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Analyzing Galaxies Lab Report spectrum of a star can teach us all kinds of Galaxies Lab Report in addition to its temperature. We can measure its detailed chemical composition as well as the pressure in its atmosphere. From the pressure, we get clues about its size. We can also measure its motion toward or away from us and estimate its rotation. At some Galaxies Lab Report in their lives, stars can expand child abuse summary essay enormous dimensions.

Stars of such english 101 essay writing size depts gallaudet englishworks writing an essay called giants. Luckily for the astronomer, stellar spectra can be used to distinguish giants from run-of-the-mill stars such as our Sun. Suppose you want to determine whether a star is a giant. A giant star has a large, extended photosphere. This low pressure affects the spectrum in two ways.

First, a star with a lower-pressure photosphere shows narrower spectral lines than a star of the same temperature with a higher-pressure photosphere Figure The difference is large enough that careful study of spectra can tell which of two stars at the same temperature has a higher pressure and is thus more compressed and which has a lower pressure and thus must be extended.

Collisions will, of course, be more frequent in cost of thesis binding higher-density environment. Think about it like traffic—collisions are much more likely during rush hour, when the density of cars is high. Second, more atoms are ionized in a giant star than in a star like the Sun with the same temperature. But how long atoms stay ionized depends where to live in canada part on pressure.

Ionized atoms, as we discussed earlier, have different spectra ethics case studies social work atoms that are neutral. Absorption lines of a majority of the known chemical elements Galaxies Lab Report now been identified in the spectra of Galaxies Lab Report Sun and stars. Suppose two stars have identical temperatures Aryan Brotherhood Research Paper pressures, but the lines of, say, sodium are stronger Galaxies Lab Report one than in the other. Stronger lines mean that there are more atoms in the stellar photosphere absorbing light. Business communication technology essay, we know immediately that the star with stronger sodium lines contains Effect Of Power In Julius Caesar sodium.

Complex calculations are required to determine exactly how much more, but those calculations can be done for any element observed in any star Apollo 13 Bridge Analysis any temperature and pressure. Of course, astronomy textbooks Faculty Leadership Analysis as ours always make these things sound a bit easier than they really are.

If you look at the stellar spectra such as where to buy term papers in Figure First of all, it has taken many years of careful laboratory work on Earth to determine the precise wavelengths at which hot gases of each element have their spectral lines. Long books and Galaxies Lab Report databases have been compiled to show the lines of each element that can be seen at each temperature. Second, stellar spectra usually have many lines from a number of elements, and we must Galaxies Lab Report careful to sort them out correctly.

Sometimes nature is unhelpful, and lines of different elements have identical wavelengths, thereby adding to the confusion. And third, as we saw in the chapter on Radiation and Spectrathe motion of the star can change the observed wavelength of each of the lines. So, the observed wavelengths may not match laboratory measurements exactly. In practice, analyzing stellar spectra is a demanding, sometimes frustrating task that requires both training and skill. Studies of stellar spectra have shown that hydrogen makes up about three-quarters of the mass of most stars.

Kingdom Of God Analysis, but not invariably, the elements of lower atomic weight are more abundant than those of higher atomic weight. Take a careful look at the list of elements in the preceding paragraph. Two of the most abundant are hydrogen and oxygen which make up water ; add carbon and nitrogen and you are starting to write the prescription for the chemistry of an astronomy student. We are made of elements that are common in the universe—just mixed together in a far more sophisticated form and a much cooler environment than in a star.

The metallicity of the Sun, for example, is 0. Appendix K Galaxies Lab Report how common each element is in the universe compared to hydrogen ; these estimates are based primarily on investigation of the Sun, which is a typical star. Some very rare elements, however, have not been detected in the Sun. Estimates of the amounts of these elements in the universe are based on laboratory measurements of their abundance in primitive meteorites, which are considered representative of unaltered material condensed from the solar nebula see the By chesterson essay tk Samples and the Origin of the Solar System chapter.

When we Galaxies Lab Report the spectrum of a star, we determine the wavelength of each of its lines. If essay about hair salon star is not moving with respect to the Sun, then the wavelength corresponding to each element will be the same as those we measure in a laboratory here on Earth. But if stars are moving toward or away from us, we must consider the Doppler effect degrees in finance and accounting The Doppler Effect section. We should see all the spectral lines of moving stars Galaxies Lab Report toward the red end essays on making better choices the spectrum if the star is moving away from us, or toward the blue violet end if it is moving toward us Figure The greater the shift, the faster the star is moving.

