Tag

Astrometry

All articles tagged with #astrometry

Hubble and Webb reveal Omega Centauri's hidden stellar-mass black hole after 23-year hunt
space1 month ago

Hubble and Webb reveal Omega Centauri's hidden stellar-mass black hole after 23-year hunt

Astronomers using two decades of precise astrometry from NASA's Hubble Space Telescope and the James Webb Space Telescope have identified the first stellar-mass black hole in the Milky Way's Omega Centauri, named oMEGACat BH-2, by tracking a visible star's sky motion around an unseen companion. The binary completes an orbit every 94 years, and the black hole weighs about 4.46 solar masses, confirming a black hole rather than a neutron star. The system likely formed through dynamical interactions in the cluster; this discovery supports Omega Centauri's hidden black-hole population and points to more finds as Hubble, Webb, and future missions survey the cluster.

Omega Centauri's 94-Year Binary Unveils Its First Stellar-Mass Black Hole
science1 month ago

Omega Centauri's 94-Year Binary Unveils Its First Stellar-Mass Black Hole

Astronomers using two decades of Hubble imagery and JWST data have identified the first stellar-mass black hole in the globular cluster Omega Centauri, designated oMEGACat BH-2, weighing about 4.46 solar masses and in a 94-year orbit around a sun-like star — the longest-period black hole binary yet found. The discovery, based on precise astrometry of stellar wobble, supports the existence of a hidden population of black holes in metal-poor clusters, though the period and mass have uncertainties due to partial orbital coverage; further observations with JWST and upcoming missions will refine the parameters and reveal more such systems.

Omega Centauri Unveils Its First Hidden Stellar-Mass Black Hole
space1 month ago

Omega Centauri Unveils Its First Hidden Stellar-Mass Black Hole

Astronomers using over two decades of Hubble data and JWST observations have confirmed the first stellar-mass black hole in the Omega Centauri globular cluster, designated oMEGACat BH-2, with a mass of 4.46 solar masses orbiting a sun-like star every 94 years. The finding suggests Omega Centauri could host a large hidden population of such black holes and highlights astrometry as a key method, with plans to find more using Roman Space Telescope in the future.

Astronomers uncover first stellar-mass black hole in Omega Centauri with Hubble and Webb
science1 month ago

Astronomers uncover first stellar-mass black hole in Omega Centauri with Hubble and Webb

University of Utah researchers used two decades of Hubble data and recent JWST observations to measure stellar motions via astrometry, revealing Omega Centauri’s first stellar-mass black hole, oMEGACat BH-2, with a mass of about 4.46 solar masses and a 94-year orbit—the longest known for a black hole binary. The discovery in this metal-poor globular cluster challenges existing formation theories and suggests such black hole populations may be common, with future surveys (including NASA’s Roman Space Telescope) likely to find more.

Roman Space Telescope Could Weigh Hidden Neutron Stars via Gravitational Microlensing
science3 months ago

Roman Space Telescope Could Weigh Hidden Neutron Stars via Gravitational Microlensing

NASA’s Nancy Grace Roman Space Telescope could spot and weigh isolated neutron stars in the Milky Way using astrometric microlensing in its Galactic Bulge Time Domain Survey; by tracking tiny shifts in background starlight as a neutron star passes in front, Roman can directly measure the masses of otherwise invisible remnants, helping map the neutron star–black hole population and shedding light on neutron-star birth kicks, with even a few detections significantly advancing stellar evolution models.

Colossal exomoon candidate could redefine the meaning of 'moon'
space7 months ago

Colossal exomoon candidate could redefine the meaning of 'moon'

Astronomers using the GRAVITY instrument on the VLT detected a small but measurable wobble in the gas giant HD 206893 B’s orbit, implying a massive unseen companion — an exomoon potentially about 40% of Jupiter’s mass (roughly nine Neptune masses) orbiting at ~0.2 AU with a ~9‑month period and a ~60° inclination. If confirmed, it would be among the most massive moons known and could force a reevaluation of what defines a moon, while guiding future exomoon searches via astrometry.

