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  2. Significant figures - Wikipedia

    en.wikipedia.org/wiki/Significant_figures

    If it is the rough estimation, then only the first three non-zero digits are significant since the trailing zeros are neither reliable nor necessary; 45600 m can be expressed as 45.6 km or as 4.56 × 10 4 m in scientific notation, and neither expression requires the trailing zeros. An exact number has an infinite number of significant figures.

  3. Chronology of computation of π - Wikipedia

    en.wikipedia.org/wiki/Chronology_of_computation...

    Showed that π is not a Liouville number: 1954 S. C. Nicholson & J. Jeenel Using the NORC [26] 13 minutes 3,093: 1957 George E. Felton: Ferranti Pegasus computer (London), calculated 10,021 digits, but not all were correct [27] [28] 33 hours 7,480: January 1958 Francois Genuys IBM 704 [29] 1.7 hours 10,000: May 1958 George E. Felton: Pegasus ...

  4. Neutrino - Wikipedia

    en.wikipedia.org/wiki/Neutrino

    Each second, about 65 billion (6.5 × 10 10) solar neutrinos pass through every square centimeter on the part of the Earth orthogonal to the direction of the Sun. [15] Since neutrinos are insignificantly absorbed by the mass of the Earth, the surface area on the side of the Earth opposite the Sun receives about the same number of neutrinos as ...

  5. Pi - Wikipedia

    en.wikipedia.org/wiki/Pi

    The number π (/ p aɪ / ⓘ; spelled out as "pi") is a mathematical constant, approximately equal to 3.14159, that is the ratio of a circle's circumference to its diameter.It appears in many formulae across mathematics and physics, and some of these formulae are commonly used for defining π, to avoid relying on the definition of the length of a curve.

  6. Big Bang - Wikipedia

    en.wikipedia.org/wiki/Big_Bang

    A few minutes into the expansion, when the temperature was about a billion kelvin and the density of matter in the universe was comparable to the current density of Earth's atmosphere, neutrons combined with protons to form the universe's deuterium and helium nuclei in a process called Big Bang nucleosynthesis (BBN). [35]

  7. Great Oxidation Event - Wikipedia

    en.wikipedia.org/wiki/Great_Oxidation_Event

    Stage 1 (3.85–2.45 Ga): Practically no O 2 in the atmosphere. The oceans were also largely anoxic – with the possible exception of O 2 in the shallow oceans.; Stage 2 (2.45–1.85 Ga): O 2 produced, rising to values of 0.02 and 0.04 atm, but absorbed in oceans and seabed rock.

  8. Sea level rise - Wikipedia

    en.wikipedia.org/wiki/Sea_level_rise

    Modelling results predict that Asia will suffer direct economic damages of US$167.6 billion at 0.47 meters of sea level rise. This rises to US$272.3 billion at 1.12 meters and US$338.1 billion at 1.75 meters. There is an additional indirect impact of US$8.5, 24 or 15 billion from population displacement at those levels.

  9. 2013 Virginia gubernatorial election - Wikipedia

    en.wikipedia.org/wiki/2013_Virginia...

    Cuccinelli's 2013 campaign conducted an analysis that found McAuliffe's spending plan would cost at least $14 billion – including $12 billion in new spending – over a four-year term and would translate into a $1,700 tax hike on the average Virginia family.