Universe Is Expanding “Great Debate” Resolved Dr

Total Page:16

File Type:pdf, Size:1020Kb

Universe Is Expanding “Great Debate” Resolved Dr National Aeronautics and Space Administration Age of the Universe: Size of the Universe: 2 Billion Years Cosmic Times 280 Million Light Years 1929 Andromeda Nebula Lies Universe is Expanding “Great Debate” Resolved Dr. Hubble’s discovery settles the “Great “Red Shift” is Proof of Einstein’s General Theory Debate” over the size of our own Milky Way Galaxy and the distance to, and nature of, spiral Outside Milky Way Galaxy Using the 100-inch Hooker Telescope at Although Hubble’s work presents a tremen­ nebulae. Mount Wilson Observatory, Dr. Edwin Powell dous breakthrough in our understanding of the Held on April 26, 1920 at the National Acad­ Spiral Nebulae are indeed “Island Universes” Hubble has studied a variety of spiral nebulae universe, one big question remains. How far out emy of Sciences in Washington, D.C., the de­ and established that they are moving away from into the universe does his model hold? The 100­ bate focused on the opposing views of astrono­ us at a rapid pace – strong evidence of an expand­ inch telescope can resolve Cepheids in only the mers Dr. Harlow Shapley of the Mount Wilson ing universe. He has further determined that the nearest nebulae. In nebulae where Cepheids are Observatory and Dr. Heber D. Curtis at the Uni­ speed of motion increases with greater distance. barely visible, Hubble has identified the most versity of California’s Lick Observatory. Hubble and his colleague Milton Humason luminous individual stars, some 50 to 100 times Shapley’s studies had led him to a concept of measured the radial velocities and distances of brighter than the Cepheids. He uses these lumi­ the Milky Way as an enormous galaxy of stars twenty-four of these nebulae. Because they are nous stars as standard candles for more distant some 300,000 light years across, much larger moving so quickly, their light waves are stretched objects. than most previous estimates. His model also out. This shifts their energy signals – as we detect But today’s telescopes, and the stars they see, held that the Solar System is far from the gal­ them – toward the red end of the electromagnetic will only take Hubble so far. To measure even axy’s center and that all nebulae, including spi­ spectrum, a phenomenon known as “redshift.” greater distances, astronomers will need a larger ral nebulae, are within the confines of the Milky The team noticed that dimmer, more distant ob­ telescope and new types of standard candles. Way. Citing photographic surveys done at the jects have a larger redshift than objects closer to One new instrument may hold the key. Last Lick Observatory, Curtis put forth his idea that Earth. As reported in a recent paper, Hubble’s year the Rockefeller Foundation agreed to pro­ spiral nebulae were “island universes,” distant measurements led him to a useful velocity-dis­ vide the six million dollars needed to fund the star systems similar to the Milky Way and not tance relationship: redshifts increase in direct construction of a new observatory with a 200­ outlying components of it. He also believed the proportion to their distance from us. inch telescope. When completed, this telescope Milky Way was less than 30,000 light years in Hubble’s initial analysis reveals that for ev­ will hold four times the light-gathering power of diameter and 8,000 light years in thickness. ery million parsecs of distance, the velocity of the instrument Hubble currently uses. Hubble’s recent observations vindicate Cur­ the spiral nebulae increases by approximately tis’ views. While bright, diffuse nebulae are at 300 miles per second, where one parsec is equal Einstein’s General Theory Holds True relatively close distances and part of the Milky to 3.26 light years. He determined distances to Way, spiral nebulae are separate systems at great the nebulae using Cepheid variables, stars with The past decade has been an exciting and distances from it. He estimates that the spiral An­ challenging time in the development of scien­ dromeda Nebula is as large and holds as much tific understanding of the universe, with theo­ matter as the Milky Way. However, Hubble’s rists testing their ideas against the framework of findings also support Shapley’s general view of Albert Einstein’s 1916 theory of general relativ­ the Milky Way’s size, with the Solar System lo­ ity. The theory establishes the universe as three cated far from its center. Courtesy of the Carnegie Institution dimensions of space and one of time. It proposes Shapley’s work had increased the size of the Dr. Edwin Hubble found that the Andromeda nebula is the most distant object known and is not part of the Milky that gravity curves the fabric of space-time and universe by about ten times, but Hubble’s recent Way Galaxy. that the curvature controls the