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  2. Prices of chemical elements - Wikipedia

    en.wikipedia.org/wiki/Prices_of_chemical_elements

    In the form of boric acid, price per boron contained. Min. 99% pure. 6: C: Carbon: 2.267: 200 (5.54 × 10 18 kg) 0.122: 0.28: 2018: EIA Coal [19] In the form of anthracite, price per carbon contained, assuming 90% carbon content. There is a wide variation of price of carbon depending on its form.

  3. List of most expensive paintings - Wikipedia

    en.wikipedia.org/wiki/List_of_most_expensive...

    Georgia O'Keeffe holds the record for the highest price paid for a painting by a woman. On November 20, 2014 at Sotheby's, the Crystal Bridges Museum of American Art bought her 1932 painting Jimson Weed/White Flower No. 1 for US$44.4 million (equivalent to US$57.2 million in 2023). [ 14][ 15] Among the listed top 89, only six are paintings by ...

  4. Wisconsin voters weigh in on Harris, Trump and how they'll ...

    www.aol.com/news/wisconsin-voters-weigh-harris...

    Wisconsin was decided by just 20,000 votes in 2020, remains deeply divided politically and is expected once again to be one of the most important states in this fall’s presidential matchup ...

  5. Cosmological constant - Wikipedia

    en.wikipedia.org/wiki/Cosmological_constant

    Using the values known in 2018 and Planck units for Ω Λ = 0.6889 ± 0.0056 and the Hubble constant H 0 = 67.66 ± 0.42 (km/s)/Mpc = (2.192 7664 ± 0.0136) × 10 −18 s −1, Λ has the value of = = = where is the Planck length. A positive vacuum energy density resulting from a cosmological constant implies a negative pressure, and vice versa.

  6. Boeing still doesn’t know how a plane missing four bolts was ...

    www.aol.com/boeing-still-doesn-t-know-132342888.html

    The door plug blowout on a 737 Max has brought all types of unwanted attention and legal problems to Boeing since the January 5 Alaska Airlines flight. This week Boeing tried its best to put the ...

  7. Discovery of cosmic microwave background radiation - Wikipedia

    en.wikipedia.org/wiki/Discovery_of_cosmic...

    The discovery of cosmic microwave background radiation constitutes a major development in modern physical cosmology. In 1964, US physicist Arno Allan Penzias and radio-astronomer Robert Woodrow Wilson discovered the cosmic microwave background (CMB) , estimating its temperature as 3.5 K, as they experimented with the Holmdel Horn Antenna .

  8. Greisen–Zatsepin–Kuzmin limit - Wikipedia

    en.wikipedia.org/wiki/Greisen–Zatsepin–Kuzmin...

    The Greisen–Zatsepin–Kuzmin limit ( GZK limit or GZK cutoff) is a theoretical upper limit on the energy of cosmic ray protons traveling from other galaxies through the intergalactic medium to our galaxy. The limit is 5 × 1019 eV (50 EeV), or about 8 joules (the energy of a proton travelling at ≈ 99.999 999 999 999 999 999 98 % the speed ...

  9. Cosmic ray - Wikipedia

    en.wikipedia.org/wiki/Cosmic_ray

    The magnitude of the energy of cosmic ray flux in interstellar space is very comparable to that of other deep space energies: cosmic ray energy density averages about one electron-volt per cubic centimetre of interstellar space, or ≈1 eV/cm 3, which is comparable to the energy density of visible starlight at 0.3 eV/cm 3, the galactic magnetic ...