AstroUnit

For the first time, a giant exoplanet has been discovered orbiting a dead star (which in this case happens to a white dwarf) every 1.4 days. The planet is roughly the same size as Jupiter and is no more than 14 times as massive and has an equilibrium temperature of 165 K. The mass of the white dwarf is approximately 0.5 solar masses and with the radius roughly 10% that of the Sun. The groundbreaking discovery demonstrated that giant planets can be scattered into tight orbits without being tidally disrupted, and motivates searches for smaller transiting planets around white dwarfs. NGC 2392: A planetary nebula, a phase that results when a star like the Sun becomes a red giant and sheds its outer layers. Source:  Chandra Exoplanet research is clearly amongst the most interesting research topics in astronomy. With the advancement of high-quality telescopes and detectors, thousands of exoplanets have been discovered and the numbers are only projected to surge in the coming years. Normally,

A large team of astronomers discovered the first asteroid inside the orbit of Venus using the Zwicky Transient Facility  located at the Palomar Observatory in California, United States. The asteroid has been named 2020 AV2 and is roughly 2 km in size with an aphelion distance (i.e., the point in the orbit of an object where it is farthest from the Sun ) of 0.65 astronomical units. The discovery could very well indicate that there may be a yet undiscovered population of asteroid lying outside of the asteroid belt and if more such asteroids are discovered,  currently favored asteroid population models may need to be adjusted. Image of the largest asteroid Ceres. Source  Wikipedia As of this writing, almost all of  1 million known asteroids  lie between the orbits of Mars and Jupiter with only a handful lying near the orbit of Earth.  Many scientists argue that there must be another population of asteroids present near the orbit of Venus. However, no such asteroids have been detected unt

Astronomers J. Scholtz and J. Unwin in a new study investigated the anomalous orbits of trans-Neptunian objects (TNOs) and excess in microlensing events using the 5-year Optical Gravitational Lensing Experiment (OGLE) and came to the conclusion that these gravitational anomalies can be explained if a tiny primordial black hole with a mass few times that of the Earth were to be lurking in the outskirts of the Solar System. According to the leading Planet 9 hypothesis, it is believed that a super Earth-sized rogue planet must be present to shepherd the orbits of the TNOs. However, the new study suggested that the probability of the Sun capturing a primordial black hole is comparable to the capturing of a rogue planet and suggested ways by which the scenario could be verified or falsified.    An Artist's illustration of the Solar system. Credit:  pixel4k Until now, two distinct but seemingly interconnected gravitational anomalies have been detected with no consensus regarding its sour

Have you ever wondered what is the biggest structure in our Universe? Well, the answer is the Hercules–Corona Borealis Great Wall. It's so massive that it takes light approximately 10 billion (10,000,000,000) years to cross it. It was first detected in 2013 by a team of astronomers while analyzing data from the Swift Gamma-Ray Burst Mission, together with other data from ground-based telescopes. Now, a new study using advanced statistical tools offered arguments that suggest that the structure may not be real and speculated about its potential origin.  This enormous image shows Hubble’s view of the massive galaxy cluster MACS J0717.5+3745. Credit:  NASA, ESA, Harald Ebeling (the University of Hawaii at Manoa) & Jean-Paul Kneib (LAM) The Hercules–Corona Borealis Great Wall is by far the largest structure in the observable Universe inferred from the clustering of gamma-ray bursts. The length of this structure is roughly 10% of the entire Universe. The structure lies in the conste

On May 21, 2019, at 03:02:29 UTC the Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo collaboration observed a short duration of the gravitational-wave signal, named GW190521. The detected signal is consistent with the merger of two black holes with masses of 85 and 66 solar masses. The mass of the remnant black hole is estimated to be around 142 solar masses, which makes the historic event GW190521 the first observational confirmation for the existence of an intermediate-mass black hole (IMBH).  Artist's impression of binary black holes about to collide. Source:  Caltech Black holes can be grouped into 4 categories depending on their masses. Firstly, there are the supermassive black holes that reside exclusively at the heart of galaxies having masses in the range from a few million to billions of solar masses. Then there are  the intermediate-mass black holes having masses between a hundred to a few thousands of solar masses. Next are  the stellar-mass black ho

A team of astronomers made a groundbreaking discovery of six closely bound galaxies being powered by a single supermassive black hole with a mass greater than a billion solar masses at a redshift of 6.31. Out of the six galaxies, four are massive star-forming galaxies and the other two are comparatively low mass galaxies. This is the first discovery of a galactic overdensity around a supermassive black hole in the first billion years of the Universe and confirms the idea that the most distant and massive black holes form and grow within massive dark matter halos in large scale structures.   MS 0735.6+7421: Six objects ranging in location from within the Milky Way to billions of light-years away: Source:  Chandra One of the major challenges in astronomy is to explain the existence of supermassive black holes powering luminous quasars at high redshifts. A quasar is an extremely bright active galactic nucleus fueled by a supermassive black hole. Quasars are typical of the size of our sola

 A new study proposed an interesting and robust test that can be used to infer the origin of solar mass black holes. Solar mass black holes are not expected to form from the conventional stellar evolution but can be produced naturally via neutron star (NS) implosions from the capture of small primordial black holes (PBHs) or from the accumulation of dark matter (DM). The study reports that the mass distribution of such solar-mass BHs would be similar to that of the NSs. This would differ from the mass distribution of black holes in the solar-mass range predicted either by conventional stellar evolution or early universe PBH production.  An artist's impression of IGR J17091-3624: The stellar-mass black hole with the fastest Wind. Source:  Chandra Solar mass black holes should not be confused with stellar-mass black holes. A stellar-mass black hole is a black hole formed by the gravitational collapse of a star. They have masses between 5 to several tens of solar masses and have been

A team of astronomers has discovered a new exoplanet named TOI-824 b orbiting a nearby star TOI-824 which is only 208 light-years away from us. The planet is massive in size with a mass equivalent to almost 19 times that of the Earth and has a radius equal to 3 times that of the Earth. The planet has an orbital period of 1.393 days and has a mean density of roughly 4 gm/cc making it more than twice as dense as Neptune. The discovery was made using data from the Transiting Exoplanet Survey Satellite (TESS).                        An artist’s impression of an exoplanet. Source:  Alpha Coders As the name suggests, an exoplanet is a planet outside the solar system. The first confirmed detection of an exoplanet was made in 1992 by astronomers Aleksander Wolszczan and Dale Frail. On 6 October 1995, Michel Mayor and Didier Queloz discovered the first exoplanet orbiting a Sun-like star. This discovery was groundbreaking and opened a new area of research in observational astronomy. For their di