We can calculate it by applying Newton's version of Kepler's third law with Earth's orbital period (1 year) and Earth's average distance from the Sun (1 AU).
The four variables astronomers use to classify stars are temperature, luminosity, size or radius, and mass. By analyzing these properties, astronomers can determine a star's position on the Hertzsprung-Russell diagram and classify it into different spectral types and stages of stellar evolution.
Astronomers study celestial bodies, helio astronomers specifically study suns.
Scientists determine the Milky Way's mass outside the Sun's orbit by observing the motions of stars and gas in the galaxy and using gravitational models to calculate the total mass that is needed to hold these objects in their orbits. This method allows for estimating the mass of the Milky Way's dark matter halo, which makes up the majority of its mass.
The color of a star can provide information about its temperature and age. Hotter stars tend to appear blue while cooler stars appear redder. By studying the color of a star, astronomers can determine its surface temperature and stage in its life cycle.
The mass of the Sun can be determined using Kepler's Third Law of Planetary Motion, which relates the period of a planet's orbit to its distance from the Sun. By knowing the period of Earth's orbit (1 year) and its average distance from the Sun (1 astronomical unit), we can calculate the Sun's mass to be approximately 1.989 x 10^30 kg.
Astronomers determine the mass of the sun by observing the orbits of planets and other celestial bodies around it. They use Newton's law of universal gravitation and Kepler's laws of planetary motion to calculate the mass of the sun accurately. By measuring the orbital velocities and distances of objects in the solar system, astronomers can infer the mass of the sun through mathematical calculations.
In order to conveniently compare the distances from the various planets, astronomers devised a measure called the "astronomical unit". The Earth is one AU from the Sun. In order to conveniently compare the sizes of other stars to our Sun, astronomers use a "solar mass" as the mass of the Sun. and a "solar radius" as the radius of our Sun. This helps to make the comparisons more obvious to non-astronomers.
It's not got an exact definition, but astronomers usually mean a star of about 8 times the mass of the Sun or higher.
Astronomers use complex calculations to determine celestial bodies' distance.They've stated that the sun is 150 million kilometers far away from the Earth.
Astronomers can determine the star's temperature, chemical composition, mass, luminosity, and age by analyzing its spectrum. By studying the absorption and emission lines in the spectrum, astronomers can also infer the star's motion, magnetic fields, and if it has any companions such as planets or other stars.
Astronomers think the sun will die in 2012
Astronomers use the method of parallax to determine the distance to relatively close stars like Sirius. By measuring the apparent shift in position of the star as the Earth moves around the Sun, astronomers can calculate the star's distance based on trigonometry.
Parallax is the method that astronomers use to measure the distance from the sun to the earth.
Yes. In fact, it seems that most galaxies have a gigantic black hole (with a mass of millions, or even billions, of times the mass of our Sun) in their center.
To calculate the mass of the sun, scientists use the gravitational pull it exerts on other objects, like planets. By observing the orbits of planets around the sun and applying Newton's law of universal gravitation, they can determine the sun's mass. This method is based on the relationship between the mass of an object and the gravitational force it generates.
No.
For two or three hundred years, astronomers have had a fair idea the the Sun is not the center of the Universe.