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    Category Astronomy/Space

    Cosmic barbecue: Researchers spot 60 new ‘hot Jupiter’ candidates

    July 8, 2017, Categories  Astronomy/Space

    The diagram above shows a hot Jupiter at various phases of its orbit. The sizes of the star and planet and the separations between them are to scale for a typical hot Jupiter. The amount of reflected starlight that is observed depends on the planet's position within its orbit and the inclination of the orbit with respect to the observer.

    The diagram above shows a hot Jupiter at various phases of its orbit. The sizes of the star and planet and the separations between them are to scale for a typical hot Jupiter. The amount of reflected starlight that is observed depends on the planet’s position within its orbit and the inclination of the orbit with respect to the observer.

     
    Yale researchers have identified 60 potential new “hot Jupiters” — highly irradiated worlds that glow like coals on a barbecue grill and are found orbiting only 1% of Sun-like stars. Hot Jupiters constitute a class of gas giant planets located so close to their parent stars that they take less than a week to complete an orbit. Second-year Ph.D...
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    First look at Gravitational Dance that drives Stellar Formation

    July 7, 2017, Categories  Astronomy/Space

    Left: three color composite image of SDC13 where red, green and blue bands correspond to 70?m HIGAL (Molinari et al. 2010), 24?m Spitzer MIPSGAL (Carey et al. 2009) and 8?m Spitzer GLIMPSE (Churchwell et al. 2009) maps respectively. The four dark, filamentary arms are clearly visible. Right: Brand new, high resolution map of SDC13 tracing the internal dense ammonia gas revealing cores dotted along all the filaments. Credit: G. Williams et al. / University of Cardiff

    Left: three color composite image of SDC13 where red, green and blue bands correspond to 70?m HIGAL (Molinari et al. 2010), 24?m Spitzer MIPSGAL (Carey et al. 2009) and 8?m Spitzer GLIMPSE (Churchwell et al. 2009) maps respectively. The four dark, filamentary arms are clearly visible. Right: Brand new, high resolution map of SDC13 tracing the internal dense ammonia gas revealing cores dotted along all the filaments. Credit: G. Williams et al. / University of Cardiff

    Swirling motions in clouds of cold, dense gas have given, for the first time, an active insight into how gravity creates the compact cores from which stars form in the interstellar medium...

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    Re-Making Planets after Star-Death

    July 7, 2017, Categories  Astronomy/Space

    1. Data at wavelength of 0.45 mm, combined from SCUBA and SCUBA-2, in a false-colour image. The Geminga pulsar (inside the black circle) is moving towards the upper left, and the orange dashed arc and cylinder show the ‘bow-wave’ and a ‘wake’. The region shown is 1.3 light-years across; the bow-wave probably stretches further behind Geminga, but SCUBA imaged only the 0.4 light-years in the centre. Credit: Jane Greaves / JCMT / EAO. 2. Sketch of the nebula formed by a wind of electrons and positrons coming from the pulsar, and the interaction with interstellar gas. Geminga crossed the plane of the Galaxy (off to the bottom right) around 100,000 years ago. It is thought that the supernova explosion was not symmetric, causing the remnant to recoil at around 200 km per second from its birth location. Credit: Jane Greaves / University of Cardiff.

    1. Data at wavelength of 0.45 mm, combined from SCUBA and SCUBA-2, in a false-colour image. The Geminga pulsar (inside the black circle) is moving towards the upper left, and the orange dashed arc and cylinder show the ‘bow-wave’ and a ‘wake’. The region shown is 1.3 light-years across; the bow-wave probably stretches further behind Geminga, but SCUBA imaged only the 0.4 light-years in the centre. Credit: Jane Greaves / JCMT / EAO. 2. Sketch of the nebula formed by a wind of electrons and positrons coming from the pulsar, and the interaction with interstellar gas. Geminga crossed the plane of the Galaxy (off to the bottom right) around 100,000 years ago...

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    Recreating Interstellar Ions with Lasers

    July 6, 2017, Categories  Astronomy/Space

    1. Mechanisms and time-resolved dynamics for trihydrogen cation (H3 ) formation from organic molecules in strong laser fields. Scientific Reports, 2017; 7 (1) DOI: 10.1038/s41598-017-04666-w 2. MSU's Marcos Dantus has recreated interstellar ions with lasers. Credit: Courtesy of MSU

    1. Mechanisms and time-resolved dynamics for trihydrogen cation (H3 ) formation from organic molecules in strong laser fields. Scientific Reports, 2017; 7 (1) DOI: 10.1038/s41598-017-04666-w
    2. MSU’s Marcos Dantus has recreated interstellar ions with lasers.
    Credit: Courtesy of MSU

    Trihydrogen, H3+, is called the molecule that made the universe, where it plays a greater role in astrochemistry than any other molecule. While H3+ is astronomically abundant, no scientist understood the mechanisms that form it from organic molecules. Until now. Using lasers, Michigan State University scientists have unlocked the secret and published their results in the current issue of Scientific Reports...

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