How do you find the density of the Sun?
Table of Contents
How do you find the density of the Sun?
1.41 g/cm³
Sun/Density
Density is mass over volume, so the average den- sity of the Sun is 1.42 g/cm3. Finally, we just need to convert this to number density by dividing the mass density by the mass per particle. The mass per particle is given as 10−24 g, so we get the average number density of the Sun to be 1.42·1024 particles/cm3.
What is the density of each layer of the Sun?
| Age | At least 4.5 billion years, in present state. |
|---|---|
| Mean density of entire Sun | 1.41 g/cm^3 |
| Interior (center of the Sun) | 160 g/cm^3 |
| Surface (photosphere) | 10^{-9} g/cm^3 |
| Chromosphere | 10^{-12} g/cm^3 |
What is the average density of the Sun kg/m 3?
Bulk parameters
| Sun | Ratio (Sun/Earth) | |
|---|---|---|
| Volumetric mean radius (km) | 695,700. | 109.2 |
| Mean density (kg/m3) | 1408. | 0.255 |
| Surface gravity (eq.) (m/s2) | 274.0 | 28.0 |
| Escape velocity (km/s) | 617.6 | 55.2 |
What is the density of the photosphere?
(b) Estimate the particle density of the photosphere which has an average density of about 10–6 kg/m3.
What is the average density of the Sun How does it compare to the average density of Earth?
The radius of the sun at 696,000 km is 109 times the Earth’s radius. Its surface gravity is 274 m/s2 or 28.0 times that of the Earth. Its mean density is 1410 kg/m3 or 0.255 times the mean density of Earth.
How dense is the chromosphere?
The density of the chromosphere decreases with distance from the center of the Sun. This decreases exponentially from 1017 particles per cubic centimeter, or approximately 2×10−4 kg/m3 to under 1.6×10−11 kg/m3 at the outer boundary.
What is the density of the Sun’s core?
about 150 g/cm³
The temperature at the very center of the Sun is about 15,000,000° C (27,000,000° F) and the density is about 150 g/cm³ (approximately 10 times the density of gold, 19.3 g/cm³ or lead, 11.3 g/cm³).
How many Jupiters can fit in the Sun?
1,000 Jupiters
According to multiple studies, around 1,000 Jupiters could fit into the Sun.
What is the density of the Sun compared to Earth?
On average, it has a density of 1.408 g/cm3, which is roughly one-quarter that of Earth. However, models of the sun estimate that it has a density of 162.2 g/cm3 closer to the core, which is 12.4 times that of Earth.
How does the density affect the photosphere?
The electron density is a strong function of density and the negatively ionized hydrogen drops off rapidly above the photosphere. The sun’s limb is darker than the center. Another effect which can be observed in the photosphere are the electron transitions which form absorption lines.
How do you find density if you only have mass?
The formula for density is the mass of an object divided by its volume. In equation form, that’s d = m/v , where d is the density, m is the mass and v is the volume of the object.