is a Canadian-American astronomer, best known for her measurement of the Hubble constant, and as director of the Carnegie Observatories in Pasadena, California, and Las Campanas, Chile. She is now the John & Marion Sullivan University Professor of Astronomy and Astrophysics at the University of Chicago. Her principal research interests are in observational cosmology, focusing on measuring both the current and past expansion rates of the universe, and on characterizing the nature of dark energy.
Find Below Wiki Age, weight, Height, Net Worth as Wikipedia, Husband, There is no question is the most popular & Rising celebrity of all the time. You can know about the net worth Wendy this year and how she spent her expenses. Also find out how she got wealth at the age of 65. She has a kind heart and lovely personality. below you find everything about her.
|Date of Birth||July 17, 1957|
|Birth Day||July 17|
|Age||65 years old|
|Also Known for||Astronomer|
Also Known by the Full name Wendy Laurel Freedman, is a Good Astronomer. She was born on July 17, 1957, in Toronto. is a beautiful and populous city located in Toronto Canada.
Read Also: Mark Drakeford Wiki, Biography, Age, Net Worth, Family, Instagram, Twitter, Social Profiles & More Facts
Wendy Laurel Freedman Net Worth
Wendy Laurel Freedman has a net worth of $1.5 million (Estimated) which she earned from her occupation as Astronomer. Famously known as the Astronomer of Canada. She is seen as one of the most successful Astronomer of all times. Wendy Laurel Freedman Wealth & Primary Source of earning is being a successful Canadian Astronomer.
Wendy entered the career as Astronomer In her early life after completing her formal education..
|Estimated Net Worth in 2022||$0.5 Million to $1.5 Million Approx|
|Previous Year’s Net Worth (2021)||Being Updated|
|Earning in 2021||Not Available|
|Annual Salary||Being Updated|
|Cars Info||Not Available|
Personal Life, Relationships and Dating
Freedman is married to longtime collaborator Barry F. Madore. They have two children.
Born on July 17, 1957, the Astronomer is Probably the most famous person on social media. Wendy is a popular celebrity and social media influencer. With her huge number of social media followers, she frequently shares numerous individual media files for viewers to comment with her massive amount of support from followers across all major social media sites. Affectively interact with and touch her followers. You can scroll down for information about her Social media profiles.
Life Story & Timeline
Asteroid 107638 Wendyfreedman, discovered by David Healy at the Junk Bond Observatory in 2001, was named in her honor. The official naming citation was published by the Minor Planet Center on 6 January 2007 (M.P.C. 58597 ).
Freedman initiated the Giant Magellan Telescope (GMT) Project and served as chair of the board of directors from its inception in 2003 until 2015. GMT is an international consortium of leading universities and science institutions to build a 25-meter optical telescope at the Carnegie Institution for Science’s Las Campanas Observatory in the Chilean Andes. With a primary mirror 80 feet (24 meters) in diameter, the GMT is poised to be the world’s largest ground-based telescope when it is completed. The telescope, which has entered its construction phase and is expected to become fully operational by 2024, will be able to produce images 10 times sharper than those of the Hubble Space Telescope.
Freedman was co-leader of an international team of 30 astronomers to carry out the Hubble Space Telescope Key Project, a program aiming to establish the distance scale of the Universe and measure the current expansion rate, a quantity known as the Hubble constant. This quantity determines the size of the visible universe and is key to determining its age. Over the course of the Key Project, the team measured the distances to 24 galaxies using Cepheid variable stars, and measured the Hubble constant using five independent methods. The project’s researchers, led by Freedman, published their final result in 2001. The work provided a value of the Hubble constant accurate to 10%, resolving a long-standing, factor-of-two debate.
She has received several awards for her contributions to observational cosmology, including a Centennial Lectureship of the American Physical Society (1999), the John P. McGovern Award in Science (2000), the Magellanic Premium Award of the American Philosophical Society (2002) and the Marc Aaronson Lectureship and prize (1994) “in recognition of a decade of fundamental contributions to the areas of the extra galactic distance scale and the stellar populations of galaxies”. In 2009 Freedman was one of three co-recipients of the Gruber Cosmology Prize. She received the 2016 Dannie Heineman Prize for Astrophysics, awarded jointly by the American Institute of Physics and the American Astronomical Society, “for her outstanding contributions and leadership role in using optical and infrared space- and ground-based observations of Cepheid stars, together with innovative analysis techniques, to greatly improve the accuracy of the cosmic distance scale and thereby constrain fundamental cosmological parameters.”
Freedman grew up in a culturally Jewish family in Toronto, the daughter of a medical doctor and a concert pianist. Her early interest in science was kindled by a formative high-school physics class. This led her to the University of Toronto, where she was first a biophysics student, then an astronomy major, receiving her B.Sc. in 1979. She remained at Toronto for her graduate work, receiving a Ph.D. in astronomy and astrophysics in 1984. Joining the Carnegie Observatories in Pasadena, California, as a post-doctoral fellow in 1984, she became a faculty member of the scientific staff three years later as the first woman to join Carnegie’s permanent staff. In 2003 she was named to the Crawford H. Greenewalt Chair and Director of Carnegie Observatories. Freedman’s early work was principally on the Cepheid distance scale.
Wendy Laurel Freedman (born July 17, 1957) is a Canadian-American astronomer, best known for her measurement of the Hubble constant, and as director of the Carnegie Observatories in Pasadena, California, and Las Campanas, Chile. She is now the John & Marion Sullivan University Professor of Astronomy and Astrophysics at The University of Chicago. Her principal research interests are in observational cosmology, focusing on measuring both the current and past expansion rates of the universe, and on characterizing the nature of dark energy.