, just 7.2 light-years toward the constellation Hydra – 

A young, ambitious astronomer working at Pennsylvania State University’s Center for Exoplanets and Habitable Worlds discovered the dimmest, coolest brown dwarf detected during the human journey to the beginning of space and time. Kevin Lehman first noticed a fast moving object, quickly dubbed WISE J085510.83-071442.5, in March of 2013. Excited at a new discovery, he spent the next few days analyzing more images of the same part of the sky taken by NASA’s Spitzer Space Telescope and Gemini South Telescope on Cerro Pachon in Chile.

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Welcome to the Sun’s Neighborhood This diagram illustrates the locations of the star systems closest to the sun. The year when the distance to each system was determined is listed after the system’s name. NASA’s Wide-field Infrared Survey Explorer, or WISE, found two of the four closest systems: the binary brown dwarf WISE 1049-5319 and the brown dwarf WISE J085510.83-071442.5. NASA’s Spitzer Space Telescope helped pin down the location of the latter object. The closest system to the sun is a trio of stars that consists of Alpha Centauri, a close companion to it and the more distant companion Proxima Centauri. Image credit: Penn State University

“It’s very exciting to discover a new neighbor of our solar system that is so close,” said Kevin Luhman, an astronomer at Pennsylvania State University’s Center for Exoplanets and Habitable Worlds, University Park. “And given its extreme temperature, it should tell us a lot about the atmospheres of planets, which often have similarly cold temperatures.” 

Kevin Luhman originally spotted the fast motion of WISE J085510.83-071442.5 in infrared images taken by NASA’s Wide-field Infrared Survey Explorer (WISE). Later analysis of infrared images taken by NASA’s Spitzer Space Telescope were needed to determine its chilly temperature of between minus (54-9) Fahrenheit [minus (13 – 48) degrees Celsius]. Astronomers would use measurements taken by Spitzer and WISE at different positions around the sun to determine its distance of 7.2 light-years from Earth using the parallax effect. To scientists, it added up to a brown dwarf or maybe a large Jupiter-size planet lost in space. 

“This object appeared to move really fast in the WISE data,” said Luhman. “That told us it was something special.” 

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Cold and Quick: a Fast-Moving Brown Dwarf This animation shows the coldest brown dwarf yet seen, and the fourth closest system to our sun. Called WISE J085510.83-071442.5, this dim object was discovered through its rapid motion across the sky. It was first seen in two infrared images taken six months apart in 2010 by NASA’s Wide-field Infrared Survey Explorer, or WISE (see orange triangles). Two additional images of the object were taken with NASA’s Spitzer Space Telescope in 2013 and 2014 (green triangles). All four images were used to measure the distance to the object — 7.2 light-years — using the parallax effect. › See animation The Spitzer data were used to show that the body is as cold as the North Pole (or between minus 54 and 9 degrees Fahrenheit, which is minus 48 to minus 13 degrees Celsius). Image credit: NASA/JPL-Caltech/Penn State

Additional calculations estimated the mass of WISE J085510.83-071442.5 at between 3 and 10 times the mass of Jupiter. It could be a gas giant like Jupiter that was flung out of its host star system by gravitational interactions with more massive bodies. Astronomers determined it was more likely a very cool brown dwarf than a large gas giant planet since they have been detected more often. If this is the case, it’s the coldest brown dwarf star discovered during the human journey to the beginning of space and time. A nice shiny feather in the hat of a young, aspiring astronomer on the rise.  

“It is remarkable that even after many decades of studying the sky, we still do not have a complete inventory of the sun’s nearest neighbors,” said Michael Werner, the project scientist for Spitzer at NASA’s Jet Propulsion Laboratory in Pasadena, Calif. JPL manages and operates Spitzer. “This exciting new result demonstrates the power of exploring the universe using new tools, such as the infrared eyes of WISE and Spitzer.” 