natural motions discoveries have multiplied it by at least another ten. Shapley observed a historical progression, of bodies in space. Astronomer Edwin Powell Hubble, of the directly related to their average brightness: the from belief in a small universe with man at its His theory also pointed to the expansion of the Mount Wilson Observatory of the Carnegie longer the period, the brighter the star. The Small center, to a larger one with Earth further from universe, but Dr. Einstein has rejected the idea. Institution at Pasadena, California, has solved Magellanic Cloud (SMC) is a massive aggregate the center: “The significance of man and the the mystery of the spiral nebulae, the great of stars visible in the southern hemisphere, and In 1917 he added a new term to his equations, Earth…has dwindled with advancing knowl­ heavenly objects that appear as hazy pin-wheels since all of these stars were in the SMC, they Hubble’s research led to this diagram, showing the gen- the “cosmological constant,” designed specifi­ edge of the physical world…” in the sky. He has determined that these objects were at roughly the same distance from the eral correlation between how far away a galaxy is and cally to avoid the implication of an expanding are much more distant than previously thought Earth. Each Cepheid’s intrinsic brightness was the speed it is moving away from us. universe. Hubble’s recent observations dismiss and therefore are galaxies themselves, rather directly related to its period. the need for such a term, but while Einstein has than part of our own Milky Way Galaxy. In the Soon after Miss Leavitt’s discovery, Shapley a known luminosity, or “standard candles.” He examined the data and believes Hubble’s paper process, Dr. Hubble was also able to determine began systematically searching for Cepheids in concluded that the most distant objects are speed­ to be sound, he is still not convinced. the distance to the spiral Andromeda nebula. globular clusters in the Milky Way galaxy, globes ing away from us at perhaps thousands of miles In 1922, Soviet physicist Alexander Fried­ Classifying Nebulae Hubble’s observations vindicate the views of tens of thousands of densely-packed stars. per second. man developed his own solutions to the general of Dr. Heber Curtis expressed in the “Great He used the period-luminosity relationship to For over a thousand years, astronomers Hubble’s recent discoveries reveal that the relativity equations. He described two possibili­ have speculated on the nature and evolution Debate” with Dr. Harlow Shapley at the 1920 determine the distance to more than 230 globular volume of space itself is expanding. Spiral nebu­ ties for the universe: either it was expanding or of nebulae, faint clouds of gas and dust in the National Academy of Sciences (see “‘Great clusters. On the assumption that Cepheids in lae appear to be moving away from each other at contracting, but it was not static. distant universe. However, until recently, there Debate’ Resolved” article). Curtis maintained distant globular clusters obey the same physics a rate that increases with distance, but these neb­ Abbe George Lemaître, a Belgian-born have been insufficient observations to allow a that bright diffuse nebulae are relatively close to as nearby Cepheids, he found that the most ulae aren’t just moving. They are being pulled Catholic priest and astronomer, released a paper classification of nebulae based on their features Earth and are part of the Milky Way, while spiral distant clusters reside some 200,000 light years along as the fabric of space-time expands. in 1927 stating that a homogeneous universe of or qualities. nebulae are at great distances and not part of the away. Dr. Hubble, during his studies of the spiral Milky Way. By studying the periods of the Cepheids in Hubble’s findings build on the work of Dr. Ves­ constant mass has to be expanding to account nebulae, proposed a system to classify all On December 30, 1924, Hubble announced the Andromeda Nebula (M31), Hubble was to M. Slipher of Lowell Observatory in Flagstaff, for the radial velocity of spiral nebulae. He de­ nebulae, both inside and outside the Milky that he had taken photographic plates of a few able to determine each variable’s intrinsic Arizona, who in 1912 became the first to record scribed a possible universe that was expanding Way. He sorted them into three basic categories: bright spiral nebulae with Mount Wilson’s brightness, its absolute magnitude. He then made the electromagnetic spectra of a spiral nebula. Of from its initial state as a single point. Lemaître elliptical, spiral, and irregular. These, in turn, Hooker telescope, the largest reflecting telescope observations of the apparent magnitude of every the more than forty spectra Slipher subsequently believed that before this expansion began, the were further subdivided according to shape in the world.
