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Topic: Star

NASA Researchers are creating Alien Atmospheres on Earth

 

NASA Jet Propulsion Laboratory 

NASA - National Aeronautics and Space AdministrationPasadena, CA – Researchers at NASA’s Jet Propulsion Laboratory in Pasadena, California, are cooking up an alien atmosphere right here on Earth. In a new study, JPL scientists used a high-temperature “oven” to heat a mixture of hydrogen and carbon monoxide to more than 2,000 degrees Fahrenheit (1,100 Celsius), about the temperature of molten lava.

The aim was to simulate conditions that might be found in the atmospheres of a special class of exoplanets (planets outside our solar system) called “hot Jupiters.”

This artist's concept shows planet KELT-9b, an example of a "hot Jupiter," or a gas giant planet orbiting very close to its parent star. KELT-9b is an extreme example of a hot Jupiter, with dayside temperatures reaching 7,800 degrees Fahrenheit (4,300 Celcius). (NASA/JPL-Caltech)

This artist’s concept shows planet KELT-9b, an example of a “hot Jupiter,” or a gas giant planet orbiting very close to its parent star. KELT-9b is an extreme example of a hot Jupiter, with dayside temperatures reaching 7,800 degrees Fahrenheit (4,300 Celcius). (NASA/JPL-Caltech)

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NASA’s NICER instrument discovers Black Hole consuming nearby Star

 

Written by Jeanette Kazmierczak
NASA’s Goddard Space Flight Center

NASA - National Aeronautics and Space AdministrationGreenbelt, MD – Scientists have charted the environment surrounding a stellar-mass black hole that is 10 times the mass of the Sun using NASA’s Neutron star Interior Composition Explorer (NICER) payload aboard the International Space Station.

NICER detected X-ray light from the recently discovered black hole, called MAXI J1820+070 (J1820 for short), as it consumed material from a companion star. Waves of X-rays formed “light echoes” that reflected off the swirling gas near the black hole and revealed changes in the environment’s size and shape.

In this illustration of a newly discovered black hole named MAXI J1820+070, a black hole pulls material off a neighboring star and into an accretion disk. Above the disk is a region of subatomic particles called the corona. (Aurore Simonnet and NASA’s Goddard Space Flight Center)

In this illustration of a newly discovered black hole named MAXI J1820+070, a black hole pulls material off a neighboring star and into an accretion disk. Above the disk is a region of subatomic particles called the corona. (Aurore Simonnet and NASA’s Goddard Space Flight Center)

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NASA Hubble Space Telescope captures image of Cosmic Holiday Wreath

 

Space Telescope Science Institute (STScI) 

NASA - National Aeronautics and Space AdministrationWashington, D.C. – This festive NASA Hubble Space Telescope image resembles a holiday wreath made of sparkling lights. The bright southern hemisphere star RS Puppis, at the center of the image, is swaddled in a gossamer cocoon of reflective dust illuminated by the glittering star. The super star is ten times more massive than the Sun and 200 times larger.

RS Puppis rhythmically brightens and dims over a six-week cycle. It is one of the most luminous in the class of so-called Cepheid variable stars. Its average intrinsic brightness is 15,000 times greater than the Sun’s luminosity.

NASA Hubble Space Telescope's cosmic holiday wreath is made up of sparkling stars with RS Puppis, a type of variable star known as a Cepheid variable. As variable stars go, Cepheids have comparatively long periods — RS Puppis, for example, varies in brightness by almost a factor of five every 40 or so days. RS Puppis is unusual; this variable star is shrouded by thick, dark clouds of dust enabling a phenomenon known as a light echo to be shown with stunning clarity. These Hubble observations show the ethereal object embedded in its dusty environment, set against a dark sky filled with background galaxies. (NASA, ESA and the Hubble Heritage Team (STScI/AURA) – Hubble/Europe Collaboration; Acknowledgement: H. Bond (STScI and Pennsylvania State University)

NASA Hubble Space Telescope’s cosmic holiday wreath is made up of sparkling stars with RS Puppis, a type of variable star known as a Cepheid variable. As variable stars go, Cepheids have comparatively long periods — RS Puppis, for example, varies in brightness by almost a factor of five every 40 or so days. RS Puppis is unusual; this variable star is shrouded by thick, dark clouds of dust enabling a phenomenon known as a light echo to be shown with stunning clarity. (NASA, ESA and the Hubble Heritage Team (STScI/AURA) – Hubble/Europe Collaboration; Acknowledgement: H. Bond (STScI and Pennsylvania State University)