Work’s never done

Never one to rest on his laurels, in March of 2013, Kevin Luhman discovered a pair of warmer brown dwarf stars just 6.5 light-years from Earth during his analysis of WISE images. Since this time, his search for rapidly moving bodies close to Earth has also shown that the outer solar system probably doesn’t contain a large, undiscovered planet X or Nemesis, as people often refer to it. I did mention he was ambitious. 

Learn more about WISE J085510.83-071442.5.

You can learn more about Kevin Luhman here

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Discover the work being done by Pennsylvania State University’s Center for Exoplanets and Habitable Worlds. 

Discover the Gemini South Telescope on Cerro Pachon in Chile. 

Read about a recent observation by the Kepler Space Telescope of a supernova shock wave in visible light.

Learn more about the incredible polynesian navigators and how they populated the islands of the Pacific Ocean.

Read about a supermassive black hole astronomers recently found residing in a galactic backwater.

Kepler Captures Supernova Shockwave in Visible Light

Mining of Kepler space mission data reveals “supernova’s shockwave” in visible light

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Space news (massive supernovae) – 1.2 billion light-years from Earth –

An international team of scientists at the University of Notre Dame in Indiana mining three years of Kepler Space Telescope data for massive supernovae discovered something never seen during the human journey to the beginning of space and time. Buried in the Kepler data Peter Garnavich and team observed for the first time the brilliant flash of a massive supernova’s shockwave in visible light as it reached the surface of the exploding star.

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NASA scientists Peter Garnavich. Credit: NASA

“In order to see something that happens on timescales of minutes, like a shock breakout, you want to have a camera continuously monitoring the sky,” said Garnavich. “You don’t know when a supernova is going to go off, and Kepler’s vigilance allowed us to be a witness as the explosion began.”

Garnavich’s the leader of the Kepler Extragalactic Survey (KEGS) research team, which is currently mining NASA’s Kepler K2 mission data looking for massive supernovae. NASA’s repurposed planet hunter is expected to detect around a dozen more events during its mission to capture the light from hundreds of distant galaxies and trillions of stars.

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The diagram illustrates the brightness of a supernova event relative to the sun as it unfolds. For the first time, a supernova shockwave has been observed in the optical wavelength or visible light as it reaches the surface of the star. This early flash of light is called a shock breakout. 

Astronomers call the brilliant flash of a supernova’s shockwave “a shock breakout”. This event only lasts around twenty minutes in the cases observed, so catching the flash as it happens is truly a milestone for astronomers studying supernovae. By piecing together individual moments of a supernova astronomers hope to learn more about the history of chemical complexity and the evolution of life.

“All heavy elements in the universe come from supernova explosions. For example, all the silver, nickel, and copper in the earth and even in our bodies came from the explosive death throes of stars,” said Steve Howell, project scientist for NASA’s Kepler and K2 missions at NASA’s Ames Research Center in California’s Silicon Valley. “Life exists because of supernovae.”

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NASA scientist Steve Howell. Credit: NASA

Massive supernovae and their less energetic brothers are the seeds of chemical complexity in the cosmos, spreading the elements of creation across the breadth of the universe. Understanding the physics behind these titanic events can help tell us how these elements of creation were spread across the universe.

Kepler observes two massive supernovae

The Kepler Space Telescope observed a type II supernova shockwave in visible light as it broke the surface of the star for the first time in history as supermassive red giant KSN 2011d went supernova in 2011. Containing roughly 500 times the mass of Sol, this supermassive star at the moment the shockwave from the supernova reached its surface was 130,000,000 times brighter than the Sun. Continuing to explode and grow, the star eventually reached a maximum brightness over 1 billion times greater than Sol 14 days later.

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This artist’s conception of the repurposed Kepler K2 spacecraft. Credit. NASA/Kepler K2

The Kepler Space Telescope also observed a second type II supernova in 2011. Red super massive star KSN 2011a contains 300 times as much mass as Sol and occupies a volume of space that would easily engulf the orbit of Earth around the Sun. Only 700 million light-years from Earth, astronomers weren’t able to observe a shock breakout in the data for this supernova, but they think it might be due to gas masking the shockwave as it reached the surface of the star.