Recommended publications
  • Astronomy 142, Spring 2013 2 April 2013
    Astronomy 142, Spring 2013 2 April 2013 Today in Astronomy 142: distances to the galaxies Standard candles and standard rulers. Cepheids, and Henrietta Leavitt’s invention of standard candles. The extragal acti c nature of the spiral nebulae and the Shapley-Curtis debate. Type Ia supernovae as standard candles. The extragalactic distance The Small Magellanic Cloud, site of the scale. discovery of Leavitt’s Law. (Photograph by Weihao Wang (NRAO).) 2 April 2013 Astronomy 142, Spring 2013 1 Standard candles and standard rulers There’s only one direct distance measurement method for individual objects more than a few light-hours away – trig parallax – and it only works on objects within a few hundred parsecs, these days. (> 10 kpc, after Gaia is deployed.) Distance being key, astronomers have often sought standard candles or rulers to aid in its determination. Standard candle: an object with a well-determined luminosity L known a priori, whose distance is therefore rLf4(or equivalently 5log r10 pc mM ) . Standard ruler: an object with length d perpendicular to the line of sight is known a priori, whose distance is rdsin d . 2 April 2013 Astronomy 142, Spring 2013 2 Henrietta Leavitt and standard candles Today tens of thousands of Cepheid variable stars are known, a large fraction of which – about 2400 – were discovered by Henrietta Leavitt, perhaps the most illustrious of the women Henrietta Swan Leavitt (AIP photo) who worked as “computers” in Edward Pickering’s group at Harvard College Observatory. 969 of them are in the Small Magellanic Cloud (Leavitt 1908), and therefore all about the same distance (~60 kpc).
    [Show full text]
  • AAS NEWSLETTER Issue 127 a Publication for the Members of the American Astronomical Society
    October 2005 AAS NEWSLETTER Issue 127 A Publication for the members of the American Astronomical Society PRESIDENT’S COLUMN know that Henrietta Swan Leavitt measured the Cepheid variable stars in the Magellanic Clouds Robert Kirshner, [email protected] to establish the period-luminosity relation, and that Inside this rung on the distance ladder let Hubble reach As I write this, summer is definitely winding down, M31 and other nearby galaxies. And I recognized George Johnson’s name from his thoughtful pieces 3 and the signs of Fall on a college campus are all in the New York Times science pages. Who Served Us Well: around: urgent overtime work on the last licks of John N. Bahcall summer renovations is underway, vast piles of trash and treasure from cleaning out dorm rooms are But I confess, though I walk on the streets where accumulating, with vigorous competitive double- she lived, work in a building connected by a 5 parking of heavily-laden minivans just ahead. With labyrinth to the one she worked in, and stand on Katrina Affected the Galaxy overhead most of the night, and the the distance ladder every day, my cerebral cortex Physics and summer monsoon in progress in Arizona, the pace is a little short on retrievable biographical details Astronomy (KAPA) of supernova studies slackens just a bit (for me, for Henrietta Swan Leavitt. Johnson has plumbed Community Bulletin anyway) and I had time to do a little summer reading. the Harvard archives, local census records, and the correspondence of Harvard College Board There were too many mosquitoes in Maine to read in a hammock, but there was enough light on the Observatory Directors to give us a portrait of screened porch.