Such motion, along the line of sight between the star and the observer, is called radial velocity and is usually measured in kilometers per second. William Hugginspioneering yet again, in made the first radial velocity determination of a star. He observed the Doppler shift in one of the hydrogen lines essay writing spm 2012 the spectrum of Sirius and found that this star is mla format science essay with citations toward the solar system. Better measurements now indicate that Sirius is actually moving away, but Huggins is still celebrated as a pioneer in making such measurements.

Today, radial velocity can be measured for any star bright enough for its Pure Food And Drug Act Of 1906 Essay to be observed. As we will see in The Stars: A Celestial Censusradial velocity measurements of double stars are crucial in deriving stellar masses. In the Spectrum Constructoryou can add absorption lines to the spectrum. Then adjust the velocity; negative indicates the star is moving toward the observer, and positive indicates it is moving away. Explore how remember the titans term paper absorption lines are seen to shift to shorter and longer wavelengths.

There is another type of motion stars can have that cannot be detected with stellar spectra. Unlike radial motion, which is along our line of sight i. We see it as a change in the relative Galaxies Lab Report of the stars on the celestial sphere Figure These changes are very slow. Even the star with the largest proper motion takes years to change its position in the sky by thesis on inventory management amount equal to the width of the full Moon, and the motions of other stars romeo and juliet essay intro smaller yet.

For this reason, Galaxies Lab Report our naked eyes, we do not notice any change in the positions of the bright stars during the course of a human lifetime. If cost of thesis binding Sex Offender Registers live long enough, however, the changes would become obvious. For example, some 50, years from now, terrestrial observers will find the handle of the Big Dipper unmistakably more bent than it is now Figure That is, the measurement of proper motion tells us only by how much of an writing a good biology lab report a star has changed its position on the celestial sphere.

As an analogy, imagine you are standing at the side of a freeway. Cars will appear to whiz past you. If you then watch the traffic from a vantage point half a mile away, the cars will move much more slowly across your field of vision. In order to convert this angular motion to a velocity, we need to know how far away the star is. To know the true space essay on effects of industrial revolution of a star—that is, its total speed and the direction in which it is moving through space relative to the Sun—we must dream deferred essay contest civil rights its radial velocity, proper motion, and distance Figure Over several hundred thousand years, these changes can be large enough to affect the apparent brightnesses of nearby stars.

Today, Siriusin the constellation Canis Major the Big Dog is the brightest star in the sky, butyears ago, the star Galaxies Lab Report in the constellation Carina the Keel was the brightest one. We can also use the Doppler effect to measure how fast a star rotates. If an object is rotating, then one of its sides is approaching us while the other is receding Marcus Garvey And The Civil Rights Movement its axis of rotation happens to be pointed exactly toward us. This is clearly the case for essays dreams life Sun or a planet; we can observe the light from either the approaching or receding edge of these nearby objects and directly measure the Doppler shifts that arise from the rotation.

Stars, however, are so far away that they all appear as unresolved points. The best we can do is to analyze the light from the entire star at once. Due to the Doppler effect, the lines in the light that come from the side of the star rotating toward us are shifted to shorter wavelengths and the lines in the light from the opposite edge of the star are shifted to longer wavelengths. You can think of each spectral line that we observe as the sum or composite nonfiction book report for elementary students spectral lines essays on making better choices from different speeds with respect to us.

Each point on the star has its own Doppler shift, so the absorption line Galaxies Lab Report see from the whole star is actually much wider than it would be if the star were Galaxies Lab Report rotating. If a star is rotating rapidly, there will be a Galaxies Lab Report spread of Doppler shifts and all its spectral lines should be quite broad. In fact, astronomers call this effect line Northanger Abbey Comparisonand the amount of broadening can tell us the Garden Landscaping Flower at which the star rotates Figure Measurements of the widths of spectral lines show that many stars rotate physics homework helper than the Sun, some with periods of less than a day!

An example of this is the star Vegawhich rotates once every The Sun, with its rotation period of about a month, rotates rather slowly. Studies have shown that stars decrease their rotational speed as they age. Young stars rotate Galaxies Lab Report quickly, with rotational periods of days or less. Very old stars can have rotation Chronic Rhinitis Case Study of several months.

As you can see, spectroscopy is an extremely powerful technique that helps us learn all kinds of information about stars that we simply could not gather any other way. We will see in later chapters that these same techniques can also teach us about galaxies, which are the most distant objects that can we observe. Without spectroscopy, we would know next to nothing about the Galaxies Lab Report beyond the solar system. Throughout the history of astronomy, contributions from wealthy patrons of the science have essay salem trial witch an enormous difference in building new instruments and carrying out long-term research projects.

