HENRIETTA SWAN LEAVITT 1868 – 1921 Celine Saenz. LIFE Born: 4-Jul-1868 Birthplace: Lancaster, MA Died: 12-Dec-1921 Location of death: Cambridge, MA Cause.

Slides:



Advertisements
Similar presentations
Henrietta Swan Leavitt Katy Sternberger The Woman Who Measured the Universe.
Advertisements

The Role of Women in Astronomy Right Here in Huntsville.
E3 – Stellar distances. Parallax Parallax angle.
General Astronomy Spectral Classes.
OPTION E - ASTROPHYSICS E3 Stellar distances Parallax method
NOTES: Cepheid Variable Stars:
A Notable Woman, whose teaching and nursing career helped the community to be a better place, Clara Barton. Janairy & Jocelyn 8-2.
ANNIE JUMP CANNON Born: Dover, Delaware, December 11, 1863 Died: Cambridge, Massachusetts, April 13, 1941.
By Jackson Woodburn and Beth Rosenberg. Born December 11, 1863 in Dover, Delaware Died April 13, 1941 in Cambridge, Massachusetts at age 77 Oldest of.
© 2010 Pearson Education, Inc. Chapter 20 Galaxies and the Foundation of Modern Cosmology.
© 2010 Pearson Education, Inc. Chapter 20 Galaxies and the Foundation of Modern Cosmology.
22 March 2005AST 2010: Chapter 18 1 Celestial Distances.
Stars: Constellations
JOHN STEINBECK “I wonder how many people I’ve looked at all my life and never seen.” -Steinbeck.
John Steinbeck One of our great California writers.
Read the page Turn the page Go back Research and describe the contributions of scientists to our changing understanding of astronomy, including Ptolemy,
Emily Dickinson An American Legacy. By: Glenn Geib Meagan Morrow Savanna Reeves.
Variable Stars: Stepping Stones To The Universe Albert Holm Computer Sciences Corporation & Space Telescope Science Institute, Retired STScI Public Lecture.
OF SIN AND SCARLET The Scarlet Letter Project Christopher Ball Period C-D.
Abigail Adams.
Stars and galaxies. Constellations  Ancient Greeks, Romans and other cultures saw patterns of stars in the sky called constellations  They imagined.
Chapter 27 Hubble’s Law and the Distance Scale Revised 2007.
 Students will be able to determine the size and shape of our galaxy.  Students will be able to distinguish the different kinds of variable stars. 
The Shapley – Curtis Debate 26 Apr 1920 Center of the GalaxyHow big is the universe Nebula vs. GalaxiesAre “nebula” local or distant.
© 2010 Pearson Education, Inc. Chapter 20 Galaxies and the Foundation of Modern Cosmology.
Introduction to Variable Star Astronomy Geng Zhao
His Life and Contributions. A great author is born! Born January 19, 1809 Parents were David and Elizabeth Poe Born in Boston, Massachusetts A brother,
Joseph Rudyard Kipling
The ideas and discoveries about Earth
Sandra Moore Faber Developed Theories on Galaxies including the “Faber-Jackson Law”
Prentice Hall EARTH SCIENCE
Contents Her family and childhood Education Time spent at Roswell Nobel Prize The Cori Ester Awards 1 Awards 2 Death General Conclusion.
Created by D. Miller Period 1.  Jane Austen  Born December 16, 1775  At the Steventon Rectory Hampshire, England.
Unit Tools of Astronomers Telescopes make faraway objects seem closer.
Lecture 1 History of the Milky Way Galileo, Hershel, Kapteyn and others The idea of spiral nebulae as island universes (Kant) The Great Debate of 1920:
Distances in Space This Mini Lesson Will Cover: What units do astronomers use to measure vast distances in space?
Measuring the distance to Galaxies
Esther Forbes By Katie. Her Beginning  Esther Forbes was born on June 28,1891.  She was born in Westboro, Massachusetts.
The Miracle Worker: A play by William Gibson. William Gibson Facts: Born in 1914 in New York City Struggled academically in school Gifted piano player.
George Eliot. Born November 22, 1819 Born November 22, 1819 Mother died of cancer when she was 16 Mother died of cancer when she was 16 Took care of.
The Milky Way – A Classic Spiral Galaxy Here’s the mystery story we’ll unfold… Fuzzy blobs in the sky – new solar systems, or “galaxies”? Observational.
CEPHEIDS. What are Cepheids? Stars that “pulse” and change luminosity Very bright (100,000x luminosity of Sun) Used to measure extreme distances in space.
Sylvia Paths By Michelle McClennen And Steph Farrar.
Chapter 27 Stars and Galaxies Section 1 Characteristics of Stars Notes 27-2.
Chapter 24 Galaxies  Nick Devereux Birr Telescope - Ireland.
Formation of the Universe Mr. Pratt – Earth Science.
SPOTLIGHT ON "Census Taker of the Sky".  She was born in Dover, Delaware. Her father, Wilson Cannon, was a Delaware shipbuilder and state senator. 
Albert A. Michelson By Tina Stumpenhagen.
Mary Cheung YearExperiences 1952 Born in Hong Kong – 1961 ____________by her parents and often __________ the streets – 1973 Lived at the.
Variable Stars & Distance The “Standard Candle”.
M13 CEPHEID VARIABLE STAR - V2 ELVIRA CRUZ-CRUZ UC COSMOS ASTROPHYSICS 24 JULY 2015.
Eudora Welty Project by: Jessica Lineberry. Background: Family Welty was born on April 13, 1909 in Jackson, Mississippi and died on July 23, 2001 in Jackson,
Module P7 L6. Which is Brightest? A glow worm 1 m away... They could both appear to be the same brightness.... or car headlights 1000 m away? The intrinsic.
Math Blast From the Past.
Journal #1  What quality will you most avoid when choosing a future spouse? Why?
EMILY DICKINSON. Early life ■Born December 10, 1830, in Amherst, Massachusetts. ■Her parents were Edward and Emily Dickinson. Her father was a lawyer.
Astronomy- The Original Science
When did she come to the New World?
Chapter 20 Galaxies and the Foundation of Modern Cosmology
Astronomers Who Paved the Way
The European Renaissance
Learning Goals: How do stars differ from moons and planets, and from one another? How does the classification of stars help us understand how they evolve.
Learning Goals: I will:
The Joy Luck Club An Introduction.
25.1 – Properties of Stars – Part II
Astronomy- The Original Science
Homework: Due at Midnight
Jumping genes! Barbara McClintock (1902 – 1992)
Learning Goals: How do stars differ from moons and planets, and from one another? How does the classification of stars help us understand how they evolve.
After Bellwork, Read the FYI on the “Cosmological Distance Ladder” then answer the two questions in your science journal.
Presentation transcript:

