Nia Imara | |
---|---|
Born | |
Alma mater | Kenyon College (BA) University of California, Berkeley (PhD) |
Known for | Science and art |
Scientific career | |
Institutions | UC Santa Cruz Center for Astrophysics | Harvard & Smithsonian |
Thesis | The Formation and Evolution of Giant Molecular Clouds (2010) |
Doctoral advisor | Leo Blitz |
Website | niaimara |
Nia Imara is an American astrophysicist, artist, and activist. Imara's scientific work deals with galactic mass, star formation, and exoplanet detection. Imara was the first African-American woman to earn a PhD in astrophysics at the University of California, Berkeley [1] and was the inaugural postdoctoral fellow in the Future Faculty Leaders program at Harvard University. [2] In 2020, Imara joined the University of California, Santa Cruz as an assistant professor in the Department of Astronomy. [3] Her recent work includes 3D-printing models to aid visualization of molecular clouds.
Imara was born in East Oakland, Oakland, California and grew up in the San Francisco Bay Area. [4] She received her bachelor's degree from Kenyon College in 2003, [5] majoring in mathematics and physics. [4] While at Kenyon College, she competed on the college's swim team. [6] She moved to the University of California, Berkeley for her postgraduate studies, and in 2010 she became the first African-American woman to earn a PhD in astrophysics at University of California, Berkeley. [4] Her dissertation was on The Formation and Evolution of Giant Molecular Clouds and was supervised by Leo Blitz. [7]
From 2014 to 2017, Imara was the inaugural postdoctoral fellow in the Future Faculty Leaders program at Harvard University. Her postdoctoral research focused on giant molecular clouds, the birth sites of stars, and the properties and cosmological effects of galactic and intergalactic dust. [2] She used the world's largest fully steerable radio telescope, the Robert C. Byrd Green Bank Telescope, to conduct her research. [4]
In 2017, she was appointed as the John Harvard Distinguished Science Fellow and the Harvard FAS Dean's Postdoctoral Fellow at the Harvard–Smithsonian Center for Astrophysics. [8] Imara works with the Banneker Institute at Harvard, and is a member of the Breakthrough Starshot research team. [9] [10] Her work investigates the structure and evolution of stellar nurseries in both the Milky Way Galaxy and other galaxies throughout the universe, [11] and she has developed a model that connects galaxy mass, star formation rates and dust temperatures. [12]
In fall 2020, Imara joined the faculty in the Astronomy and Astrophysics Department at the University of California, Santa Cruz.
Together with Rosanne Di Stefano, Imara proposed a method for detecting exoplanets in X-ray binary star systems. [13] Imara, Di Stefano, and their other collaborators found evidence, using the Chandra X-Ray Observatory, of a potential planet passing in front of a star that is 28 million light-years away in the M51 galaxy. [14] Their findings were published to Nature Astronomy in an October 2021 paper entitled "A possible planet candidate in an external galaxy detected through X-ray transit." [15] If the findings are confirmed, this would represent the first sighting of a planet outside of our Milky Way Galaxy. [16]
To help visualize molecular clouds, Imara has developed a way to use "high-resolution bitmap-based three-dimensional (3D) printing" to create handheld models for teaching and outreach. [17] These models, according to CNET , are "polished, baseball-size orbs that look like oversized marbles with swirling patterns inside." [18] Models in 3D are better than 2D images because, says Imara, "when we’re looking at a flat picture, we often can’t tell how far a certain structure extends into the depth of the cloud. But when we have a tool like this 3D-printed object, it’s inherently interactive, and we can see a structure sort of winding its way through the cloud." [19]
Imara is an advocate for equity in STEM. She founded the Equity and Inclusion Journal Club at Harvard University in 2018 which was originally co-organized with Dr. Anna Pancoast. [20] She has visited South Africa and Ghana to teach and advocate in programs designed to increase diversity in astronomy and other STEM areas. [21] [22]
In 2020, Imara founded Onaketa, an organization that connects students from underserved communities of color with free math and science tutoring. [23] [24]
Imara has described the field of astronomy as a uniquely powerful tool for engaging the general public with, and expanding access to, science: "Everyone’s captivated by astronomy, by the stars, what’s out there in the universe...And so I made a conscious choice a long time ago that I wanted to share my work with the community, with Black folks and other people of color, especially.” [23] Imara recently appeared as herself in the "Age of Stars" episode of the 2021 PBS Nova documentary series "Universe Revealed," [25] as well as a short segment in Ancient Skies "Gods and Monsters" (TV Episode 2019). [26]
A molecular cloud, sometimes called a stellar nursery (if star formation is occurring within), is a type of interstellar cloud, the density and size of which permit absorption nebulae, the formation of molecules (most commonly molecular hydrogen, H2), and the formation of H II regions. This is in contrast to other areas of the interstellar medium that contain predominantly ionized gas.
