Karen Masters

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Karen Masters
Karen Masters, astronomer, December 2017.jpg
Born1979 (age 4445)
Alma mater University of Oxford
Organization Haverford College
Known for Astrophysics, formation and evolution, Galaxy Zoo

Karen Masters (born 1979) is an Astrophysicist and Full Professor of Astrophysics in Haverford College [1] , Pennsylvania exploring galaxy formation. She is also the project scientist for the citizen science project Galaxy Zoo, and uses the classifications to study the evolution of galaxies.

Contents

Education

Masters was born in Birmingham and attended King Edward VI College, Nuneaton. [2] She completed a BSc in Physics at the University of Oxford in 2000. [3] She received a PhD in Astronomy from Cornell University in 2005, entitled "Galaxy flows in and around the Local Supercluster", under the supervision of Martha Haynes and Riccardo Giovanelli. [4]

Research

In 2005 Masters moved to Harvard University to work as a postdoctoral researcher with John Huchra on a project to make the most complete map of the local Universe. [5] Masters "unveiled the most complete 3-D map of the local universe (out to a distance of 380 million light-years) ever created" [6] in 2011 at the 218th meeting of the American Astronomical Society. The map was created using data from the Two-Micron All-Sky Survey.

She moved to the Institute of Cosmology and Gravitation at the University of Portsmouth in October 2008. [2] She was appointed the Gruber Foundation IAU Fellow in 2008. [7] In 2010 Masters was awarded a Leverhulme Early Career Fellowship, for a project entitled "Do bars kill spiral galaxies?". [8] She was promoted to Senior Lecturer in 2014 and Associate Professor in 2015. [9] She has been working on extragalactic astronomy, and in 2018 was appointed as Associate Professor at Haverford College in Pennsylvania. [10]

Masters is the Project Spokesperson for the Sloan Digital Sky Survey. [11]

Public engagement

Masters coordinates the research scientists for Galaxy Zoo, a crowd-sourced galaxy classification project. [3] She has appeared on the BBC Sky At Night. [12]

She coordinated the She's An Astronomer page for Galaxy Zoo, collating the stories of women from astronomy. [13] In 2014 Masters won the Women of the Future Award for Science. [14] [15] That year she was listed as one of the BBC's top 100 women. [16]

Related Research Articles

<span class="mw-page-title-main">Extragalactic astronomy</span> Study of astronomical objects outside the Milky Way Galaxy

Extragalactic astronomy is the branch of astronomy concerned with objects outside the Milky Way galaxy. In other words, it is the study of all astronomical objects which are not covered by galactic astronomy.

The following is a timeline of galaxies, clusters of galaxies, and large-scale structure of the universe.

<span class="mw-page-title-main">Sandra Faber</span> American astrophysicist

Sandra Moore Faber is an American astrophysicist known for her research on the evolution of galaxies. She is the University Professor of Astronomy and Astrophysics at the University of California, Santa Cruz, and works at the Lick Observatory. She has made discoveries linking the brightness of galaxies to the speed of stars within them and was the co-discoverer of the Faber–Jackson relation. Faber was also instrumental in designing the Keck telescopes in Hawaii.

<span class="mw-page-title-main">Great Attractor</span> Region of overdensity of galaxies within the local supercluster

The Great Attractor is a region of gravitational attraction in intergalactic space and the apparent central gravitational point of the Laniakea Supercluster of galaxies that includes the Milky Way galaxy, as well as about 100,000 other galaxies.

<span class="mw-page-title-main">Observable universe</span> All of space observable from the Earth at the present

The observable universe is a ball-shaped region of the universe consisting of all matter that can be observed from Earth or its space-based telescopes and exploratory probes at the present time; the electromagnetic radiation from these objects has had time to reach the Solar System and Earth since the beginning of the cosmological expansion. Initially, it was estimated that there may be 2 trillion galaxies in the observable universe. That number was reduced in 2021 to only several hundred billion based on data from New Horizons. Assuming the universe is isotropic, the distance to the edge of the observable universe is roughly the same in every direction. That is, the observable universe is a spherical region centered on the observer. Every location in the universe has its own observable universe, which may or may not overlap with the one centered on Earth.

