Nov 22, 2024 · This interactive 3D model of the Sun, our star, allows you to explore the surface of the Sun up close. Access the interactive here or find the downloadable file below.

May 2, 2018 · @ThePlushieGamer7 The sun isn't mostly white, actually. It's a type G star, meaning that it is not hot enough to produce white light. White stars are typically very young, very luminous, and very hot, being generally types A, B, or O. …

The standard solar model (SSM) is a mathematical model of the Sun as a spherical ball of gas (in varying states of ionisation, with the hydrogen in the deep interior being a completely ionised plasma).

From the center out, the three large interior layers of the Sun are (1) the core, (2) the radiative zone, and (3) the convective zone. The outer visible layers are (4) the photosphere, (5) the chromosphere, and (6) the outermost layer, the corona, which extends outward for …

Oct 10, 2012 · This graphic shows a model of the layers of the Sun, with approximate mileage ranges for each layer: for the inner layers, the mileage is from the sun’s core; for the outer layers, the mileage is from the sun’s surface. The inner layers are the Core, Radiative Zone and Convection Zone.

Online 3D simulation of the Solar System and night sky in real-time - the Sun, planets, dwarf planets, comets, stars and constellations

The standard solar model is one of the most complete and successful theories in modern astronomy. I discuss the basic assumptions of the model: hydrostatic equilibrium, energy trans-port, thermonuclear reactions, and initial conditions. The successes and failures of the model are illustrated, followed by a brief analysis of the model data.

Visualize orbits, relative positions and movements of the Solar System objects in an interactive 3D Solar System viewer and simulator.

The Standard Model of the Sun (see Figure 1) makes it possible for scientists to estimate the temperature profile of the sun. Data from the sun's profile (see Figure 2) make it possible to make observations, predictions, and to compare these predictions based on the Standard Solar Model.

Apr 25, 2020 · From the interior to the outer atmosphere: core, where nuclear reaction occurs, the engine of the star; radiative zone, where energy is primarily transported toward the exterior by means of radiative diffusion; convective zone, where energy is primarily transported by convection; photosphere, the shell from which light is radiated; chromosphere,...