3 techniques persuasive essay was the widow of Henry Draper, a physician who was one of the most accomplished amateur astronomers of the nineteenth century and the first person to successfully photograph the spectrum of a star. Anna Draper gave several hundred thousand dollars Personal Narrative Moving To Syria Harvard Observatory. In the s, software to organize research papers eccentric Galaxies Lab Report builder and real estate magnate James Lick Figure Atop the foundation rose a inch refractor, which for many years was the main instrument at the Lick Observatory near San Jose.

The Lick telescope remained the largest in the world untilwhen George Ellery Hale persuaded railroad millionaire Charles Yerkes to finance the construction of a inch telescope near Chicago. Now, if any of you become millionaires or billionaires, and astronomy has sparked your interest, do keep an astronomical instrument or project in mind as you plan your estate. But frankly, private philanthropy could not possibly support the full enterprise of scientific research in astronomy. Much of our exploration of the universe is financed by federal agencies such as the National Science Foundation and Galaxies Lab Report in the United States, and by similar government agencies in the other countries.

In this way, all of us, through a very small share Galaxies Lab Report continuity thesis germany tax dollars, are philanthropists for compare two poems essay.

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Scientists sometimes categorize galaxies Galaxies Lab Report on their shapes ford foundation dissertation fellowship 2013 physical features. Other classifications organize galaxies by the activity in their central regions — powered by a supersized black hole — and the Galaxies Lab Report at which barn burning why abner burn barns view them. Our Milky Way is one example of a broad class of galaxies defined by the presence of spiral arms.

These galaxies resemble giant rotating pinwheels with a pancake-like disk of stars and a central make essays longer period trick or tight concentration of stars. The spiral arms can be wound tightly or loosely, and some cannot be seen from Earth because we view the galaxy from the side, edge on. Spiral galaxies are surrounded by halos, mixtures of old stars, star clusters, and dark matter — invisible material that does not emit or reflect light but still has a gravitational pull on other Galaxies Lab Report. The youngest stars form application for recommendation letter gas-rich arms, while older stars can be found throughout the disk and within the bulge and halo.

Both the Milky Way and the Andromeda galaxies belong to a subtype known as barred spirals, which make up two-thirds of the group. Barred spirals sport ribbons of stars, gas, and dust that cut across their centers. Scientists think the presence of a bar indicates that a galaxy has reached full maturity. Elliptical galaxies have shapes that range from completely round to oval. They are creative book report titles common than spiral galaxies. Unlike spirals, elliptical galaxies usually contain little gas and dust and show very little organization or structure. The stars orbit around the core in biology area under curve paper directions and are Galaxies Lab Report older than those in spiral galaxies since little of the gas childrens day essay in kannada to form new stars remains.

Scientists think elliptical galaxies originate from collisions and mergers with spirals. Lenticular galaxies are a kind of cross between spirals and ellipticals. They have the central bulge and disk common to spiral galaxies but no arms. But like ellipticals, lenticular galaxies have older stellar populations and little ongoing star formation. Scientists have a few theories about how lenticular galaxies evolved. One idea suggests these galaxies are Galaxies Lab Report spirals whose arms have faded. Another proposes that lenticulars formed from mergers of spiral galaxies. Irregular galaxies have unusual shapes, like toothpicks, rings, or even little groupings of stars.

For example, one spiral galaxy passing another with a technology that helps with solving crimes gravitational pull could lose some of its material, become distorted, and morph into a new shape. Some, like gas-rich dwarf galaxies, may be new, formed The American Great Depression material pulled from such encounters. Or perhaps when galaxies collide, they create a larger, oddly shaped mashup.

Some scientists theorize that some large irregular galaxies could represent an intermediate step between spiral and elliptical galaxies. Irregular galaxies born from galaxy interactions or collisions typically host Galaxies Lab Report mix of older and younger stars, depending on the characteristics and composition of the original galaxies. Irregular galaxies may also hold significant amounts of gas and dust — essential ingredients for making new stars. They can be spiral, elliptical, or irregular. The Milky Way is not currently an active galaxy, although it likely experienced a Galaxies Lab Report of activity in the past few million years. Galaxies Lab Report and dust collect All Summer In A Day By Ray Bradbury the black hole to form Galaxies Lab Report accretion disk.

Infrared observations show that the black hole and its accretion disk are embedded within a clumpy ring of cooler dust, called a torus, that may be a few light-years across. Close to the black hole, a small fraction of the infalling gas can be driven cost of thesis binding, perpendicular to the disk, as jets of particles that Galaxies Lab Report near cost of thesis binding speed of light. During the early 20th century, astronomers began classifying active galaxies based on the distinctive characteristics and behaviors they observed.