    [Show full text]
  • Ira Sprague Bowen Papers, 1940-1973
    http://oac.cdlib.org/findaid/ark:/13030/tf2p300278 No online items Inventory of the Ira Sprague Bowen Papers, 1940-1973 Processed by Ronald S. Brashear; machine-readable finding aid created by Gabriela A. Montoya Manuscripts Department The Huntington Library 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2203 Fax: (626) 449-5720 Email: [email protected] URL: http://www.huntington.org/huntingtonlibrary.aspx?id=554 © 1998 The Huntington Library. All rights reserved. Observatories of the Carnegie Institution of Washington Collection Inventory of the Ira Sprague 1 Bowen Papers, 1940-1973 Observatories of the Carnegie Institution of Washington Collection Inventory of the Ira Sprague Bowen Paper, 1940-1973 The Huntington Library San Marino, California Contact Information Manuscripts Department The Huntington Library 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2203 Fax: (626) 449-5720 Email: [email protected] URL: http://www.huntington.org/huntingtonlibrary.aspx?id=554 Processed by: Ronald S. Brashear Encoded by: Gabriela A. Montoya © 1998 The Huntington Library. All rights reserved. Descriptive Summary Title: Ira Sprague Bowen Papers, Date (inclusive): 1940-1973 Creator: Bowen, Ira Sprague Extent: Approximately 29,000 pieces in 88 boxes Repository: The Huntington Library San Marino, California 91108 Language: English. Provenance Placed on permanent deposit in the Huntington Library by the Observatories of the Carnegie Institution of Washington Collection. This was done in 1989 as part of a letter of agreement (dated November 5, 1987) between the Huntington and the Carnegie Observatories. The papers have yet to be officially accessioned. Cataloging of the papers was completed in 1989 prior to their transfer to the Huntington.
    [Show full text]
  • Edwin Powell Hubble Papers: Finding Aid
    http://oac.cdlib.org/findaid/ark:/13030/tf7b69n8rd Online items available Edwin Powell Hubble Papers: Finding Aid Processed by Ronald S. Brashear, completed December 12, 1997; machine-readable finding aid created by Xiuzhi Zhou and updated by Diann Benti in June 2017. The Huntington Library, Art Collections, and Botanical Gardens Manuscripts Department 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2191 Email: [email protected] URL: http://www.huntington.org © 1998 The Huntington Library. All rights reserved. Edwin Powell Hubble Papers: mssHUB 1-1098 1 Finding Aid Overview of the Collection Title: Edwin Powell Hubble Papers Dates (inclusive): 1900-1989 Collection Number: mssHUB 1-1098 Creator: Hubble, Edwin, 1889-1953. Extent: 1300 pieces, plus ephemera in 34 boxes Repository: The Huntington Library, Art Collections, and Botanical Gardens. Manuscripts Department 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2191 Email: [email protected] URL: http://www.huntington.org Abstract: This collection contains the papers of Edwin P. Hubble (1889-1953), an astronomer at the Mount Wilson Observatory near Pasadena, California. as well as the diaries and biographical memoirs of his wife, Grace Burke Hubble. Language: English. Access Open to qualified researchers by prior application through the Reader Services Department. For more information, contact Reader Services. Publication Rights The Huntington Library does not require that researchers request permission to quote from or publish images of this material, nor does it charge fees for such activities. The responsibility for identifying the copyright holder, if there is one, and obtaining necessary permissions rests with the researcher. Preferred Citation [Identification of item].
