Stars are made up of mainly hydrogen and helium gases, along with trace amounts of other elements like carbon, oxygen, and nitrogen. These elements undergo nuclear fusion in the star's core, producing energy and light.
The fusion of iron into heavier elements cannot support a star because it requires more energy than it produces, leading to a loss of energy and the collapse of the star.
Stars are made up of mostly hydrogen and helium gas, along with trace amounts of other elements. The force of gravity causes these gases to come together and form a star. As the gases compress and heat up, nuclear fusion reactions occur in the star's core, producing energy and light. This energy counteracts the force of gravity, keeping the star stable and allowing it to shine. The size, temperature, and lifespan of a star are determined by its mass and composition.
The most numerous elements in the Earth's crust are oxygen, silicon, aluminum, and iron. These elements make up the majority of the Earth's crust by mass.
The four elements that make up over 95 percent of the human body are oxygen, carbon, hydrogen, and nitrogen. These elements are fundamental in forming essential molecules like proteins, carbohydrates, and fats, which are crucial for energy production and bodily functions.
The presence of elements heavier than helium in stars is important because they provide crucial information about the star's age, composition, and evolutionary history. These heavier elements, also known as metals, are created through nuclear fusion processes in the cores of stars and are dispersed into space when the star dies. By studying the abundance of these elements in a star, scientists can gain insights into its formation and evolution.
Hydrogen and Helium
Stars are composed mostly of hydrogen and helium.
The two main gases that make up a young star are hydrogen and helium. These elements were formed during the Big Bang and are the most abundant elements in the universe.
The mystery star is made up of a variety of elements, such as hydrogen, helium, carbon, oxygen, and trace amounts of other elements like iron, silicon, and nitrogen. These elements are formed through nuclear fusion processes that occur in the star's core.
The exact mix is different depending on the star's age and size, but hydrogen and helium are always the two most prevalent elements.
The exact mix is different depending on the star's age and size, but hydrogen and helium are always the two most prevalent elements.
Objects are not made of forces. A star is made of hydrogen, helium and, later in its life, heavier elements.
It allows scientists to see how hot that star is and what spectrum it has.
Carbon and oxygen are the two main elements that make up a white dwarf star. These elements are the end products of nuclear fusion in the core of the star before it exhausted its nuclear fuel and collapsed to form a white dwarf.
Scientists can assess which elements are present in the star, by looking at the light it gives off and breaking this light down into the different colours that make up the total colour. They look at the spectrum given off. The different elements present in the star cause different light wavelengths (or colours) to be emitted.
Carbon, hydrogen and oxygen are the only elements that make up sugars.
New elements - helium always, heavier elements often (up to iron) and heavier than that if the star explodes.