"Gaia Discovers New Tidal Stellar Stream"
astronomy2 years ago

"Gaia Discovers New Tidal Stellar Stream"

Chinese astronomers have used data from ESA's Gaia satellite to discover a new tidal stellar stream in the northern hemisphere of the Milky Way, characterized by low metallicity and high energy. The stream, approximately 80 degrees long and 1.7 degrees wide, was found at a high Galactic latitude and is associated with the merging event Sequoia. Further studies, particularly spectroscopic observations, are needed to better understand this newly detected stellar stream and its properties, with implications for the potential discovery of more such structures in the galaxy.

Gaia's Quest: Searching for Another Earth
space-science2 years ago

Gaia's Quest: Searching for Another Earth

The European Space Agency's Gaia mission, which aims to map over one billion stars in the Milky Way, has the potential to detect Earth-like planets up to 30 light-years away using astrometry. Gaia's astrometry method allows for more accurate determination of an exoplanet's orbital parameters and can detect planets far away from their host stars. If advanced astrometry precision is achieved, Gaia could detect the four giant planets in our solar system within 100 years. Additionally, over 300 stars within ten parsecs from our solar system could potentially detect Earth if they achieve microarcsecond accuracy. The possibility of extraterrestrial intelligences (ETIs) using similar technology to Gaia raises the question of whether they could discover planets in our solar system, including Earth.

astronomy3 years ago

"Newly Discovered Exoplanet Resembles a Younger Version of Jupiter"

Scientists at the University of Texas at Austin have used astrometry to directly capture images of AF Lep b, one of the lowest-mass planets ever observed. This groundbreaking technique could revolutionize the discovery of extrasolar planets that are challenging to detect due to their distance, mass, or orientation relative to Earth. AF Lep b is approximately three times the mass of Jupiter and orbits a young Sun-like star about 87.5 light-years away. The combination of direct imaging and astrometry allows for the identification of previously difficult-to-detect extrasolar planets and enables the direct measurement of a planet's mass. The researchers plan to further study AF Lep b using advanced telescopes.

"Revolutionary Exoplanet Discoveries: Young Jupiter's Sibling and Eclipsing Cataclysmic Variable System Unveiled"
astronomy3 years ago

"Revolutionary Exoplanet Discoveries: Young Jupiter's Sibling and Eclipsing Cataclysmic Variable System Unveiled"

Astronomers using the W. M. Keck Observatory have successfully captured direct images of AF Lep b, one of the lowest-mass planets, using the astrometry technique. This marks the first time astrometry has been used to detect a giant planet orbiting a young Sun-like star. AF Lep b is approximately three times the mass of Jupiter and orbits a young star about 87.5 light-years away. This breakthrough could revolutionize the discovery of extrasolar planets that are challenging to detect due to their distance, mass, or orientation relative to Earth.

astronomy3 years ago

"Stunning Discovery: Young Planet Mirrors Jupiter's Features"

Astronomers have discovered a young exoplanet, AF Lep b, using the astrometry method, which involves measuring tiny changes in a star's position caused by the gravitational tugs of an orbiting planet. This is the first time astrometry has been used to find a giant planet orbiting a young star similar to the Sun. The team also used direct imaging to confirm the planet's existence and determine its mass, distance from its star, and orbital eccentricity. Further observations and studies of AF Lep b will be conducted using advanced telescopes like the James Webb Space Telescope.

'Jupiter's Younger Sibling' Marks Start of Exoplanet Discovery Era
astronomy3 years ago

'Jupiter's Younger Sibling' Marks Start of Exoplanet Discovery Era

Astronomers using the W. M. Keck Observatory in Hawaii have directly captured images of AF Lep b, one of the lowest-mass planets ever discovered. The planet is about three times the mass of Jupiter and orbits a young sun-like star about 87.5 light-years away. The discovery was made using a technique called astrometry, which measures the subtle movements of a host star over many years to help astronomers determine whether hard-to-see orbiting companions, including planets, are gravitationally tugging at it. This new method of combining direct imaging with astrometry could help astronomers find extrasolar planets that were hard to find before with other methods.