London: In a new study, astronomers have identified two white dwarf stars considered to be the oldest and closest known to man.
A University of Oklahoma assistant professor and colleagues identified these 11-12-billion-year-old white dwarf stars only 100 light years away from Earth.
According to the OU researcher, these stars are the closest known examples of the oldest stars in the Universe forming soon after the Big Bang.
Mukremin Kilic, assistant professor of physics and astronomy in the OU College of Arts and Sciences and lead author on a recently published paper, announced the discovery.
“A white dwarf is like a hot stove; once the stove is off, it cools slowly over time. By measuring how cool the stove is, we can tell how long it has been off. The two stars we identified have been cooling for billions of years,” Kilic said.
Kilic explained that white dwarf stars are the burned out cores of stars similar to the Sun. In about 5 billion years, the Sun also will burn out and turn into a white dwarf star. It will lose its outer layers as it dies and turn into an incredibly dense star the size of Earth.
Known as WD 0346+246 and SDSS J110217, 48+411315.4 (J1102), these stars are located in the constellations Taurus and Ursa Major, respectively.
Kilic and colleagues obtained infrared images using NASA’s Spitzer Space Telescope to measure the temperature of the stars. And, over a three-year period, they measured J1102’s distance by tracking its motion using the MDM Observatory’s 2.4m telescope near Tucson, Arizona.
“Most stars stay almost perfectly fixed in the sky, but J1102 is moving at a speed of 600,000 miles per hour and is a little more than 100 light years from Earth,” John Thorstensen, co-author of the study from Dartmouth College, said.
“We found its distance by measuring a tiny wiggle in its path caused by the Earth’s motion—it’s the size of a dime viewed from 80 miles away,” he said.
Piotr Kowalski of Helmholtz Centre Potsdam in Germany modelled the atmospheric parameters of these stars. Based on these temperature measurements, Kilic and his colleagues were able to estimate the ages of the stars.
“Based on the optical and infrared observations of these stars and our analysis, these stars are about 3700 and 3800 degrees on the surface,” Kowalski, co-author of the study, said.
The study will be published in the Monthly Notices of the Royal Astronomical Society.
A University of Oklahoma assistant professor and colleagues identified these 11-12-billion-year-old white dwarf stars only 100 light years away from Earth.
According to the OU researcher, these stars are the closest known examples of the oldest stars in the Universe forming soon after the Big Bang.
Mukremin Kilic, assistant professor of physics and astronomy in the OU College of Arts and Sciences and lead author on a recently published paper, announced the discovery.
“A white dwarf is like a hot stove; once the stove is off, it cools slowly over time. By measuring how cool the stove is, we can tell how long it has been off. The two stars we identified have been cooling for billions of years,” Kilic said.
Kilic explained that white dwarf stars are the burned out cores of stars similar to the Sun. In about 5 billion years, the Sun also will burn out and turn into a white dwarf star. It will lose its outer layers as it dies and turn into an incredibly dense star the size of Earth.
Kilic and colleagues obtained infrared images using NASA’s Spitzer Space Telescope to measure the temperature
“We found its distance by measuring a tiny wiggle in its path caused by the Earth’s motion—it’s the size of a dime viewed from 80 miles away,” he said.
Piotr Kowalski of Helmholtz Centre Potsdam in Germany modelled the atmospheric parameters of these stars. Based on these temperature measurements, Kilic and his colleagues were able to estimate the ages of the stars.
“Based on the optical and infrared observations of these stars and our analysis, these stars are about 3700 and 3800 degrees on the surface,” Kowalski, co-author of the study, said.
The study will be published in the Monthly Notices of the Royal Astronomical Society.
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