Anyone can look up at the sky at night and see the stars. But what are those little white dots? We know that stars give off light, but most people do not know that stars are composed of atoms. We know that stars are made up of atoms because of the light they emit due to nuclear reactions from atoms within them. Scientists are also able to observe spectral lines when looking through a telescope with a spectrometer attached. They are able to tell based on these spectral lines that stars are made up of mostly hydrogen atoms. We are able to prove that stars are made up of atoms by explaining the atomic model, quantum mechanics, and nuclear reactions.
Every atom is different. Each different type of atom has a different number of protons, neutrons, and electrons. The protons and neutrons make up the nucleus and the electrons orbit the nucleus due to electromagnetism. The number of electrons determines how much energy an atom has. If a high-energy photon comes into contact with an atom, it can cause the electrons to gain more energy. High-energy atoms collide and create nuclear reactions within the stars, which generate even more energy. This high energy is what produces the white light that we see. The simple fact that we can see the light from stars proves that they are made up of atoms.
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When viewing our universe, scientists often attach a spectrometer to a telescope. When they shine white light at it, they can observe certain colors and spectral lines or black lines, which signify which photons or colors we can see and which have been absorbed by the atoms. These black lines on the spectrometer indicate what types of atoms there are based on which types of photons are being absorbed and emitted. Each atom absorbs different colors on the spectrometer, so we are able to tell based on the spectral lines what atom we are
The Atomic Theory is a theory that explains what matter is made of. The Atomic theory states that matter can’t be divided as it is made up of minute particles called atoms that cannot be separated. The very word atom is derived from the Greek word Atmos which means indivisible.
Atoms have three subatomic particles, protons, neutrons and electrons. The atom, the smallest unit of matter which means it’s the smallest thing that takes space and has mass is so small it would take a million of atoms to cross this dot. Knowing they’re incredibly tiny, the electrons having a single negative charge; they move around the nucleus where the protons with a single positive charge and the neutron who does not have a charge are packed. Electrons are only ones that are involved with the chemical activity of an atom, thus, the more electrons an atom has the more energy it will possess. Electrons aren’t just moving around the nucleus, they move around by levels called electron shells. The first level can hold two electrons, the second and third can hold up to eight electrons.
For centuries, physicists and philosophers alike have wondered what makes up our universe. Aristotle thought that all matter came in one of four forms: Earth, Air, Fire, and Water. Since then we have come a long way, with the discovery of the atoms and the subatomic particles they are made of. We can even guess at what makes up protons and neutrons. We have since then discovered and predicted the existence of particles other than the atom, such as the photon, neutrino, axion, and many others.
Stars are born and reborn from an explosion of a previous star. The particles and helium are brought together the same way the last star was born. Throughout the life of a star, it manages to avoid collapsing. The gravitational pull from the core of the star has to equal the gravitational pull of the gasses, which form a type of orbit. When this equality is broken, the star can go into several different stages. Some stars that are at least thirty times larger than our sun can form black holes and other kinds of stars.
The purpose of this lab was to analyse how light and color is created inside an atom in order to deduce what an unknown chemical compound was. We did two different experiments in order to examine how light is created and changed. In one, we looked at how chemical compounds affected a flame’s color, and to determine what the unknown salt contains. In the other lab, we looked at how atoms create light, and how it is displayed on the elements individual spectral line.
An atom, by definition, is the smallest part of any substance. The atom has three main components that make it up: protons, neutrons, and electrons. Protons and neutrons are within the nucleus in the center of the atom. The electrons revolve around the nucleus in many orbitals. These orbitals consist of many different shapes, including circular, spiral, and many others.
When you look into the night sky, sometimes you see small specks of light. Those tiny specks of light are actually giant exploding spheres of hydrogen and helium called stars. Many people know about stars but don't know the many interesting behind them.
Atomism tells us that everything in the universe is fashioned out of small invisible and eternally existing particles called atoms. Certain qualities of atoms explain why different substances have different attributes.
The Atomic Theory began in roughly 400BC with Democritus in Ancient Greece and is universally believed to be correct today. Democritus who was born in 460 BC and died 370 BC and is known as the father of modern science. Democritus proclaimed that everything is made up of atoms. He continued his theory to say that atoms will always be in motion, between atoms there is empty space, atoms are unbreakable, there are an infinite number of atoms all different sizes and shapes. He also said that iron atoms are solid and strong and have hooks to lock them together, water atoms are smooth and slippery, salt atoms have sharp jagged edges because of its taste and air atoms are light and spiralling.
