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Psychology, Experimental --- Experimental design --- Psychometrics --- Psychologie expérimentale --- Plan d'expérience --- Psychométrie --- Experimental design. --- Psychology, Experimental. --- Psychometrics. --- Psychologie expérimentale --- Plan d'expérience --- Psychométrie --- Measurement, Mental --- Measurement, Psychological --- Psychological measurement --- Psychological scaling --- Psychological statistics --- Psychology --- Psychometry (Psychophysics) --- Scaling, Psychological --- Psychological tests --- Scaling (Social sciences) --- Experimental psychology --- Experimental psychologists --- Design of experiments --- Statistical design --- Mathematical optimization --- Research --- Science --- Statistical decision --- Statistics --- Analysis of means --- Analysis of variance --- Measurement --- Scaling --- Methodology --- Experiments
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If you have ever wondered how we get from the awesome impersonality of the Big Bang universe to the point where living creatures can start to form, and evolve into beings like you, your friends and your family, wonder no more. Steve Miller provides us with a tour through the chemical evolution of the universe, from the formation of the first molecules all the way to the chemicals required for life to evolve. Using a simple Hydrogen molecule – known as H-three-plus - as a guide, he takes us on a journey that starts with the birth of the first stars, and how, in dying, they pour their hearts out into enriching the universe in which we live. Our molecular guide makes its first appearance at the source of the Chemical Cosmos, at a time when only three elements and a total of 11 molecules existed. From those simple beginnings, H-three-plus guides us down river on the violent currents of exploding stars, through the streams of the Interstellar Medium, and into the delta where new stars and planets form. We are finally left on the shores of the sea of life. Along the way, we meet the key characters who have shaped our understanding of the chemistry of the universe, such as Cambridge physicist J.J. Thomson and the Chicago chemist Takeshi Oka. And we are given an insider’s view of just how astronomers, making use of telescopes and Earth-orbiting satellites, have put together our modern view of the Chemical Cosmos.
Cosmochemistry. --- Cosmochemistry --- Physics --- Astronomy & Astrophysics --- Physical Sciences & Mathematics --- Physics - General --- Theoretical Astronomy --- Astrochemistry --- Cosmic chemistry --- Space chemistry --- Physics. --- Physical chemistry. --- Planetology. --- Astronomy. --- Physics, general. --- Popular Science in Astronomy. --- Physical Chemistry. --- Chemistry --- Space sciences --- Chemistry, Physical organic. --- Chemistry, Physical organic --- Chemistry, Organic --- Chemistry, Physical and theoretical --- Planetary sciences --- Planetology --- Natural philosophy --- Philosophy, Natural --- Physical sciences --- Dynamics --- Chemistry, Theoretical --- Physical chemistry --- Theoretical chemistry
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Science --- Space research --- Solar system --- Astrophysics --- Physics --- Physicochemistry --- zonnestelsel --- astrofysica --- popularisering wetenschap --- fysica --- ruimte (astronomie) --- planeten --- astronomie --- fysicochemie
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Science --- Science --- Sciences --- Sciences --- Public opinion. --- Social aspects. --- Opinion publique --- Aspect social
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If you have ever wondered how we get from the awesome impersonality of the Big Bang universe to the point where living creatures can start to form, and evolve into beings like you, your friends and your family, wonder no more. Steve Miller provides us with a tour through the chemical evolution of the universe, from the formation of the first molecules all the way to the chemicals required for life to evolve. Using a simple Hydrogen molecule - known as H-three-plus - as a guide, he takes us on a journey that starts with the birth of the first stars, and how, in dying, they pour their hearts out into enriching the universe in which we live. Our molecular guide makes its first appearance at the source of the Chemical Cosmos, at a time when only three elements and a total of 11 molecules existed. From those simple beginnings, H-three-plus guides us down river on the violent currents of exploding stars, through the streams of the Interstellar Medium, and into the delta where new stars and planets form. We are finally left on the shores of the sea of life. Along the way, we meet the key characters who have shaped our understanding of the chemistry of the universe, such as Cambridge physicist J.J. Thomson and the Chicago chemist Takeshi Oka. And we are given an insider's view of just how astronomers, making use of telescopes and Earth-orbiting satellites, have put together our modern view of the Chemical Cosmos.
Science --- Space research --- Solar system --- Astrophysics --- Physics --- Physicochemistry --- zonnestelsel --- astrofysica --- popularisering wetenschap --- fysica --- ruimte (astronomie) --- planeten --- astronomie --- fysicochemie
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Medical microbiology. --- Microbiology. --- Microbiology --- Infectious Disease Medicine
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