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  2. Atmosphere - Wikipedia

    en.wikipedia.org/wiki/Atmosphere

    A stellar atmosphere is the outer region of a star, which includes the layers above the opaque photosphere; stars of low temperature might have outer atmospheres containing compound molecules. The atmosphere of Earth is composed of nitrogen (78%), oxygen (21%), argon (0.9%), carbon dioxide (0.04%) and trace gases. [2]

  3. Atmosphere of Earth - Wikipedia

    en.wikipedia.org/wiki/Atmosphere_of_Earth

    The atmosphere of Earth is composed of a layer of gas mixture that surrounds the Earth's planetary surface (both lands and oceans), known collectively as air, with variable quantities of suspended aerosols and particulates (which create weather features such as clouds and hazes), all retained by Earth's gravity.

  4. Primary atmosphere - Wikipedia

    en.wikipedia.org/wiki/Primary_atmosphere

    A primary atmosphere is an atmosphere of a planet that forms by accretion of gaseous matter from the accretion disc of the planet's sun. Planets such as Jupiter and Saturn have primary atmospheres. Primary atmospheres are very thick compared to secondary atmospheres like the one found on Earth .

  5. Omega Leonis - Wikipedia

    en.wikipedia.org/wiki/Omega_Leonis

    The primary is a G-type main sequence star with a spectral classification of G1 V. [5] It has about 35% [9] more mass than the Sun and shines six [10] times as brightly from an outer atmosphere that has an effective temperature of 5940 K. [9] The system is roughly 3.7 billion years old [9] and is a member of the galactic thin disk population. [9]

  6. Planetary core - Wikipedia

    en.wikipedia.org/wiki/Planetary_core

    The internal structure of the inner planets. The internal structure of the outer planets. A planetary core consists of the innermost layers of a planet. [1] Cores may be entirely liquid, or a mixture of solid and liquid layers as is the case in the Earth. [2]

  7. Outer space - Wikipedia

    en.wikipedia.org/wiki/Outer_space

    In 2009, measurements of the direction and speed of ions in the atmosphere were made from a sounding rocket. The altitude of 118 km (73.3 mi) above Earth was the midpoint for charged particles transitioning from the gentle winds of the Earth's atmosphere to the more extreme flows of outer space.

  8. Stellar corona - Wikipedia

    en.wikipedia.org/wiki/Stellar_corona

    Coronal stars are ubiquitous among the stars in the cool half of the Hertzsprung–Russell diagram. [25] These coronae can be detected using X-ray telescopes. Some stellar coronae, particularly in young stars, are much more luminous than the Sun's. For example, FK Comae Berenices is the prototype for the FK Com class of variable star. These are ...

  9. Secondary atmosphere - Wikipedia

    en.wikipedia.org/wiki/Secondary_atmosphere

    The giant planets, such as Jupiter and Saturn, became large enough where they were able to hold onto their primary atmosphere that they gained during formation while terrestrial planets, such as Venus and Earth, do not have enough gravity to hold onto the original atmosphere. By being made of rock, they are able to go through geologic processes ...