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  2. Sun - Wikipedia

    en.wikipedia.org/wiki/Sun

    Illustration of different stars' internal structure based on mass. The Sun in the middle has an inner radiating zone and an outer convective zone. The radiative zone is the thickest layer of the Sun, at 0.45 solar radii. From the core out to about 0.7 solar radii, thermal radiation is the primary means of energy transfer. [74]

  3. Helophilus pendulus - Wikipedia

    en.wikipedia.org/wiki/Helophilus_pendulus

    The abdomen is patterned with yellow, black and grey, and for this reason it is sometimes called the footballer. [3] It has a black central face-stripe. It has a wing-length of 8.5–11.25 mm (0.33–0.44 in). The tergites two and three are yellow patterned with black. The black pattern consists of a band across the apex of the tergite (on its ...

  4. Solar System - Wikipedia

    en.wikipedia.org/wiki/Solar_System

    [f] Six planets, seven dwarf planets, and other bodies have orbiting natural satellites, which are commonly called 'moons'. The Solar System is constantly flooded by the Sun's charged particles, the solar wind, forming the heliosphere. Around 75–90 astronomical units from the Sun, [g] the solar wind is halted, resulting in the heliopause.

  5. Convection zone - Wikipedia

    en.wikipedia.org/wiki/Convection_zone

    These are the granular zones in the outer layers of the stars. A convection zone, convective zone or convective region of a star is a layer which is unstable due to convection. Energy is primarily or partially transported by convection in such a region. In a radiation zone, energy is transported by radiation and conduction.

  6. Sphere of influence (astrodynamics) - Wikipedia

    en.wikipedia.org/wiki/Sphere_of_influence_(astro...

    In the patched conic approximation, once an object leaves the planet's SOI, the primary/only gravitational influence is the Sun (until the object enters another body's SOI). Because the definition of r SOI relies on the presence of the Sun and a planet, the term is only applicable in a three-body or greater system and requires the mass of the ...

  7. Poles of astronomical bodies - Wikipedia

    en.wikipedia.org/wiki/Poles_of_astronomical_bodies

    The poles of astronomical bodies are determined based on their axis of rotation in relation to the celestial poles of the celestial sphere. Astronomical bodies include stars, planets, dwarf planets and small Solar System bodies such as comets and minor planets (e.g., asteroids), as well as natural satellites and minor-planet moons.

  8. Analemma - Wikipedia

    en.wikipedia.org/wiki/Analemma

    What is called the analemma, on the globe, is a narrow slip of paper, the length of which is equal to the breadth of the torrid zone. It is pasted on some vacant place on the globe, in the torrid zone, and is divided into months and days of months, correspondent to the sun's declination for every day in the year.

  9. Orrery - Wikipedia

    en.wikipedia.org/wiki/Orrery

    An orrery should properly include the Sun, the Earth and the Moon (plus optionally other planets). A model that only includes the Earth, the Moon, and the Sun is called a tellurion or tellurium, and one which only includes the Earth and the Moon is a lunarium. A jovilabe is a model of Jupiter and its moons. [22]