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on April 25, 2022

How far as a percentage does the radiative zone extend to the photosphere?

Space and Astronomy

Above the core is a region known as the radiative zone—named for the primary mode of transporting energy across it. This region starts at about 25% of the distance to the solar surface and extends up to about 70% of the way to the surface.

Contents:

  • How far does the radiation zone extend?
  • How long is the radiative zone?
  • What percent of the diameter of the Sun is the radiative zone?
  • How deep is the radiative zone?
  • What happens in the photosphere?
  • How thick is the photosphere?
  • What percentage of the Sun is the photosphere?
  • Where do you find the photosphere?
  • How thick is the chromosphere?
  • What is chromosphere photosphere?
  • What is in the chromosphere?
  • What does the chromosphere contribute to the solar spectrum?
  • What is the differences between chromosphere and photosphere?
  • How far does the solar corona extend?
  • Is the chromosphere hotter than the photosphere?
  • How can the corona be hotter than the photosphere which is closer to the surface of the Sun?
  • How does the Parker Solar Probe not melt?
  • How can you identify the chromosphere during a total solar eclipse?
  • Is the chromosphere heated by the corona?
  • How hot is the chromosphere?
  • Is chromosphere visible?
  • Where is the chromosphere of the Sun quizlet?
  • What does a chromosphere look like?

How far does the radiation zone extend?

The radiative zone extends outward from the outer edge of the core to the interface layer or tachocline at the base of the convection zone (from 25% of the distance to the surface to 70% of that distance).

How long is the radiative zone?

approximately 0.25 to 0.7 solar radii

Just outside the Inner Core of the sun at a distance approximately 0.25 to 0.7 solar radii lies the Radiative Zone. This zone radiates energy through the process of photon emission and capture by the hydrogen and helium ions.

What percent of the diameter of the Sun is the radiative zone?

The radiative zone of the sun starts at about 25 percent of the radius, and extends to about 70 percent of the radius.

How deep is the radiative zone?

Around the core there is the radiative zone. In this region, energy is transported by radiation (you have radiation around the core of a nuclear central, around a nuclear explosion,…). With respect to the surface of the Sun, the radiative zone extends from a depth of 515,000 km to 200,000 km.

What happens in the photosphere?

The photosphere is the lowest layer of the sun’s atmosphere — the innermost layer we can observe directly. The term photosphere means “sphere of light” and is the layer where most of the sun’s energy is emitted. It takes about eight minutes for sunlight from the photosphere to reach Earth.

How thick is the photosphere?

about 300 km thick

The photosphere is about 300 km thick. Most of the Sun’s visible light that we see originates from this region. The chromosphere is about 2000 km thick. We only see this layer and the other outer layers during an eclipse.

What percentage of the Sun is the photosphere?

The Sun is composed primarily of the chemical elements hydrogen and helium; they account for 74.9% and 23.8% of the mass of the Sun in the photosphere, respectively.

Where do you find the photosphere?

Photosphere – The photosphere is the deepest layer of the Sun that we can observe directly. It reaches from the surface visible at the center of the solar disk to about 250 miles (400 km) above that.

How thick is the chromosphere?

The chromosphere is the second most outer layer of the Sun. Several thousand kilometres thick, it resides above the photosphere and beneath the corona.



What is chromosphere photosphere?

the corona – the outermost, hot shell of the atmosphere. the chromosphere – a transparent layer between the corona and the photosphere. the photosphere – the visible “surface” of the Sun. the sunspots – dark areas on the photosphere, which are cooler than the surroundings.

What is in the chromosphere?

The chromosphere is above the photosphere, the visible “surface” of the Sun. It lies below the solar corona, the Sun’s upper atmosphere, which extends many thousands of kilometers above the chromosphere into space. The plasma (electrically charged gas) in the chromosphere has a very low density.

What does the chromosphere contribute to the solar spectrum?

A wavelength of 656.3 nm is in the red part of the spectrum, which causes the chromosphere to have its characteristic reddish colour. By analysing the spectrum of the chromosphere, it was found that the temperature of this layer of the solar atmosphere increases with height in the chromosphere itself.

What is the differences between chromosphere and photosphere?

The photosphere is the Sun’s outer shell from which light is radiated. It has a surface temperature of about 6,000K. The chromosphere is above the photosphere. I is a low density layer which is about 2,000km thick.

How far does the solar corona extend?

5 million miles



All NASA Missions
Now, using NASA’s Solar Terrestrial Relations Observatory, scientists have found that this atmosphere, called the corona, is even larger than thought, extending out some 5 million miles above the sun’s surface — the equivalent of 12 solar radii.

Is the chromosphere hotter than the photosphere?

While the photosphere hovers around 5,800 kelvin, the temperature of the chromosphere varies between 4,500 K and 20,000 K. Even though it’s more distant from the center of the Sun, the chromosphere is hotter than the photosphere.

How can the corona be hotter than the photosphere which is closer to the surface of the Sun?

Jim Klimchuk, a solar scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, explained that the new evidence supports a theory that the sun’s corona is heated by tiny explosions called nanoflares.

How does the Parker Solar Probe not melt?

The thermal Protection System (TPS) is 8 feet (2.4 meters) in diameter and 4.5 inches (115 millimeters) thick to protect Parker Solar Probe from the intense heat generated by the Sun. Even though the shield provides just a few inches of protection, this allows the spacecraft to maintain a temperature of 85 F (30 C).



How can you identify the chromosphere during a total solar eclipse?

How can you identify the chromosphere during a total solar eclipse? It’s a reddish glow at the end or beginning of an eclipse.

Is the chromosphere heated by the corona?

In the chromosphere, almost all the mechanical energy flux supplied to the outer solar atmosphere by magneto-convection is converted into heat and radiation, leaving a small amount to power the solar wind and the hot corona: the chromosphere requires over 30 times more energy than the corona and heliosphere combined.

How hot is the chromosphere?

The chromosphere lies above the photosphere and temperatures range from approximately 11,000 degrees F (6,000 degrees C) nearest the photosphere to about 7,200 degrees F (4,000 degrees C) a couple of hundred miles higher up.

Is chromosphere visible?

It is about 2,000 to 3,000 kilometres deep, which is located immediately above the photosphere and just below the corona. It is normally not visible because its density is very low and due to the excessive brightness of the photosphere. The chromosphere, thus, can be only seen during a complete solar eclipse.

Where is the chromosphere of the Sun quizlet?

Where is the chromosphere on the Sun? It is the layer above the visible surface of the Sun.



What does a chromosphere look like?

The chromosphere (colour sphere), named by the English astronomer Sir Joseph Norman Lockyer in 1868, appears briefly as a bright crescent, red with hydrogen light, during solar eclipses when the body of the Sun is almost obscured by the Moon.

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