“That is the puzzle of these results,” said Garnavich. “You look at two supernovae and see two different things. That’s maximum diversity.”

“While Kepler cracked the door open on observing the development of these spectacular events, K2 will push it wide open observing dozens more supernovae,” said Tom Barclay, senior research scientist and director of the Kepler and K2 guest observer office at Ames. “These results are a tantalizing preamble to what’s to come from K2!”

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Drawing of Tom Barclay. Credit: Tom Barclay.com

Watch this YouTube video on this event here.

Learn more about K2.

Discover what the Kepler Extragalactic Survey has told us here.

Take the voyage of the Kepler Space Telescope.

Learn more about type II supernovas here.

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Learn more about astronomy at the University of Notre Dame here.

Read about the giant bubble observed by the Hubble Space Telescope.

Learn more about the prominent emission lines in young stars.

Read about two merging black holes astronomers are watching.

The Human Journey to the Beginning of Space and Time is All-Systems-Go for Jupiter’s Moon Europa

Planetary scientists and exobiologists are planning a trip to determine if an ocean of water exists beneath its icy surface

Four hundred years ago, the astronomer Galileo's discovery of Jupiter's four large moons forever changed humanity's view of the universe, helping to bring about the understanding that Earth was not the center of all motion. Today one of these Galilean moons could again revolutionize science and our sense of place, for hidden beneath Europa's icy surface is perhaps the most promising place to look for present-day environments that are suitable for life.
Four hundred years ago, the astronomer Galileo’s discovery of Jupiter’s four large moons forever changed humanity’s view of the universe, helping to bring about the understanding that Earth was not the center of all motion. Today one of these Galilean moons could again revolutionize science and our sense of place, for hidden beneath Europa’s icy surface is perhaps the most promising place to look for present-day environments that are suitable for life. (Image courtesy of NASA)

Space news (July 15, 2015) – the search for life beyond Earth – With abundant water, a rocky substrate, and available heat energy due to tidal forces, Europa would be one of the best places in the solar system to search for signs of life.  

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John Grunsfeld, associate administrator for NASA’s Science Mission Directorate in Washington. Credit: NASA

Today we’re taking an exciting step from concept to a mission, in our quest to find signs of life beyond Earth,” said John Grunsfeld, associate administrator for NASA’s Science Mission Directorate in Washington. “Observations of Europa have provided us with tantalizing clues over the last two decades, and the time has come to seek answers to one of humanity’s most profound questions.”  

Artist concept of NASA's Europa mission spacecraft approaching its target for one of many flybys. Image credit: NASA/JPL-Caltech
Artist concept of NASA’s Europa mission spacecraft approaching its target for one of many flybys. Image credit: NASA/JPL-Caltech

NASA’s Europa Multiple Flyby Mission will conduct a detailed survey of the moon and its suitability for sustaining life. Estimates by planetary scientists indicate there could be as much as twice the volume of water as on Earth underneath the icy crust of this distant moon.  

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NASA astrobiologist Dr. Richard Hoover discovered this ancient moss still capable of growing and reproducing after 40,000 years beneath the Russian permafrost. Credit: (NASA/MSFC)

Could extremophiles – extreme forms of life found on Earth – exist on Europa? Some exobiologists think it could be possible forms of life found surviving and evolving in extreme environments on our planet could be tough enough. The existence of single-celled life forms in such environments would truly be a monumental point in human history.  

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NASA astrobiologist Dr. Richard Hoover retrieved this extremophile bacterium from ice dating to over 32,000 years ago. Credit: (NASA/MSFC)

Energy for living things to survive, prosper and evolve could be extracted from the environment if heat energy produced by tidal flexing of the crust of Europa is sufficient to drive chemical reactions. Chemical reactions that could recycle elements, making them available for use by living things in the battle to survive and evolve.  

