photosphere

For the Sun, the surface is taken to mean the photosphere.

Let's say the photosphere, about a million kilometers from the center.

I believe we are now in what is called the star's photosphere."

Here, the core was the star, extending out almost to the photosphere itself.

Above the level of the photosphere is the stellar atmosphere.

The buried heat would leak to the photosphere and out.

The same physical effect makes sunspots dark in the photosphere.

The visible outer surface of the Sun is called the photosphere.

At the time of my waking, the photosphere was almost sterile.

"But we're cruising through the photosphere of a star, as you may have noticed."

Of course we'll have to slow down as the photosphere gets thicker, but that's all right.

The temperature of the star's photosphere has been measured at 5,368 24 K.

The Sun's radius is measured from its center to the edge of the photosphere.

Therefore, the photosphere is typically used to describe the Sun's or another star's visual surface.

These often have strong magnetic fields in their photosphere.

Below him still, a vague rolling sphere of fire, lay the photosphere.

The temperature of the photosphere is 5998 kelvins and have mass 5% more than our Sun.

In the outer reaches of the photosphere, the density is extremely low.

It is within the photosphere that sun spots, or regions of lower than average temperature, appear.

It moves upwards at about 20 km/s from the photosphere.

Lieserl, you may not believe this, but you're actually illuminating the photosphere.

Stars slowly lose mass by the emission of a stellar wind from the photosphere.

In the bottom part it touches the photosphere and gravity shapes the features.

The optical depth at the photosphere turns out to be .

The outer, light-emitting layer of a star is known as the photosphere.