how many generations does it take to develop
How Many Generations Does It Take To Develop A New Plan...
The mass of a star—how much material it contains—is one of its most important characteristics. If we know a star’s mass, as we shall see, we can estimate how long it will shine and what its ultimate fate will be. Yet the mass of a star is very difficult to measure directly.
Luminosity is the amount of light that a star radiates. The size of the star and its surface temperature determine its luminosity.
Which of the following has contributed most to our understanding of the process of star formation? Astronomers have observed many different stars at each step of the formation process. … A single molecular cloud fragments as it collapses, forming many stars at once.
A star’s life cycle is determined by its mass. … As the main sequence star glows, hydrogen in its core is converted into helium by nuclear fusion. When the hydrogen supply in the core begins to run out, and the star is no longer generating heat by nuclear fusion, the core becomes unstable and contracts.
What property of a star determines how the star will end its life? Mass– the life cycle is determined by the mass of the star. you see, the heavier the star, the shorter its lifespan. very heavy stars only live ~100.000 years, while stars like the sun can last billions of years.
They are all undergoing fusion of hydrogen into helium within their cores. The rate at which they do this and the amount of fuel available depends upon the mass of the star. Mass is the key factor in determining the lifespan of a main sequence star, its size and its luminosity.
Astronomers classify stars according to their physical characteristics. Characteristics used to classify stars include color, temperature, size, composition, and brightness. Stars vary in their chemical composition.
Most important is the composition of the solar surface. In Chapter 5 we examine how the photosphere of a star emits light in a black-body spectrum and how this is modulated by atomic absorptions further out in the star’s atmosphere (see also Sec.
The reason why stars are so important is because they have helped humans navigate through Earth . When it was dark these stars would light up the sky giving people light . In addition stars are very important because they make life on Earth.
Spectroscopic binaries appear close even when viewed through a telescope. Scientists must measure the wavelengths of the light the stars emit and determine their binary nature based on features of those measurements.
The characteristics that are used in order to classify the stars on the Hertzsprung-Russell diagram are size, density, temperature, and absolute brightness.
List the 5 Characteristics used to classify stars. color, temperature, size, composition, and brightness.
It is much closer to us than any other star, and by studying the sun, we can therefore learn more about other stars. The better we understand other stars, the more we know about the Milky Way. From there we know more about other galaxies and in the end we learn more about the universe.
A stellar spectrum can reveal many properties of stars, such as their chemical composition, temperature, density, mass, distance and luminosity. Spectroscopy can show the velocity of motion towards or away from the observer by measuring the Doppler shift.
What is characteristic of a main sequence star? The rate of nuclear energy generated in the hydrogen to helium fusing core equals the rate radiated from the surface. The birth of stars is a battle between gravity and radiation pressure.
Two quantities, mass and age, are probably most fundamental. The progress of a star’s life is predestined by its mass, because ultimately the mass determines how much energy the star can produce and how quickly it will do so. The age of a star tells you how far along it is in its evolution.
What characteristic of a star primarily determines its location on the main sequence? nuclear fusion. Why do higher mass stars live shorter lives on the main sequence than lower mass stars? Higher mass stars burn through their nuclear fuel faster.
These three pieces of evidence, 1) stellar evolu- tion theory, 2) expanding OB associations and 3) the interstellar medium, constitute three basic “proofs” of ongoing star formation in the Milky Way.
The primary factor determining how a star evolves is its mass as it reaches the main sequence.
The spectral type of a star uniquely determines its color. Redder main-sequence stars are fainter on average than bluer main-sequence stars. Based on this, what basic property of a star determines its color (and thus its spectral type)? Temperature.
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