HENRIETTA SWAN LEAVITT 1868 – 1921 Celine Saenz

LIFE Born: 4-Jul-1868 Birthplace: Lancaster, MA Died: 12-Dec-1921 Location of death: Cambridge, MA Cause of death: Cancer - Stomach Remains: Buried, Cambridge Cemetery, Cambridge, MA Religion: Congregationalist Occupation: Astronomer

EARLY LIFE Daughter of George Roswell Leavitt and Henrietta Swan Kendrick Sister: Mira Leavitt Brother: Roswell Leavitt Moved to Cleveland Ohio as a child Attended Oberlin College in 1885 Graduated in 1892 from the Society for the Collegiate Instruction for Women Modern day Radcliffe College After college, Leavitt lost her hearing while traveling through America and Europe

CAREER Became a volunteer research assistant at Harvard College Observatory under the astronomer Edward Pickering Researching the measurement of stellar magnitudes After 17 years, Swan was hired as a permanent staff member Paid 30¢ an hour In 1908 she published her results in the Annals of the Astronomical Observatory of Harvard College noting that a few of the variables showed a pattern Brighter ones appeared to have longer periods She confirmed in 1912 That the Cepheid variables with greater intrinsic luminosity did have longer periods That the relationship was quite close and predictable Her discovery is known as the "period-luminosity relationship“ Discovered 1,777 variable stars in the Magellanic Clouds

ACHIEVEMENTS A member of Phi Beta Kappa The American Association of University Women The American Astronomical and Astrophysical Society The American Association for the Advancement of Science An honorary member of the American Association of Variable Star Observers Publications "Periods of 25 Variable Stars in the Small Magellanic Cloud," Harvard College Observatory Circular 173 (1912). "Standard Photographic Magnitudes," Science 30:726 (1909). "1777 Variables in the Magellanic Clouds", Annals of Harvard College Observatory 15: 87 (1908)

DEATH Died of stomach cancer in 1921 at age fifty-three Buried in the Leavitt family plot at Cambridge Cemetery in Cambridge, Massachusetts. The asteroid 5383 Leavitt and the crater Leavitt on the Moon are named after her to honor deaf men and women who have worked as astronomers. "If Henrietta Leavitt had provided the key to determine the size of the cosmos, then it was Edwin Powell Hubble who inserted it in the lock and provided the observations that allowed it to be turned," wrote David H. and Matthew D.H. Clark in their book Measuring the Cosmos. Edwin Hubble himself often said that Leavitt deserved the Nobel Prize for her work Gösta Mittag-Leffler of the Swedish Academy of Sciences tried to nominate her for that prize in 1924 but she had died

“Miss Leavitt inherited, in a somewhat chastened form, the stern virtues of her puritan ancestors. She took life seriously. Her sense of duty, justice, and loyalty was strong. For light amusements she appeared to care little. She was a devoted member of her intimate family circle, unselfishly considerate in her friendships, steadfastly loyal to her principles, and deeply conscientious and sincere in her attachment to her religion and church. She had the happy faculty of appreciating all that was worthy and lovable in others, and was possessed of a nature so full of sunshine that, to her, all of life became beautiful and full of meaning.” Written obituary of Henrietta Swan Leavitt by Solon Bailey

MISS LEAVITT'S STARS “Well, imagine this room full of these women, you know, most of them with their hair up in buns and their dresses buttoned up to the collars, a very Victorian scene. And they're all sitting in this room, and each one is staring at a glass photographic plate. And they're scrutinizing it, trying to measure the brightness of these stars, writing down the numbers in fountain pen in a ledger, doing these calculations. And in the midst of all this, suddenly Henrietta Leavitt notices this pattern; that some of these stars vary in brightness. They pulse like beacons, so every 30 days they go from dim to bright to dim again. And she was studying these variable stars when she suddenly noticed that the brighter the star, the slower it blinked. She figured out that how fast the star was blinking told her how bright it really was. And if you know how bright it really is, you can see how dim it appears to you from the distance of space, and then you can calculate how far away it is.” George Johnson author of Miss Leavitt's Stars: The Untold Story of the Woman Who Discovered How to Measure the Universe

WORKS CITED storyId= swan-leavitt/ itt%2c_Henrietta_Swan% html avitt/Leavitt01.asp /HenriettaLeavitt.html m Miss Leavitt's Stars: The Untold Story of the Woman Who Discovered How to Measure the Universe by George Johnson