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    Mars’ Surface Hardened Quickly, Boosting Odds of Life: Study

    June 27, 2018, Categories  Astronomy/Space

    This image montage taken by NASA's Curiosity rover shows the surface of planet Mars, which researchers believe hardened only 20 million years after the birth of the Sun, much earlier than first thought

    This image montage taken by NASA’s Curiosity rover shows the surface of planet Mars, which researchers believe hardened only 20 million years after the birth of the Sun, much earlier than first thought

    The crust that encases rocky planets and makes possible the emergence of life took shape on Mars earlier than thought and at least 100 million years sooner than on Earth, researchers said Wednesday. Analysing grains of the mineral zircon extracted from a Martian meteorite known as Black Beauty, they determined that the Red Planet’s outer layer hardened 4.547 billion years ago, only 20 million years after the birth of the Sun.

    “Mars’s primary crust formation—which is the end product of planet formation—happened much faster than previously thought,” said Martin Bizzarro, a scientist at Denmark...

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    Planet Formation Starts Before Star Reaches Maturity

    June 27, 2018, Categories  Astronomy/Space

    MC1A is a still developing star in the constellation Taurus. Red are areas with many dust particles. Green and blue are two types of carbon monoxide. The absence of green / blue carbon monoxide in the inner part indicates that dust particles in the young protoplanetary disk have grown from less than a thousandth of a millimeter to a millimeter. Credit: Jørgensen/Harsono/ESASky/ESAC [CC-BY-SA 3.0]

    MC1A is a still developing star in the constellation Taurus. Red are areas with many dust particles. Green and blue are two types of carbon monoxide. The absence of green / blue carbon monoxide in the inner part indicates that dust particles in the young protoplanetary disk have grown from less than a thousandth of a millimeter to a millimeter. Credit: Jørgensen/Harsono/ESASky/ESAC [CC-BY-SA 3.0]

    A European team of astronomers has discovered that dust particles around a star already coagulate before the star is fully grown. Dust particle growth is the first step in the formation of planets. The researchers from the Netherlands, Sweden and Denmark publish their findings in Nature Astronomy.

    In recent years, astronomers have discovered numerous planetary systems around other stars...

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    Recreating the Chameleon: Material Mimics Color Changes of Living Organisms

    June 27, 2018, Categories  Physics, Technology/Electronics, Chemistry/Nanotechnology

    a) This is a photograph of the spherical colloidal crystals containing 0.20 wt% carbon black (CB). The size of the fine silica particles ranges from 200 to 300 nm, and 11 different sizes were used. b) This is a picture of a weevil drawn using spherical colloidal crystals prepared using monodispersed silica particles with various particle sizes and CB. The surroundings of the weevils are drawn with spherical colloidal crystals that do not contain CB and change with the color of the background. Credit: John Wiley & Sons, Inc.

    a) This is a photograph of the spherical colloidal crystals containing 0.20 wt% carbon black (CB). The size of the fine silica particles ranges from 200 to 300 nm, and 11 different sizes were used. b) This is a picture of a weevil drawn using spherical colloidal crystals prepared using monodispersed silica particles with various particle sizes and CB. The surroundings of the weevils are drawn with spherical colloidal crystals that do not contain CB and change with the color of the background. Credit: John Wiley & Sons, Inc.

    Researchers at Nagoya University develop a composite material that, by adjusting its composition and exposing it to different types of light, can mimic animals’ changes in color...

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    The Na/K-ATPase Oxidant Amplification Loop Regulates Aging

    June 27, 2018, Categories  Health/Medical, Biology/Biotechnology

    Effects of pNaKtide on adipocyte phenotype, senescence, and apoptosis in C57Bl6 aging mice. (A) H&E staining in visceral adipose tissue. Images taken with 40X objective lens; scale bar represents 100 µm. Arrows mark “crown like structures” indicative of inflammation. (B) Quantitative analysis of adipocytes area in visceral adipose tissue. (C) Representative images of TUNEL assay with quantification in C57B16 aging mice. Images taken with 40X objective lens; scale bar represents 25 µm. (D–F) qRT-PCR analysis of ApoJ, p21 and PPARγ in C57Bl6 aging mice with GAPDH as a loading control. Y, young; Y + P, young + pNaKtide; OB, old baseline; O, old; O + P, old + pNaKtide; O + WD, old + western diet; O + WD + P, old + western diet + pNaKtide. N = 8/group, *p < 0.05, **p < 0.01 vs Y, #p < 0.05, ##p < 0.01 vs O, &p < 0.05, &&p < 0.01 vs O + WD.

    Effects of pNaKtide on adipocyte phenotype, senescence, and apoptosis in C57Bl6 aging mice. (A) H&E staining in visceral adipose tissue. Images taken with 40X objective lens; scale bar represents 100 µm. Arrows mark “crown like structures” indicative of inflammation. (B) Quantitative analysis of adipocytes area in visceral adipose tissue. (C) Representative images of TUNEL assay with quantification in C57B16 aging mice. Images taken with 40X objective lens; scale bar represents 25 µm. (D–F) qRT-PCR analysis of ApoJ, p21 and PPARγ in C57Bl6 aging mice with GAPDH as a loading control. Y, young; Y + P, young + pNaKtide; OB, old baseline; O, old; O + P, old + pNaKtide; O + WD, old + western diet; O + WD + P, old + western diet + pNaKtide. N = 8/group, *p < 0.05, **p < 0...

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