An open cluster is a type of star cluster made of tens to a few thousand stars that were formed from the same giant molecular cloud and have roughly the same age. More than 1,100 open clusters have been discovered within the Milky Way galaxy, and many more are thought to exist. They are loosely bound by mutual gravitational attraction and become disrupted by close encounters with other clusters and clouds of gas as they orbit the Galactic Center. This can result in a loss of cluster members through internal close encounters and a dispersion into the main body of the galaxy. Open clusters generally survive for a few hundred million years, with the most massive ones surviving for a few billion years. In contrast, the more massive globular clusters of stars exert a stronger gravitational attraction on their members, and can survive for longer. Open clusters have been found only in spiral and irregular galaxies, in which active star formation is occurring.
Astronomy is a natural science that studies celestial objects and the phenomena that occur in the cosmos. It uses mathematics, physics, and chemistry in order to explain their origin and their overall evolution. Objects of interest include planets, moons, stars, nebulae, galaxies, meteoroids, asteroids, and comets. Relevant phenomena include supernova explosions, gamma ray bursts, quasars, blazars, pulsars, and cosmic microwave background radiation. More generally, astronomy studies everything that originates beyond Earth's atmosphere. Cosmology is a branch of astronomy that studies the universe as a whole.
Astrophysics is a science that employs the methods and principles of physics and chemistry in the study of astronomical objects and phenomena. As one of the founders of the discipline, James Keeler, said, Astrophysics "seeks to ascertain the nature of the heavenly bodies, rather than their positions or motions in space–what they are, rather than where they are." Among the subjects studied are the Sun, other stars, galaxies, extrasolar planets, the interstellar medium and the cosmic microwave background. Emissions from these objects are examined across all parts of the electromagnetic spectrum, and the properties examined include luminosity, density, temperature, and chemical composition. Because astrophysics is a very broad subject, astrophysicists apply concepts and methods from many disciplines of physics, including classical mechanics, electromagnetism, statistical mechanics, thermodynamics, quantum mechanics, relativity, nuclear and particle physics, and atomic and molecular physics.
Christopher Fulton McKee is an astrophysicist.
The Local Bubble, or Local Cavity, is a relative cavity in the interstellar medium (ISM) of the Orion Arm in the Milky Way. It contains the closest of celestial neighbours and among others, the Local Interstellar Cloud, the neighbouring G-Cloud, the Ursa Major moving group and the Hyades. It is estimated to be at least 1000 light years in size, and is defined by its neutral-hydrogen density of about 0.05 atoms/cm3, or approximately one tenth of the average for the ISM in the Milky Way (0.5 atoms/cm3), and one sixth that of the Local Interstellar Cloud (0.3 atoms/cm3).
The following outline is provided as an overview of and topical guide to astronomy:
Frank Hsia-San Shu was a Chinese-American astrophysicist, astronomer, and author. He served as a Professor Emeritus at the University of California, Berkeley and University of California, San Diego. He is best known for proposing the density wave theory to explain the structure of spiral galaxies, and for describing a model of star formation, where a giant dense molecular cloud collapses to form a star.
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Atomic astrophysics is concerned with performing atomic physics calculations that will be useful to astronomers and using atomic data to interpret astronomical observations. Atomic physics plays a key role in astrophysics as astronomers' only information about a particular object comes through the light that it emits, and this light arises through atomic transitions.
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. Our bitmap-based 3D printing approach thus faithfully reproduces the subtle density gradient distribution within molecular clouds in a tangible, intuitive, and visually stunning manner. While laying the groundwork for the intuitive analysis of other structurally complex astronomical data sets, our 3D-printed models also serve as valuable tools in educational and public outreach endeavors.
The models are made from opaque resin deposited inside transparent resin, which makes it look like the cosmic clouds are suspended within each globe. The researchers also made half-spheres that give a view into the cross sections of the nurseries.
Then she casts the data into baseball-size spheres of resin with a 3D printer — layer by layer, each one-third the thickness of a sheet of paper. These sculptures of stellar ultrasounds have helped Imara study the processes guiding star formation more intimately than ever before.
Astrophysicist and artist Nia Imara founded Onaketa...