The outermost layer of a star is called the photosphere. The temperature at the surface is 5500 K, which corresponds to a shade of yellow. This is because all stars are either blue or white and they become redder as their temperature decreases. The photosphere emits light in every direction, and then it reflects some of this light back into space from its upper layers due to scattering. Some photons escape directly from the top of the star’s atmosphere without being scattered by gas molecules in between.
The photons can be either blue or red as they come from the star, and are scattered by dust particles in space to create an orange glow. The stellar wind is a stream of gas flowing outwards into interstellar space carrying molecules along with it. Usually this type of emission is caused by collisions between atoms that release energy, but there are also other mechanisms for creating fluorescence such as cosmic rays hitting ions or electrons in planetary atmospheres which causes them to emit light.
Interrogating the outermost layer of a star
What is sf’s photosphere?
Why does our sun look yellow?
How is sunlight created when it reaches us on earth? – Do all stars have fluorescent light?
What is the process of creating fluorescent light in a star’s atmosphere?
The photosphere is the outermost layer of a star. The photons can be either blue or red as they come from the star, and are scattered by dust particles in space to create an orange glow. The stellar wind is a stream of gas flowing outwards into interstellar space carrying molecules along with it. Usually this type of emission is caused by collisions between atoms that release energy, but there are also other mechanisms for creating fluorescence such as cosmic rays hitting ions or electrons in planetary atmospheres which causes them to emit light.
A photon becomes “visible” when its wavelength matches one on Earth’s partical spectrum–in other words, it is absorbed by the atmosphere and then re-emitted.
The photosphere is a layer that produces light in stars, but there’s much more than meets the eye. The solar wind can create fluorescence when it interacts with astronomical objects’ atmospheres and release energy to cause them to emit light. What might be happening as a star dies? Is sf IV polar or not? How does this affect its potential habitable zone? These are questions for future research!
A photon becomes visible on Earth’s partical spectrum when it is absorbed by the atmosphere–in other words, emitted back out into space (where we see it). This happens because of something called “fluorescence” where photons collide with particles in planetary atmospheres and are re-emitted.
In this post I will be examining the surface of a star and ask if is it polar or not.
Polar means having a charge or an axis along which electric currents flow, usually positively charged in one direction and negatively charged in the other. In physics, polarity may refer to two types: (i) electric dipoles that arise from unequal distribution of electrons around their atomic nuclei; such as with static electricity where opposite charges are separated over some distance by insulating matter like air. The term can also be used for octupole moments observable at the LHCb detector at CERN’s Large Hadron Collider, where we find eight quarks arranged into four different combinations of colors (red/blue-green/orange-magenta/yellow).
A star is a massive flaming ball of gas that shines due to the energy released from nuclear fusion reactions in its core. The Sun and other stars are astronomical objects, as they have no solid surface (and so can be regarded as spheroids) rather than being self-supporting physical entities; when such luminosities exceed about 106 times solar units, we call them supernovae or hypernovae. A black hole is an object which possesses gravitational force so strong that nothing at all can escape it – not even light!
This blog post will answer if a star is polar. I am going to examine what kind of pole each type of magnetic field has: dipolar magnetics, unipolar magnetics, and diamagnetic.
A star is polar because it has a dipolar magnetic field. It also is not diamagnetic or bipolar.
Dipoles are always perpendicular to the current is directed in them (along the longest axis), but they can be oriented either North-South or East-West depending on how you choose to draw your diagram–which is basically just arbitrary if we’re talking about only two dimensions! So for this particular case, imagine that I’m drawing my diagrams as though looking out at Earth’s South Pole from space: then all of these fields will be shown with their N+S orientation . If one draws instead an “Earth” diagram showing magnetic forces emanating from the center of our planet’s magnetic field, then the fields you see will be oriented North-South.
The dipole is not diamagnetic because it has two poles and so is a monopole of sorts–anything with any “poles” is going to radiate some amount of energy which can have an effect on how external objects or forces interact with them. But that’s just part of what makes stars interesting! The many different contributions to their shapes also come from various features in the stars’ outermost layers.”
A star is polar because it has a dipolar magnetic field. It also isn’t diamagnetic or bipolar.