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  2. Cavendish experiment - Wikipedia

    en.wikipedia.org/wiki/Cavendish_experiment

    Cavendish's result provided additional evidence for a planetary core made of metal, an idea first proposed by Charles Hutton based on his analysis of the 1774 Schiehallion experiment. [18] Cavendish's result of 5.4 g·cm −3 , 23% bigger than Hutton's, is close to 80% of the density of liquid iron , and 80% higher than the density of the Earth ...

  3. Metallicity - Wikipedia

    en.wikipedia.org/wiki/Metallicity

    In astronomy, metallicity is the abundance of elements present in an object that are heavier than hydrogen and helium. Most of the normal currently detectable (i.e. non-dark) matter in the universe is either hydrogen or helium, and astronomers use the word "metals" as convenient shorthand for "all elements except hydrogen and helium".

  4. It is not just heavy metals which can be toxic; other metals (for example beryllium and lithium) can be toxic too. [266] Sleeping in a closed room with an electric fan running does not result in "fan death", as is widely believed in South Korea among older people. [267] [268] As of 2019 this belief was in decline. [269]

  5. Planetary habitability - Wikipedia

    en.wikipedia.org/wiki/Planetary_habitability

    A high proportion of metals in a star correlates to the amount of heavy material initially available in the protoplanetary disk. A smaller amount of metal makes the formation of planets much less likely, under the solar nebula theory of planetary system formation. Any planets that did form around a metal-poor star would probably be low in mass ...

  6. Homestake experiment - Wikipedia

    en.wikipedia.org/wiki/Homestake_experiment

    The Homestake experiment was followed by other experiments with the same purpose, such as Kamiokande in Japan, SAGE in the former Soviet Union, GALLEX in Italy, Super Kamiokande, also in Japan, and SNO (Sudbury Neutrino Observatory) in Ontario, Canada. SNO was the first detector able to detect neutrino oscillation, solving the solar neutrino ...

  7. Sudbury Neutrino Observatory - Wikipedia

    en.wikipedia.org/wiki/Sudbury_Neutrino_Observatory

    The heavy water was viewed by approximately 9,600 photomultiplier tubes (PMTs) mounted on a geodesic sphere at a radius of about 850 centimetres (28 ft). The cavity housing the detector was the largest in the world at such a depth, [ 6 ] requiring a variety of high-performance rock bolting techniques to prevent rock bursts.

  8. Atomic and molecular astrophysics - Wikipedia

    en.wikipedia.org/wiki/Atomic_and_molecular...

    At these high frequencies, molecules in the Earth's atmosphere can block transmissions from space, and telescopes must be located in dry (water is an important atmospheric blocker), high sites. Radio telescopes must have very accurate surfaces to produce high fidelity images.

  9. Astrochemistry - Wikipedia

    en.wikipedia.org/wiki/Astrochemistry

    The discovery of interstellar formaldehyde – and later, other molecules with potential biological significance, such as water or carbon monoxide – is seen by some as strong supporting evidence for abiogenetic theories of life: specifically, theories which hold that the basic molecular components of life came from extraterrestrial sources.