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  2. Solar mass - Wikipedia

    en.wikipedia.org/wiki/Solar_mass

    The diurnal parallax of the Sun was accurately measured during the transits of Venus in 1761 and 1769, [5] yielding a value of 9″ (9 arcseconds, compared to the present value of 8.794 148 ″). From the value of the diurnal parallax, one can determine the distance to the Sun from the geometry of Earth. [6] [7]

  3. List of Solar System objects by size - Wikipedia

    en.wikipedia.org/wiki/List_of_Solar_System...

    The size of solid bodies does not include an object's atmosphere. For example, Titan looks bigger than Ganymede, but its solid body is smaller. For the giant planets , the "radius" is defined as the distance from the center at which the atmosphere reaches 1 bar of atmospheric pressure.

  4. Planetary mass - Wikipedia

    en.wikipedia.org/wiki/Planetary_mass

    The choice of solar mass, M ☉, as the basic unit for planetary mass comes directly from the calculations used to determine planetary mass.In the most precise case, that of the Earth itself, the mass is known in terms of solar masses to twelve significant figures: the same mass, in terms of kilograms or other Earth-based units, is only known to five significant figures, which is less than a ...

  5. Sun - Wikipedia

    en.wikipedia.org/wiki/Sun

    He reasoned that it was a giant flaming ball of metal even larger than the land of the Peloponnesus and that the Moon reflected the light of the Sun. [176] Eratosthenes estimated the distance between Earth and the Sun in the third century BC as "of stadia myriads 400 and 80000", the translation of which is ambiguous, implying either 4,080,000 ...

  6. Stellar mass - Wikipedia

    en.wikipedia.org/wiki/Stellar_mass

    The Sun is losing mass from the emission of electromagnetic energy and by the ejection of matter with the solar wind. It is expelling about (2–3) × 10 −14 M ☉ per year. [ 16 ] The mass loss rate will increase when the Sun enters the red giant stage, climbing to (7–9) × 10 −14 M ☉ y −1 when it reaches the tip of the red-giant ...

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  8. Earth mass - Wikipedia

    en.wikipedia.org/wiki/Earth_mass

    Earth's density varies considerably, between less than 2700 kg/m 3 in the upper crust to as much as 13 000 kg/m 3 in the inner core. [13] The Earth's core accounts for 15% of Earth's volume but more than 30% of the mass, the mantle for 84% of the volume and close to 70% of the mass, while the crust accounts for less than 1% of the mass. [13]

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