Weighing Massive Stars in nearby Galaxy reveals Excess of Heavyweights

The star-forming region, 30 Doradus, is one of the largest located close to the Milky Way and is found in the neighboring galaxy, Large Magellanic Cloud. About 2,400 massive stars in the center of 30 Doradus, also known as the Tarantula Nebula, are producing intense radiation and powerful winds as they blow off material. Credit: NASA

The star-forming region, 30 Doradus, is one of the largest located close to the Milky Way and is found in the neighboring galaxy, Large Magellanic Cloud. About 2,400 massive stars in the center of 30 Doradus, also known as the Tarantula Nebula, are producing intense radiation and powerful winds as they blow off material. Credit: NASA

An international team has revealed an ‘astonishing’ overabundance of massive stars in a neighbouring galaxy. The discovery, made in the gigantic star-forming region 30 Doradus in the Large Magellanic Cloud galaxy, has ‘far-reaching’ consequences for our understanding of how stars transformed the pristine Universe into the one we live in today...

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New Lithium-rich Battery could Last much Longer

The battery uses both oxygen and iron to store and release electrical energy. Credit: Zhenpeng Yao

The battery uses both oxygen and iron to store and release electrical energy. Credit: Zhenpeng Yao

By using iron and oxygen to simultaneously drive the electrochemical reaction, a novel battery is less expensive and has a higher capacity. On paper, it doesn’t seem like Christopher Wolverton’s super lithium-rich battery should work. For one, the novel battery uses iron, an inexpensive metal that has notoriously failed in batteries. And in another difficult feat, the battery leverages oxygen to help drive the chemical reaction, which researchers previously believed would cause the battery to become unstable. But not only does the battery work, it does so incredibly well.

Teaming up with researchers at Argonne National Laboratory, Wolverton’s group at Northwestern University developed a recha...

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Astronomers discover an M-dwarf Eclipsing Binary system

Astronomers discover an M-dwarf eclipsing binary system

Left: GMOS acquisition image of the binary system. The binary system is indicated by the green mark, where the third object (at a separation of 0.5 arcseconds) is well resolved. The Gemini spectra were carried out with a position angle of 90 degrees east of north, hence were resolve both the eclisping binary system and the third object into spectra. Right: GMOS spectra. The top panel shows the eclipsing binary spectrum (upper) and the third light object spectrum (lower). The primay (P) and secondary (S) component of the eclipsing binary system are indicated by the green label. The bottom panel shows the relative flux (in ADU) of the Hα emission line from the primary and secondary component of the ecliping binary system. Credit: Lee at al., 2017.

Astronomers have found a new eclipsing bina...

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Tabby’s Star: Alien Megastructure Not the Cause of Dimming of the ‘most Mysterious Star in the universe’

This illustration depicts an uneven ring of dust orbiting KIC 8462852, also known as Boyajian’s Star or Tabby's Star. Credit: NASA/JPL-Caltech

This illustration depicts an uneven ring of dust orbiting KIC 8462852, also known as Boyajian’s Star or Tabby’s Star. Credit: NASA/JPL-Caltech

Scientists are one step closer to solving the mystery. A team of more than 200 researchers, including Penn State Department of Astronomy and Astrophysics Assistant Professor Jason Wright and led by Louisiana State University’s Tabetha Boyajian, is one step closer to solving the mystery behind KIC 8462852, or “Tabby’s Star,” nicknamed after Boyajian, is otherwise an ordinary star, about 50% bigger and 1,000 degrees hotter than the Sun, and about than 1,000 light years away. However, it has been inexplicably dimming and brightening sporadically like no other...

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