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Two NASA Space Telescopes observe rapid growth of Young Star

 

NASA Jet Propulsion Laboratory 

NASA - National Aeronautics and Space AdministrationPasadena, CA – An adolescent star in the midst of a dramatic growth phase has been observed with the help of two NASA space telescopes. The youngster belongs to a class of stars that gain mass when matter swirling around the star falls onto its surface.

The in-falling matter causes the star to appear about 100 times brighter. Astronomers have found only 25 stars in this class, and only about half of those have been observed during an outburst.

This illustration shows a young star undergoing a type of growth spurt. Left: Material from the dusty and gas-rich disk (orange) plus hot gas (blue) mildly flows onto the star, creating a hot spot. Middle: The outburst begins - the inner disk is heated, more material flows to the star, and the disk creeps inward. Right: The outburst is in full throttle, with the inner disk merging into the star and gas flowing outward (green). (Caltech/T. Pyle (IPAC))

This illustration shows a young star undergoing a type of growth spurt. Left: Material from the dusty and gas-rich disk (orange) plus hot gas (blue) mildly flows onto the star, creating a hot spot. Middle: The outburst begins – the inner disk is heated, more material flows to the star, and the disk creeps inward. Right: The outburst is in full throttle, with the inner disk merging into the star and gas flowing outward (green). (Caltech/T. Pyle (IPAC))

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NASA’s Kepler Space Telescope captures last moments of dying Star

 

NASA Headquarters

NASA - National Aeronautics and Space AdministrationWashington, D.C. – In a galaxy far away, an old star exploded and became a supernova. About 170 million years later on February 4th, 2018, the light emanating from the explosion was received by an arsenal of high-powered telescopes.

NASA’s Kepler space telescope detected the unfurling light of SN 2018oh, as it has been labeled. The first ground-based facility to identify the signal was with the All-Sky Automated Survey for Supernova and soon observatories around the globe were monitoring the supernova as part of a unique scientific experiment designed to help solve the mystery of how stars explode.

This image scenario leading to a particular kind of Type Ia supernova in which a single white dwarf siphons off so much material from its companion star that it can no longer sustain its own weight and blows up.  It is one theory explaining the data from SN 2018oh. (NASA/JPL-Caltech)

This image scenario leading to a particular kind of Type Ia supernova in which a single white dwarf siphons off so much material from its companion star that it can no longer sustain its own weight and blows up. It is one theory explaining the data from SN 2018oh. (NASA/JPL-Caltech)

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NASA’s Parker Solar Probe now holds record for Closest Spacecraft to Sun

 

Written by Sarah Frazier
NASA’s Goddard Space Flight Center

NASA - National Aeronautics and Space AdministrationGreenbelt, MD – The NASA Parker Solar Probe now holds the record for closest approach to the Sun by a human-made object. The spacecraft passed the current record of 26.55 million miles from the Sun’s surface on October 29th, 2018, at about 12:04pm CEDT, as calculated by the Parker Solar Probe team.

The previous record for closest solar approach was set by the German-American Helios 2 spacecraft in April 1976. As the NASA Parker Solar Probe mission progresses, the spacecraft will repeatedly break its own records, with a final close approach of 3.83 million miles from the Sun’s surface expected in 2024.

NASA's Parker Solar Probe became the closest-ever spacecraft to the Sun on October 29th, 2018, when it passed within 26.55 million miles of the Sun’s surface. (NASA/JHUAPL)

NASA’s Parker Solar Probe became the closest-ever spacecraft to the Sun on October 29th, 2018, when it passed within 26.55 million miles of the Sun’s surface. (NASA/JHUAPL)

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NASA’s Spitzer Space Telescope takes a look at star forming Cat’s Paw Nebula

 

NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – This image from NASA’s Spitzer Space Telescope shows the Cat’s Paw Nebula, so named for the large, round features that create the impression of a feline footprint. The nebula is a star-forming region in the Milky Way galaxy, located in the constellation Scorpius. Estimates of its distance from Earth range from about 4,200 to about 5,500 light-years.