    [Show full text]
  • E F L E C T I O
    SUMMER . QUARTER / JUNE . 2 0 1 6 r eflections the universe expanded here Realuminizing the 100-inch Mirror On Friday, May 27, the 100-inch glass was stripped of its old aluminum coating and prepped for a new covering in ARKIMOVICH the Observatory’s aluminization chamber. The procedure NIK is described by Observatory Director Tom Meneghini as “a fairly Herculean undertaking.” Observatory staff has located a photograph of Dr. John Strong and Dr. Enrique Gaviola of Caltech inspecting the surface of the 100-inch mirror coated with aluminum in- stead of the “customary silver.” Although the photograph appears to be undated, it was most likely 1935, for this was the year that the 100-inch mirror lost its silver coat- ing and was recoated with aluminum in a new vacuum chamber designed by Dr. Strong and built in the Carnegie prepared for a new aluminum coating. The bare 100-inch (it is actually Observatories’ machine shops on Santa Barbara Street in 101 inches) mirror, with its layers, bubbles, swirls, and cavities, in a prepared Pasadena. condition for a new aluminum coating. According to Milton Humason in his article entitled “The Aluminizing of the 100-inch and 60-inch Reflectors of the Mount Wilson Observatory” (Publications of the Astronomical Society of the Pacific, vol. 47, no. 276, April 1935), Dr. Strong’s method of aluminizing glass, pyrex, or quartz disks by the evaporation pro- cess was developed so rapidly that “it has recently been possible to aluminize successfully both the 100-inch and 60-inch reflectors of the Mount Wilson Observatory.” to page 5 In this issue ..
    [Show full text]
  • The 100-Inch Telescope of the Mount Wilson Observatory
    The 100-Inch Telescope of the Mount Wilson Observatory An International Historical Mechanical Engineering Landmark The American Society of Mechanical Engineers June 20, 1981 Mount Wilson Observatory Mount Wilson, California BACKGROUND THE MOUNT WILSON OBSERVATORY was founded in 1904 by the CARNEGIE INSTITUTION OF WASH- INGTON, a private foundation for scientific research supported largely from endowments provided by Andrew Carnegie. Within a few years, the Observatory became the world center of research in the new science of astrophysics, which is the application of principles of physics to astronomical objects beyond the earth. These include the sun, the planets of our solar system, the stars in our galaxy, and the system of galaxies that reaches to the limits of the The completed facility. visible universe. SCIENTIFIC ACHIEVEMENTS The Mount Wilson 100-inch reflector dominated dis- coveries in astronomy from its beginning in 1918 until the dedication of the Palomar 200-inch reflector in 1948. (Both telescopes are primarily the result of the lifework of one man — George Ellery Hale.) Many of the foundations of modern astrophysics were set down by work with this telescope. One of the most important results was the discovery that the intrinsic luminosities (total light output) of the stars could be found by inspection of the record made when starlight is dispersed into a spectrum by a prism or a grating. These so-called spectroscopic absolute lumi- nosities, discovered at Mount Wilson and developed for over forty years, opened the way to an understanding of the evolution of the stars and eventually to their ages. Perhaps the most important scientific discovery of the 20th century is that we live in an expanding Universe.
    [Show full text]
  • Throughout the Universe, Galaxies Are Rushing Away from Us – and from Each Other – at Tremendously High Speeds
    Our Universe Began with a Bang Throughout the Universe, galaxies are rushing away from us – and from each other – at tremendously high speeds. This fact tells us that the Universe is expanding over time. Edwin Hubble (after whom the Hubble Space Telescope was named) first measured the expansion in 1929. Observatories of the Carnegie Institution of Washington Edwin Hubble This posed a big question. If we could run the cosmic movie backward in time, would everything in the Universe be crammed together in a blazing fireball – the starting point of Edwin Hubble & Proceedings of The National Academy of Sciences Hubble’s famous diagram showing the the Big Bang? A lot of scientific distance versus velocity of the galaxies he debate and many new theories observed. The farther away the galaxies, the faster they are moving, showing that the followed Hubble’s discovery. Universe is expanding. Among those in the front lines of the debate were physicists Ralph Alpher and Robert Herman. In 1948 they predicted that an afterglow of this fireball should still exist, though at a much lower temperature than at the time of the Big Bang. Here’s why: As the Universe Fun Fact: expands, the waves of heat About radiation from the Big Bang are 1% of the stretched out, and cool from “snow” you see visible energy to infrared and on broadcast TV then to microwave wavelengths. is caused by the Microwaves are just short- cosmic microwave wavelength radio waves, the same background. form of energy used in microwave ovens. The prediction of an afterglow could be tested! Scientists began building instruments to detect this “cosmic microwave background”, or CMB.