<span class="mw-page-title-main">Vera Rubin</span> American astronomer (1928–2016)

Vera Florence Cooper Rubin was an American astronomer who pioneered work on galaxy rotation rates. She uncovered the discrepancy between the predicted and observed angular motion of galaxies by studying galactic rotation curves. By identifying the galaxy rotation problem, her work provided evidence for the existence of dark matter. These results were later confirmed over subsequent decades.

Observational cosmology is the study of the structure, the evolution and the origin of the universe through observation, using instruments such as telescopes and cosmic ray detectors.

Richard Brent Tully is a Canadian-born American astronomer at the Institute for Astronomy in Honolulu, Hawaii.

The Sloan Digital Sky Survey or SDSS is a major multi-spectral imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States. The project began in 2000 and was named after the Alfred P. Sloan Foundation, which contributed significant funding.

<span class="mw-page-title-main">Galaxy filament</span> Largest structures in the universe, made of galaxies

In cosmology, galaxy filaments are the largest known structures in the universe, consisting of walls of galactic superclusters. These massive, thread-like formations can commonly reach 50/h to 80/h Megaparsecs —with the largest found to date being the Hercules-Corona Borealis Great Wall at around 3 gigaparsecs (9.8 Gly) in length—and form the boundaries between voids. Due to the accelerating expansion of the universe, the individual clusters of gravitationally bound galaxies that make up galaxy filaments are moving away from each other at an accelerated rate; in the far future they will dissolve.

<span class="mw-page-title-main">Heidi Jo Newberg</span> American astrophysicist

Heidi Jo Newberg is an American astrophysicist known for her work in understanding the structure of our Milky Way galaxy. Among her team's findings are that the Milky Way is cannibalizing stars from smaller galaxies and that the Milky Way is larger and has more ripples than was previously understood. She is a founding participant in the Sloan Digital Sky Survey (SDSS) and the Sloan Extension for Galactic Understanding and Exploration (SEGUE), and is a leader of the astrophysical MilkyWay@home volunteer computing project team. She is a professor in the Department of Physics, Applied Physics, and Astronomy at Rensselaer Polytechnic Institute (RPI) in Troy, New York, US, and a Fellow of the American Physical Society.

In cosmology, baryon acoustic oscillations (BAO) are fluctuations in the density of the visible baryonic matter of the universe, caused by acoustic density waves in the primordial plasma of the early universe. In the same way that supernovae provide a "standard candle" for astronomical observations, BAO matter clustering provides a "standard ruler" for length scale in cosmology. The length of this standard ruler is given by the maximum distance the acoustic waves could travel in the primordial plasma before the plasma cooled to the point where it became neutral atoms, which stopped the expansion of the plasma density waves, "freezing" them into place. The length of this standard ruler can be measured by looking at the large scale structure of matter using astronomical surveys. BAO measurements help cosmologists understand more about the nature of dark energy by constraining cosmological parameters.

<span class="mw-page-title-main">Laniakea Supercluster</span> Galaxy supercluster that is home to the Milky Way Galaxy and many more galaxies

The Laniakea Supercluster is the galaxy supercluster that is home to the Milky Way and approximately 100,000 other nearby galaxies.

<span class="mw-page-title-main">Beth Willman</span> American astronomer

Beth Willman is an American astronomer who is the Chief Executive Officer of the LSST Discovery Alliance, an astronomical organization notable for its support of the Vera C. Rubin Observatory. She was previously the deputy director of the National Optical-Infrared Astronomy Research Laboratory (NOIRLab) and an associate professor of astronomy at Haverford College.

<span class="mw-page-title-main">BOSS Great Wall</span> One of the largest superstructures in the observable universe

The BOSS Great Wall is a supercluster complex that was identified, using the Baryon Oscillation Spectroscopic Survey (BOSS) of the Sloan Digital Sky Survey (SDSS), in early 2016. It was discovered by a research team from several institutions, consisting of: Heidi Lietzen, Elmo Tempel, Lauri Juhan Liivamägi, Antonio Montero-Dorta, Maret Einasto, Alina Streblyanska, Claudia Maraston, Jose Alberto Rubiño-Martín and Enn Saar. The BOSS Great Wall is one of the largest superstructures in the observable universe, though there are even larger structures known.

