https://sputnikglobe.com/20230724/astrophysicists-discover-striking-two-faced-white-dwarf-1112122801.html
Astrophysicists Discover Striking 'Two-Faced' White Dwarf
Astrophysicists Discover Striking 'Two-Faced' White Dwarf
Sputnik International
This finding challenges previous theories about the evolution of white dwarfs and raises questions about why this particular star has such drastically different faces.
2023-07-24T23:22+0000
2023-07-24T23:22+0000
2023-07-24T23:19+0000
beyond politics
science & tech
space
space exploration
white dwarf stars
white dwarf
https://cdn1.img.sputnikglobe.com/img/07e7/07/18/1112122644_0:0:1600:900_1920x0_80_0_0_2f79e519f92f2b1b962a4ee42d5187a4.jpg
Astronomers have been left stumped and riddled with questions after discovering that at least one white dwarf exhibits a two-faced nature, with one side composed of hydrogen and the other made up of helium.Lead researcher Ilaria Caiazzo, a postdoctoral scholar at Caltech, describes the white dwarf's transformation from one side to the other as a complete surface change. The unique white dwarf, named Janus after the two-faced Roman god, was initially detected by the Zwicky Transient Facility. The celestial body's rapid changes in brightness caught Caiazzo's attention, which then prompted a further investigation using the CHIMERA instrument at Caltech's Palomar Observatory and the HiPERCAM on the Gran Telescopio Canarias in Spain's Canary Islands. The results confirmed that Janus rotates on its axis every 15 minutes.Subsequent observations made with the W. M. Keck Observatory in Hawaiʻi revealed the dramatic duality of the white dwarf. The team used a spectrometer to analyze the light and found that when one side of Janus was in view, it consisted predominantly of hydrogen, with no signs of helium, whereas the other side showed only helium.Researchers have put forward several theories to explain this unusual phenomenon. One theory suggests Janus may be undergoing a rare phase of white dwarf evolution, where some white dwarfs transition from being hydrogen- to helium-dominated on their surface.As white dwarfs cool over time, heavier elements sink to their cores and lighter elements, such as hydrogen, rise to the top. However, the question remains as to why this transition is happening in such an asymmetrical manner, with one side evolving before the other.The team also speculates magnetic fields play a crucial role in Janus' unique characteristic.Another theory proposes that magnetic fields may alter the pressure and density of the atmospheric gases, leading to the observed differences.Further research and observations are needed to unravel the mysteries behind Janus and determine the factors responsible for its distinct faces. The discovery opens up new avenues for understanding the complex evolution of white dwarfs and the role that magnetic fields play in shaping celestial objects.The findings of the study were published in the journal Nature.
https://sputnikglobe.com/20230717/cannibal-coronal-mass-ejection-to-hit-earth-tuesday-cause-geomagnetic-storm-1111951993.html
Sputnik International
feedback@sputniknews.com
+74956456601
MIA „Rossiya Segodnya“
2023
News
en_EN
Sputnik International
feedback@sputniknews.com
+74956456601
MIA „Rossiya Segodnya“
Sputnik International
feedback@sputniknews.com
+74956456601
MIA „Rossiya Segodnya“
white dwarf, what are the best known white dwarfs, what is white dwarf, the evolution of white dwarfs, white dwarfs stars, latest space discoveries, what is known about white dwarfs, astrophysicists discovered
white dwarf, what are the best known white dwarfs, what is white dwarf, the evolution of white dwarfs, white dwarfs stars, latest space discoveries, what is known about white dwarfs, astrophysicists discovered
Astrophysicists Discover Striking 'Two-Faced' White Dwarf
A recent groundbreaking discovery surrounding white dwarf stars has challenged previous theories about the evolution of such celestial bodies, raising questions about why this particular star can have drastically different faces.
Astronomers have been left stumped and riddled with questions after discovering that at least one white dwarf exhibits a two-faced nature, with one side composed of hydrogen and the other made up of helium.
Lead researcher Ilaria Caiazzo, a postdoctoral scholar at Caltech, describes the white dwarf's transformation from one side to the other as a complete surface change.
"The surface of the white dwarf completely changes from one side to the other," said Caiazzo. "When I show the observations to people, they are blown away."
The unique white dwarf, named Janus after the two-faced Roman god, was initially detected by the Zwicky Transient Facility.
White dwarfs are formed during the evolution of stars whose mass is insufficient to become neutron stars, namely not exceeding about 10 solar masses.
Passing the stage of a red giant star sheds the outer shell, and the former core of the star becomes a white dwarf consisting of carbon and oxygen.
The celestial body's rapid changes in brightness caught Caiazzo's attention, which then prompted a further investigation using the CHIMERA instrument at Caltech's Palomar Observatory and the HiPERCAM on the Gran Telescopio Canarias in Spain's Canary Islands. The results confirmed that Janus rotates on its axis every 15 minutes.
Subsequent observations made with the W. M. Keck Observatory in Hawaiʻi revealed the dramatic duality of the white dwarf. The team used a spectrometer to analyze the light and found that when one side of Janus was in view, it consisted predominantly of hydrogen, with no signs of helium, whereas the other side showed only helium.
Researchers have put forward several theories to explain this unusual phenomenon. One theory suggests Janus may be undergoing a rare phase of white dwarf evolution, where some white dwarfs transition from being hydrogen- to helium-dominated on their surface.
As white dwarfs cool over time, heavier elements sink to their cores and lighter elements, such as hydrogen, rise to the top. However, the question remains as to why this transition is happening in such an asymmetrical manner, with one side evolving before the other.
The team also speculates magnetic fields play a crucial role in Janus' unique characteristic.
"Magnetic fields can prevent the mixing of materials. So, if the magnetic field is stronger on one side, then that side would have less mixing and thus more hydrogen," explained Caiazzo.
Another theory proposes that magnetic fields may alter the pressure and density of the atmospheric gases, leading to the observed differences.
Further research and observations are needed to unravel the mysteries behind Janus and determine the factors responsible for its distinct faces. The discovery opens up new avenues for understanding the complex evolution of white dwarfs and the role that magnetic fields play in shaping celestial objects.
The findings of the study were published in the journal
Nature.