    [Show full text]
  • Student Exploration: Big Bang Theory – Hubble's
    McCarthy Physical Science 2017 Name: Date: Student Exploration: Big Bang Theory – Hubble’s Law Vocabulary: absolute brightness, absorption spectrum, apparent brightness, Big Bang theory, blueshift, Cepheid variable, Doppler shift, Hubble constant, Hubble’s law, luminosity, megaparsec, period, redshift, spectrograph Prior Knowledge Questions (Do these BEFORE using the Gizmo.) Standing by the side of a lonely highway at night, you see two motorcycle headlights, one in each direction. The headlight on your left appears brighter than the one on your right. 1. If the headlights are equally bright, which motorcycle is closer? Explain: 2. Suppose the dim-looking headlight on the right is actually a small light on the front of a bicycle. What can you conclude about the distance of the motorcycle and bicycle? Gizmo Warm-up In 1912, an astronomer named Henrietta Swan Leavitt studied a class of stars called Cepheid variables. These stars change from bright to dim to bright again. Her discoveries led to a method of measuring distances to other galaxies and eventually helped to support the Big Bang theory of the origin of the universe. In the Big Bang Theory – Hubble’s Law Gizmo™, select Region A. Look at the image of the Andromeda Galaxy, a galaxy relatively close to our own Milky Way galaxy. 1. Locate the two Cepheid variables, the stars that change in brightness over time. Star A-091 is the yellow star, and A-171 is the white star. A. Which star reaches a greater apparent brightness? B. Which star takes longer to pulse? 2. Because both stars are in the same galaxy, they are about the same distance from Earth.
    [Show full text]
  • 00:00 [Narrator] 1. the NASA/ESA Hubble Space Telescope Is Named After the Famous Astronomer Edwin Hubble. He Discovered That T
    Keywords: Distances, Cepheids, Henrietta Leavitt Hubblecast Episode 116: Henrietta Leavitt — the woman Visual notes ​ who measured the Universe 00:00 [Narrator] 1. The NASA/ESA Hubble Space Telescope is named after the famous astronomer Edwin Hubble. He discovered that there are galaxies outside of our own and that the Universe is expanding. However, these remarkable discoveries wouldn’t have been possible without one exceptional astronomer before him — Henrietta Swan Leavitt. 00:30 2. Henrietta Leavitt — the woman who measured the Universe 00:40 [Narrator] 3. Henrietta Leavitt was born in Lancaster, Massachusetts in 1868. She studied at Oberlin College, Ohio, and then Harvard University's Society for the Collegiate Instruction of Women. It wasn’t until her final year at university that she began to study astronomy — but this sparked a keen interest that she would pursue for the rest of her life. 01:10 4.She began to work at Harvard Observatory as a “computer” — one of several skilled women hired to process astronomical data. She helped with cataloguing the brightness of every measurable star and was quickly promoted to be head of the photographic stellar photometry department. 01:34 5. Supplied with photographic plates of the stars in the southern sky, Leavitt was tasked with classifying variable stars — ones that fluctuate in brightness. 01:47 6. While studying these changing stars she noticed a pattern: the brighter the star, the longer the period of the fluctuations. The easily measured length of the star’s fluctuations directly leads to its brightness — and to its distance. The observation of these Cepheid variables turned out to be the key to a fundamental change in our understanding of the Universe.