<span class="mw-page-title-main">Saraswati Supercluster</span> Supercluster of galaxies in the Pisces constellation

The Saraswati Supercluster is a massive galaxy supercluster about 1.2 gigaparsecs (4 billion light years) away within the Stripe 82 region of SDSS, in the direction of the constellation Pisces. It is one of the largest structures found in the universe, with a major axis in diameter of about 200 Mpc (652 million light years). It consists of at least 43 galaxy clusters, and has the mass of 2 × 1016 M, forming a galaxy filament.

<span class="mw-page-title-main">NGC 4586</span> Spiral galaxy in the constellation Virgo

NGC 4586 is a spiral galaxy located about 50 million light-years away in the constellation Virgo. The galaxy was discovered by astronomer William Herschel on February 2, 1786. Although listed in the Virgo Cluster Catalog, NGC 4586 is considered to be a member of the Virgo II Groups which form a southern extension of the Virgo cluster. NGC 4586 is currently in the process of infalling into the Virgo Cluster and is predicted to enter the cluster in about 500 million years.

<span class="mw-page-title-main">Hyperion proto-supercluster</span> Galaxy cluster in the constellation Sextans

The Hyperion proto-supercluster is the largest and earliest known proto-supercluster, 5,000 times the mass of the Milky Way and seen at 20% of the current age of the universe. It was discovered in 2018 by analysing the redshifts of 10,000 objects observed with the Very Large Telescope in Chile.

<span class="mw-page-title-main">NGC 3925</span> Galaxy in the constellation Leo

NGC 3925 is a barred lenticular galaxy and a ring galaxy located about 370 million light-years away in the constellation Leo. It was discovered by astronomer Heinrich d'Arrest on February 19, 1863.

Daniel Pomarède is a staff scientist at the Institute of Research into the Fundamental Laws of the Universe, CEA Paris-Saclay University. He co-discovered Laniakea, our home supercluster of galaxies, and Ho'oleilana, a spherical shell-like structure 1 billion light-years in diameter found in the distribution of galaxies, possibly the remnant of a Baryon Acoustic Oscillation. Specialized in data visualization and cosmography, a branch of cosmology dedicated to mapping the Universe, he also co-authored the discoveries of the Dipole Repeller and of the Cold Spot Repeller, two large influential cosmic voids, and the discovery of the South Pole Wall, a large-scale structure located in the direction of the south celestial pole beyond the southern frontiers of Laniakea.

References

  1. "FacultyKaren Masters". Haverford College. Retrieved 27 May 2024.
  2. 1 2 "She's an Astronomer: Karen Masters". Galaxy Zoo. 2 November 2009. Retrieved 5 January 2018.
  3. 1 2 "Wadham College Alumni: Karen Masters". University of Oxford. Retrieved 5 January 2018.
  4. Masters, Karen Louise (2005). "Galaxy flows in and around the Local Supercluster". Ph.D. Thesis. Bibcode:2005PhDT.........2M.
  5. "Karen Masters". The Conversation. 24 April 2013. Retrieved 5 January 2018.
  6. "Astronomers unveil the most complete 3-D map of the local universe". Smithsonian Insider. 25 May 2011. Retrieved 5 January 2018.
  7. "2008 Gruber Cosmology Prize Press Release | The Gruber Foundation". gruber.yale.edu. Retrieved 5 January 2018.
  8. "Karen Masters - Portsmouth Research Portal". researchportal.port.ac.uk. Archived from the original on 6 January 2018. Retrieved 5 January 2018.
  9. "Karen Masters". www.icg.port.ac.uk. Retrieved 5 January 2018.
  10. "Haverford Welcomes Six New Faculty Members" . Retrieved 5 January 2018.
  11. "SDSS Key Personnel". www.sdss.org. Retrieved 8 December 2019.
  12. "Secrets of the Whirlpool Galaxy, The Sky at Night - BBC Four". BBC. Retrieved 5 January 2018.
  13. "She's An Astronomer | Galaxy Zoo". blog.galaxyzoo.org. Retrieved 5 January 2018.
  14. Massey, Robert. "Dr Karen Masters wins Women of the Future award". www.ras.org.uk. Retrieved 5 January 2018.
  15. "The Future is Now: Karen Masters Wins UK Award | Science Blog from the SDSS". blog.sdss.org. Retrieved 5 January 2018.
  16. "Who are the 100 Women 2014?". BBC News. 26 October 2014. Retrieved 5 January 2018.