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One of the oldest lifeforms still existing on the Earth, a tardigrade or “water bear” is seen through an electron microscope. Less than 1 mm in length, these hardy creatures can withstand the rigors of space travel for extended periods. They’re currently being studied to see just how tough they’re. Credit: ESA/Dr. Ralph O. Schill

Could there be life existing in the oceans of Europa? The known requirements for the existence of life, extraterrestrial or Earth-based, are still pretty basic at this point and they’ll change as we discover and learn more about what life really needs to survive, prosper and evolve.  

Cutaway diagram of Europa's interior. Artwork credit: Michael Carroll
Cutaway diagram of Europa’s interior. Artwork credit: Michael Carroll

We have waited patiently since NASA’s Galileo spacecraft first showed us oceans of water could exist beneath the icy surface of Europa. Sometime in the 2020s mankind will launch the Europa Multiple Flyby Mission to this distant moon of Jupiter in a desire to take a look.  

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The Galileo spacecraft being deployed from the cargo bay of STS-34 Atlantis at 7:15 p.m. EDT on 18th October 1989. Credit: NASA/JPL

All systems go for Europa

The trip to Europa is expected to launch from Cape Canaveral and take about 6.5 years, with gravity-assist from flybys of Venus and Earth, before arriving in the Jupiter system sometime in 2026 or 2027.  

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The Europa Orbiter above the surface of Europa, with Jupiter in the background. Credit: NASA/JPL

The mission calls for a spacecraft to flyby Europa 45 times, conducting a detailed survey and analysis of the icy surface of the moon in high-resolution images. In order to give planetary scientists more information on its composition and the environment and structure of the moon’s interior regions.  

“It’s a great day for science,” said Joan Salute, Europa program executive at NASA Headquarters in Washington. “We are thrilled to pass the first major milestone in the lifecycle of a mission that will ultimately inform us on the habitability of Europa.”  

You can follow the development of NASA’s Europa Multiple Flyby Mission here.  

You can learn more about NASA’s space mission here.  

You can discover more about Jupiter’s moon Europa here.  

Learn more about the formation of young stars in galaxy clusters.

Read about NASA’s recent appeal for private business partnerships to help enable the human journey to the stars.

Learn about the kinds of planets space scientists are finding in four star systems.

The Search for the Missing Link in Black Hole Evolution

Space scientists think they have found a black hole family member they thought should exist; an intermediate-mass black hole

A newly discovered cosmic object may help provide answers to some long-standing questions about how black holes evolve and influence their surroundings, according to a new study using NASA’s Chandra X-ray Observatory.
A newly discovered cosmic object may help provide answers to some long-standing questions about how black holes evolve and influence their surroundings, according to a new study using NASA’s Chandra X-ray Observatory.

Space news (June 09, 2015) – 100 million light-years away in the direction of the constellation Camelopardalis – 

Mysterious celestial objects space scientists study to better understand the universe, black holes could hold the keys to unlocking the nature of reality. In fact, a celestial object just discovered may turn out to be the key to a long sought after question about how black holes evolve and alter the surrounding environment. 

Space scientists conducting a study of ultraluminous x-ray sources (ULXs) looking for intermediate-mass black holes using NASA’s Chandra X-ray Observatory believe they have found a candidate. An interesting object, called NGC 2276-3c, located in an arm of spiral galaxy NGC 2276, appears to have the right characteristics.  

“Astronomers have been looking very hard for these medium-sized black holes,” said co-author Tim Roberts of the University of Durham in the UK. “There have been hints that they exist, but the IMBHs have been acting like a long-lost relative that isn’t interested in being found.” 

Space scientists studying black holes have observed objects residing at the center of galaxies with masses millions and even billions of times that of the sun. They have also observed objects with characteristics of smaller black holes, with masses about five to thirty times that of the sun. 

NGC 2276-3c is a middle-class black hole, with a mass about 50,000 times that of the sun, which could grow over the next few billions of years. In fact, space scientists think its home galaxy could at the moment be interacting with elliptical galaxy NGC 2300, which could account for its asymmetrical shape. 