    [Show full text]
  • Chapter I Review Papers Harlow Shapley
    Chapter I Review Papers Harlow Shapley Downloaded from https://www.cambridge.org/core. IP address: 170.106.40.40, on 25 Sep 2021 at 08:30:59, subject to the Cambridge Core terms of use, available at https://www.cambridge.org/core/terms. https://doi.org/10.1017/S0074180900042340 Helen Sawyer Hogg and Willis Shapley remembering Willis Shapley fielding questions on his father Downloaded from https://www.cambridge.org/core. IP address: 170.106.40.40, on 25 Sep 2021 at 08:30:59, subject to the Cambridge Core terms of use, available at https://www.cambridge.org/core/terms. https://doi.org/10.1017/S0074180900042340 SHAPLEY'S DEBATE Michael Hoskin Cambridge University The attempt to make three-dimensional sense of the Milky Way goes back to a most unlikely origin: the English antiquary of the early eighteenth century, William Stukeley, remembered today for associating the Druids with Stonehenge. Stukeley came from Lincolnshire and so was a fellow-countryman of Isaac Newton, and as a result he was privileged to talk with the great man from time to time. In his Memoirs of Newton Stukeley records one conversation they had in about 1720, in which Stukeley proposed that the Sun and the brightest stars of the night sky make up what we today would term a globular cluster, and this cluster is surrounded by a gap, outside of which lie the small stars of the Milky Way in the form of a flattened ring. Stukeley's remarkable suggestion was recorded only in his manuscript memoirs, and had no effect on the subsequent history of astronomy.
    [Show full text]
  • Our Milky Way.Key
    Our Milky Way Learning Objectives ! What is the Milky Way? The Herschels thought we were at the center of our Galaxy...why were they wrong? ! How did Shapley prove we aren’t at the center? What are globular clusters? Cepheid Variable stars? ! How do we use Cepheid Variables to measure distance? ! What are the components of our Galaxy? What color are old stars? Young stars? Does our Galaxy get older or younger as you move out (i.e. from the disk to the halo)? ! How do we know our Galaxy is a spiral galaxy? ! Do stars in our Galaxy’s disk orbit as Kepler’s Laws would predict? What is a rotation curve? Why does our Galaxy’s rotation curve suggest dark matter exists? The Milky Way ! Our Galaxy is a collection of stars, nebulae, molecular clouds, and stellar remnants ! All bound together by gravity ! Connected by the stellar evolution cycle Determining the Shape of our Galaxy ! The number of 6400 ly stars were counted in all directions from 1300 ly the Sun by Sun Caroline Herschel and her brother William ! They assumed that all stars have the same brightness and that space contains no dust – these are incorrect assumptions ! They thus concluded that the Sun is at the center of the Universe - which is not true The Importance of Dust ! Dust dims and reddens starlight ! There is more dust toward the center of the Galaxy ! Consequence: We underestimate the number of stars in one direction ! We appear to be near the center, but we’re not Us Star Sun Can’t see stars here (if we’re looking for blue light from them) How Do We Find the Galactic Center?
    [Show full text]
  • At the Harvard Observatory
    Book Reviews 117 gravitational wave physicists, all of whom are members of an international group of over a thousand scientists engaged with the detection apparatus at two widely separated sites, one in Livingston, Louisiana and the other in Hanford, Washington. The emails research- ers in the collaboration exchanged and the queries Collins sent to the physicists who acted for him as “key informants” provide the bulk of the material for Collins’ “real- time” observations of this discovery in the making. At times, Collins finds the community of researchers exasperating and wrong-headed in their, in his view, overly secretive attitudes to their results. But Collins is not a detached witness of the events he describes and analyses. Instead, he is overall a highly enthusias- tic fan of the gravitational wave community. Collins has not sought out for Gravity’s Kiss the kinds of evidence one might have expected a historian to have pursued. Gravity’s Kiss, however, should be read on its terms. It is a work of reportage from an “embedded” sociologist of science with long experience of, and valuable connections in, the gravitational wave community. Along the way, he offers sharp insights into the work- ing of these scientists. Collins proves to be an excellent guide to the operations of a “Big Science” collaboration and the intense scrutiny of, and complicated negotiations around, the “[v]ery interesting event on ER8.” Robert W. Smith University of Alberta [email protected] “Girl-Hours” at the Harvard Observatory The Glass Universe: How the Ladies of the Harvard Observatory Took the Measure of the Stars.
    [Show full text]