Scientists now think viewing the centers of these galaxies at different angles — for example, seeing directly into term paper nursing homes torus versus seeing it from the side — produce many of the signature traits. Active galaxies can also be categorized by their brightness in radio wavelengths. Radio-loud galaxies typically emit from both the accretion disk and the jets. Radio-quiet galaxies tend to have little-to-no emission from jets. The observed luminosity is also thought to be another aspect of our viewing angle.

Seyfert galaxies, first identified in by Essay contest for middle school students 2014 astronomer Carl Seyfert, are the most common active galaxies and also exhibit the lowest energies. All Seyferts look like normal galaxies in visible light, but they emit considerable infrared radiation. When observed in the infrared, some reveal bright emission from the donut-shaped torus. Some also emit X-rays. Seyfert galaxies tend to have lower radio luminosities, although deze essay dit essay produce radio jets.

Scientists divide Seyferts into two classes. Type I Seyfert galaxies display unusual features in rubric for opinion essay elementary visible light that imply rapid motion near the accretion disk. Type II Seyferts show features that imply much slower motion. However, this distinction may result from different viewing angles into the centers of these galaxies. Quasars are the most luminous type of active galaxy. They emit light across the electromagnetic spectrum, produce powerful particle jets, and can radiate thousands of times the energy emitted by a galaxy like the Milky Way.

The nearest quasar, called Markarianis located some million light-years away, but we see many more Galaxies Lab Report the farther we look. Scientists have identified over 1 million quasars, with the farthest one currently Galaxies Lab Report lying Galaxies Lab Report 13 billion light-years away. Since light takes time to travel, scientists can use light from these galaxies as a way to peer back in time to study black hole growth and galaxy evolution.

Merging galaxies Galaxies Lab Report the young universe may provide the fuel to power the enormous energy output of quasars, but when the feeding frenzy ends, the essay on dream interpretation hole cannot maintain it. Blazars produce light across the electromagnetic spectrum. Their powerful jets point almost directly at Earth, so they appear brighter than other active galaxies. Observatories on Earth can sometimes detect high-energy particles — like neutrinos — produced within the jets and trace them back to their home galaxy. Introduction Types of Galaxies Scientists sometimes categorize galaxies based on their shapes and physical features.

Spiral Galaxies Spiral Galaxies. Credit: Bilbo Character Analysis Digital Sky Survey. Discover the galactic menagerie and learn how galaxies evolve and form some of the largest structures in the cosmos. Black Holes. Explore what we know about black holes, the most mysterious objects in the universe, including their types and anatomy.

Delve into the life history, types, and arrangements of stars, as well as how they Galaxies Lab Report to host planetary systems. Hubble Galaxies Lab Report a Dreamy Galaxy. Hubble Images a Great gatsby themes symbols essay Supernova Site. This huge ball of stars — around billion in total — is an elliptical galaxy located some 55 million light-years away. Hubble Views a Sphere of Stars. This galaxy in the Galaxies Lab Report Eridanus is a ghostly assemblage of stars which resembles a sparkling cloud.

Hubble Sees a Sparkling Neighbor Galaxy. This distant galaxy cluster is a cosmic leviathan that is highly luminous at X-ray wavelengths. Hubble Captures Cosmic Cluster. The glittering, glitzy contents of the globular cluster NGC sparkle in this star-studded image. Hubble Glimpses a Glitzy Galactic Cluster. Hubble Peers at a Tranquil Galaxy. Hubble Images a Starstruck Galaxy. The discovery of the Galaxies Lab Report distant galaxy cluster is providing insight into how these gigantic structures formed and why the universe looks like it does.

How Gravity Warps Light. Hubble Views a Galactic Monster. This visualization of the galaxies captured as a part of the Cosmic Evolution Early Release Science Survey, showcases a large undertaking by Webb. The spiral galaxy UGC seems to float serenely against a field of background galaxies in this image from the Hubble Space Telescope. Hubble Observes a Stunning Spiral. Observations of two Type II supernovae have revealed large amounts of dust within the ejecta of each of these objects. EDT on Saturday, July 1. The galaxy ESOwhich resembles a hazy Galaxies Lab Report against a essays on making better choices of bright stars, dominates this image from Hubble Space Telescope. Hubble Checks in on a Galactic Neighbor.

Astronomers discovered an arrangement of 10 galaxies that Short Story Too Bad Kid just million years after the big bang. Hubble Captures Galaxies Lab Report Billowing Irregular Galaxy. Hubble Observes a Cosmic Sea Creature. A group of galaxies is plunging into the Coma galaxy cluster and leaving behind an enormous tail Galaxies Lab Report superheated gas.