A star begins as nothing more than a very light distribution of interstellar gases and dust particles over a distance of a few dozen lightyears. Although there is extremely low pressure existing between stars, this distribution of gas exists instead of a true vacuum. If the density of gas becomes larger than .1 particles per cubic centimeter, the interstellar gas grows unstable. Any small deviation in density, and because it is impossible to have a perfectly even distribution in these clouds this is something that will naturally occur, and the area begins to contract. This happens because between about .1 and 1 particles per cubic centimeter, pressure gains an inverse relationship with density. This causes internal pressure to decrease with increasing density, which because of the higher external pressure, causes the density to continue to increase. This causes the gas in the interstellar medium to spontaneously collect into denser clouds. The denser clouds will contain molecular hydrogen (H2) and interstellar dust particles including carbon compounds, silicates, and small impure ice crystals. Also, within these clouds, there are 2 types of zones. There are H I zones, which contain neutral hydrogen and often have a temperature around 100 Kelvin (K), and there are H II zones, which contain ionized hydrogen and have a temperature around 10,000 K. The ionized hydrogen absorbs ultraviolet light from it’s environment and retransmits it as visible and infrared light. These clouds, visible to the human eye, have been named nebulae. The density in these nebulae is usually about 10 atoms per cubic centimeter. In brighter nebulae, there exists densities of up to several thousand atoms per cubic centimete...
However Spectroscopy is not a recent development, as it has been utilized for many years since Isaac Newton made the first advances in 1666. Spectroscopy is the study of light as a function of wavelength that has been emitted, reflected or scattered from a solid, liquid, or gas. Fundamentals of Spectroscopy Spectroscopy is the distribution of electromagnetic energy as a function of wavelength. Spectrum is basically white light dispersed by a prism to produce a rainbow of colours; the rainbow is the spectrum of sunlight refracted through raindrops. All objects with temperatures above absolute zero emit electromagnetic radiation by virtue of their warmth alone; this radiation is emitted at increasingly shorter wavelengths as temperature is increased.
For more than 40 years, astrophysicists have predicted that these regions should contain individual atoms left over from the Big Bang, primarily hydrogen and helium, with traces of deuterium, a heavier form of hydrogen, and lithium. But if they were indeed there, they had eluded sure detection until now.As the Universe expanded and cooled down, some of the elements that we see today were created. The Big Bang theory predicts how much of each element should have been made in the early universe, and what we see in very distant galaxies and ancient stars is just right.You cannot look at new stars, like the Sun, for this evidence, because they contain elements that were created in previous generations of stars. As such, the composition of new stars will be very different from the composition of stars that existed 7 billion years ago, shortly after the Big
...ions happen. Supernovas give off many elements we have today including hydrogen and heavier elements such as iron. Supernovas also play a big role in creating new stars because the aftermath of the explosion creates an elemental environment for new interstellar reactions to occur. Discovery of a supernova was difficult at first, given the fact that most occur far away from our galaxy, but new technology now allow scientist to discover many supernova within may galaxies.
Also, he discovered that light could be split into a visible spectrum of colors. Spectral colors from stars would later be used to determine their size, temperature, chemical composition, and even the direction the star is moving. Today, professional astronomers play a very different role than hundreds of years ago. Surprisingly, astronomers today spend minimal time at the telescope gazing at the night sky. Operating planetariums, teaching astronomy classes, or operating and maintaining an observatory are some of the things astronomers today do.
Generally, the universe began as a composition of radiation and subatomic particles, which proceeded with galaxies formation. Galaxies are made up of hydrogen, helium, 100-200 billions of stars, planets and most having a black hole at the center, which attracts everything present in galaxies by force of gravity. Galaxies can be classified as either spiral (Milky Way- galaxy which human kind has been found to exist), elliptical, lenticular and irregular, where the structure is determined by neighboring galaxies with most galaxies are moving away from each other. Classification of galaxies is being conducted by online programs such as Galaxy zoo, using pictures from telescopes and is making significant progress.