Framed by green clouds, the bright red bubbles are the dominant feature in the image, which was created using data from two of Spitzer’s instruments.

The Cat's Paw Nebula, imaged here by NASA's Spitzer Space Telescope using the MIPS and IRAC instruments, is a star-forming region that lies inside the Milky Way Galaxy. New stars may heat up the surrounding gas, which can expand to form "bubbles." (NASA/JPL-Caltech)

The Cat’s Paw Nebula, imaged here by NASA’s Spitzer Space Telescope using the MIPS and IRAC instruments, is a star-forming region that lies inside the Milky Way Galaxy. New stars may heat up the surrounding gas, which can expand to form “bubbles.” (NASA/JPL-Caltech)

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NASA’s Hubble, Kepler Space Telescopes discover possible Moon outside our Solar System

 

NASA Headquarters

NASA - National Aeronautics and Space AdministrationWashington, D.C. – Using NASA’s Hubble and Kepler space telescopes, astronomers have uncovered tantalizing evidence of what could be the first discovery of a moon orbiting a planet outside our solar system.

This moon candidate, which is 8,000 light-years from Earth in the Cygnus constellation, orbits a gas-giant planet that, in turn, orbits a star called Kepler-1625. Researchers caution that the moon hypothesis is tentative and must be confirmed by follow-up Hubble observations.

NASA’s Hubble and Kepler space telescopes have uncovered what could be the first moon outside our solar system ever found. More observations are needed to confirm this discovery. (NASA/ESA/L. Hustak)

NASA’s Hubble and Kepler space telescopes have uncovered what could be the first moon outside our solar system ever found. More observations are needed to confirm this discovery. (NASA/ESA/L. Hustak)

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NASA’s Hubble Space Telescope captures Ultraviolet Panoramic View of the Universe

 

NASA Headquarters

NASA - National Aeronautics and Space AdministrationWashington, D.C. – Astronomers using the ultraviolet vision of NASA’s Hubble Space Telescope have captured one of the largest panoramic views of the fire and fury of star birth in the distant universe.

The field features approximately 15,000 galaxies, about 12,000 of which are forming stars. Hubble’s ultraviolet vision opens a new window on the evolving universe, tracking the birth of stars over the last 11 billion years back to the cosmos’ busiest star-forming period, which happened about 3 billion years after the big bang.

Astronomers have just assembled one of the most comprehensive portraits yet of the universe’s evolutionary history, based on a broad spectrum of observations by the Hubble Space Telescope and other space and ground-based telescopes. (NASA, ESA, P. Oesch (University of Geneva), and M. Montes (University of New South Wales))

Astronomers have just assembled one of the most comprehensive portraits yet of the universe’s evolutionary history, based on a broad spectrum of observations by the Hubble Space Telescope and other space and ground-based telescopes. (NASA, ESA, P. Oesch (University of Geneva), and M. Montes (University of New South Wales))

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NASA’s Chandra X-ray Observatory sees Planet destroyed by nearby Star

 

NASA’s Marshall Space Flight Center

NASA - National Aeronautics and Space AdministrationHuntsville, AL – Scientists may have observed, for the first time, the destruction of a young planet or planets around a nearby star. Observations from NASA’s Chandra X-ray Observatory indicate that the parent star is now in the process of devouring the planetary debris. This discovery gives insight into the processes affecting the survival of infant planets.

Since 1937, astronomers have puzzled over the curious variability of a young star named RW Aur A, located about 450 light years from Earth. Every few decades, the star’s optical light has faded briefly before brightening again. In recent years, astronomers have observed the star dimming more frequently, and for longer periods.

This artist’s illustration depicts the destruction of a young planet or planets, which scientists may have witnessed for the first time using data from NASA’s Chandra X-ray Observatory. (Illustration: NASA/CXC/M. Weiss; X-ray spectrum: NASA/CXC/MIT/H. M.Günther)

This artist’s illustration depicts the destruction of a young planet or planets, which scientists may have witnessed for the first time using data from NASA’s Chandra X-ray Observatory. (Illustration: NASA/CXC/M. Weiss; X-ray spectrum: NASA/CXC/MIT/H. M.Günther)

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