How did space scientists locate and study NGC 2276-3c? Researchers observed the object almost at the same time using both the Chandra X-ray Observatory and European Very Long Baseline Interferometry Network (VLBI). Using the X-ray and radio data obtained, along with known facts concerning the relationship between radio and X-ray luminosities for sources powered by black holes, they estimated the mass of the object to be around 50,000 solar masses. This puts the black hole in the range of mass expected for an IMBH. 

“We found that NGC2276-3c has traits similar to both stellar-mass black holes and supermassive black holes,” said co-author Andrei Lobanov of the Max Planck Institute for Radio Astronomy in Bonn, Germany. “In other words, this object helps tie the whole black hole family together.” 

During the study, space scientists also determined NGC 2276-3c has a characteristic seen in many supermassive black holes, a powerful radio jet extending up to 2,000 light years from the black hole. A region of the radio jet extending for about 1,000 light years, also seems to be missing young stars, which they think could mean the radio jet cleared out a cavity in the surrounding gas and prevented the formation of new stars. Powerful evidence to suggest IMBHs could alter their surrounding environments in amazing ways. 

NGC 2276-3c’s location in the spiral arm of its home galaxy is also making space scientists ask questions. Was it formed in the galaxy, or did it come from the center of a dwarf galaxy that collided and merged with NGC 2276 in the past? 

A recent study by a team of researchers led by Anna Wolter of the National Institute of Astrophysics in Milan, Italy seems to support the merger theory. It concluded that new stars are forming at the rate of about five to fifteen solar masses each year in NGC 2276. A high rate of new star formation they believe was possibly triggered by a possible collision with another galaxy in the past, which points to the formation of this IMBH during a merger between galaxies.   

What’s next?

Now astronomers will do more research on NGC 2275-3c and the radio jet extending from it, in order to look for clues to the effects supermassive black hole seeds existing during the first days of the universe could have had on their surroundings.  

You can learn more about NASA’s flagship X-ray telescope, the Chandra X-ray Observatory here

Learn more about NASA’s space mission to the stars here

Read about space scientists on the trail of a cosmic mystery.  

Learn more about the physical things astronauts deal with.

Learn about the ancient astronomy knowledge of ancient Peruvians.

  

NExSS Coalition Searches for Habitable Planets and Life Beyond Earth

Groundbreaking collaboration between sciences explores planetary zoo for candidates with the ingredients for life

The search for life beyond our solar system requires unprecedented cooperation across scientific disciplines. NASA's NExSS collaboration includes those who study Earth as a life-bearing planet (lower right), those researching the diversity of solar system planets (left), and those on the new frontier, discovering worlds orbiting other stars in the galaxy (upper right). Credits: NASA
The search for life beyond our solar system requires unprecedented cooperation across scientific disciplines. NASA’s NExSS collaboration includes those who study Earth as a life-bearing planet (lower right), those researching the diversity of solar system planets (left), and those on the new frontier, discovering worlds orbiting other stars in the galaxy (upper right).
Credits: NASA

Space news (June 06, 2015) – The human search for life beyond Earth reaches for new horizons this week with the announcement NASA’s bringing together space scientists spanning a variety of scientific fields to form Nexus for Exoplanet System Science (NExSS).

Nexus for Exoplanet System Science (NExSS) brings together top research teams in Earth and planetary science and Helio and Astrophysics in an effort to determine the habitability of exoplanets discovered during the human journey to the beginning of space and time.

“This interdisciplinary endeavor connects top research teams and provides a synthesized approach in the search for planets with the greatest potential for signs of life,” says Jim Green, NASA’s Director of Planetary Science. “The hunt for exoplanets is not only a priority for astronomers, it’s of keen interest to planetary and climate scientists as well.”

Since the beginning of NASA’s Kepler Space Mission six years ago planet hunters have discovered 1852 exoplanets. Currently, there are another 4661 candidates detected by the Kepler Space Telescope, being examined closely for evidence to prove the existence of life beyond Earth. NExSS space scientists will develop techniques to confirm the habitability of these exoplanets by searching for ‘signs of life’.

Earth and planetary scientists, Heliophysicists and Astrophysicists use a “System Science” approach to better understand the ‘signs of life’ they need to look for on exoplanets discovered. They want to understand how life-on-Earth interacts with the atmosphere, geology, oceans and interior of the planet, and how this is affected by our sun. In an effort to develop better techniques to detect life on distant planets.

Dr. Paul Hertz, Director of the Astrophysics Division at NASA notes, “NExSS scientists will not only apply a systems science approach to existing exoplanet data, their work will provide a foundation for interpreting observations of exoplanets from future exoplanet missions such as TESS, JWST, and WFIRST.” The Transiting Exoplanet Survey Satellite (TESS) is working toward a 2017 launch, with the James Webb Space Telescope (JWST) scheduled for launch in 2018. The Wide-field Infrared Survey Telescope (WFIRST) is currently being studied by NASA for a launch in the 2020’s.

The search for life goes on

NExSS is led by Natalie Batalha of NASA’s Ames Research Center, Dawn Gelino of NASA’s Exoplanet Science Institute, and Anthony del Genio of NASA’s Goddard Institute for Space Studies. They’ll lead team members from ten universities and two research institutes as they search for exoplanets with signs of life.

Humans have searched for signs of life in the night sky for thousands of years and some claim to have met and interacted with extraterrestrial beings during this time.

Now, humans desire to meet and communicate with beings from another world, and NExSS is the next step towards finding the answer to the eternal question.

Are we alone in the universe?

To learn more about NExSS and the search for life visit here.

You can learn more about NASA’s space mission to the stars here.

Learn more about planets in four star systems

Read about NASA reaching out to private and business concerns to help enable the human desire to travel to Mars and beyond.

Learn how to calculate the orbits of asteroids within the Main Asteroid Belt.

Space and Time, or Spacetime

Henceforth space by itself, and time by itself, are doomed to fade away into mere shadows, and only a kind of union of the two will preserve an independent reality. (Herman Minkowski, 1908)

Albert Einstein's space-time will astonish and amaze you
Albert Einstein’s space-time will astonish and amaze you

The universe is made of different types of matter and energy traveling through space as time passes unnoticed. Until the time of Einstein, scientists thought and discussed time and space as though they’re absolute and distinct, which is the way they appear to our senses in everyday life. But what if reality is different then it appears?

At the beginning of the twentieth century, Albert Einstein introduced the idea of space and time intertwined in an amazing manner described mathematically by Einstein’s theories of relativity. A scientific theory originally published as two separate parts; the general and special theories of relativity, Einstein’s theories of relativity are currently the most accurate method scientists have to predict physical theory in our universe.

The goal of this series of articles is to show the ability of Einstein’s space-time to help us understand the true nature of physical reality in the universe. This will be accomplished by first providing knowledge and understanding of the flat space-time of the special theory of relativity and consequences of the theory such as length contraction, the twin paradox and time dilation. Next, we’ll offer an introduction to the nature and consequences of the curved space-time of the general theory of relativity, including the idea of an ever-expanding universe, and the nature and meaning of black holes.

The first article in the series is titled “Einstein’s Revelations on Space-time”. This article will be posted during the months ahead and talk about the life and work of Albert Einstein and its stunning revelations for space-time. Einstein’s theories of relativity and their dramatic consequences concerning the true nature of space-time are considered by many to be the greatest scientific discovery of the century. They have replaced ideas concerning the true nature of space and time believed since the age of Newton and Galileo, and are often difficult to grasp at first. In order to better comprehend the theories of relativity readers need to abandon preconceived notions concerning the nature of time and distance measurements, simultaneity, and causality in the universe.

Time and distance measurements in Einstein’s space-time will surprise and startle you and simultaneous events will fool you if you aren’t mentally sharp. The limiting nature of the speed of light also results in interesting consequences for cause and effect in the universe.

Welcome to Einstein’s universe!

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