All The Gravitational Waves Detected So Far

Few events in the astronomy community were received with more fanfare than the first detection of gravitational waves, which took place on September 14th, 2015.  Since then, different events have been recorded using the same techniques.  Many include data from other observational platforms, as the events that normally create gravitational waves are of interest to almost everyone in the astronomical community.  Black hole and neutron star mergers and the like provide a plethora of data to understand the physics that happen under such extreme conditions.

To distribute that data equitably, researchers at LIGO, one of the main observatories for gravitational waves, have released a data set that contains information about all 50 confirmed gravitational wave events that have taken place since observations began.  What’s more, a team from the Cardiff University made a tool that makes it much easier to navigate the data.  

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China’s Planning to Launch a Space-Based Gravitational Wave Observatory in the 2030s: TianQin. Here’s how it’ll Stack up Against LISA

Artist's impression of the Laser Interferometer Space Antenna (LISA). Credit: ESA

The successful detection of gravitational waves has been a game-changer for astronomy. And now the new frontier is in space, with satellite-based detection systems currently in development that will uncover some of the universe’s biggest mysteries. And while the team behind LISA is now developing that observatory in space, it just may be outclassed by a rival, TianQin, developed by the Chinese.

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The Kilonova-Chasing Gravitational-Wave Optical Transient Observer is About to be Watching the Whole Sky

Lately there has been a flood of interest in gravitational waves.  After the first official detection at LIGO / Virgo in 2015, data has been coming in showing how common these once theoretical phenomena actually are.  Usually they are caused by unimaginably violent events, such as a merging pair of black holes.  Such events also have a tendency to emit another type of phenomena – light.  So far it has been difficult to observe any optical associated with these gravitational-wave emitting events.  But a team of researchers hope to change that with the full implementation of the Gravitation-wave Optical Transient Observer (GOTO) telescope.

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Black Holes Make Complex Gravitational-Wave Chirps as They Merge

Simulated merger of two black holes. Credit: NASA's Goddard Space Flight Center

Gravitational waves are produced by all moving masses, from the Earth’s wobble around the Sun to your motion as you go about your daily life. But at the moment, those gravitational waves are too small to be observed. Gravitational observatories such as LIGO and VIRGO can only see the strong gravitational waves produced by merging stellar-mass black holes.

The chirp of a gravitational merger is clear. Credit: LIGO/Caltech/MIT/University of Chicago (Ben Farr)
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Behold! The Black Hole Collision Calculator!

This image shows two massive black holes in the OJ 287 galaxy. The smaller black hole orbits the larger one, which is also surrounded by a disk of gas. When the smaller black hole crashes through the disk, it produces a flare brighter than 1 trillion stars. Credit: NASA/JPL-Caltech

Black holes have been the subject of intense interest ever since scientists began speculating about their existence. Originally proposed in the early 20th century as a consequence of Einstein’s Theory of General Relativity, black holes became a mainstream subject a few decades later. By 1971, the first physical evidence of black holes was found and by 2016, the existence of gravitational waves was confirmed for the first time.

This discovery touched off a new era in astrophysics, letting people know collision between massive objects (black holes and/or neutron stars) creates ripples in spacetime that can be detected light-years away. To give people a sense of how profound these events are, Álvaro Díez created the Black Hole Collision Calculator (BHCC) – a tool that lets you see what the outcome of a collision between a black hole and any astronomical object would be!

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Gravitational waves could show what’s happening inside a star as it’s going supernova

A 2-D snapshot of a pair-instability supernovae as the explosion waves are about to break through the star's surface. The tiny disturbances represent fluid instability - in a region where different elements interact and mix. Image Credit: ASIAA/Ken Chen

It’s kind of hard to see inside a star as it’s blowing up, because of the whole “blowing up” part, but gravitational waves – tiny ripples in the fabric of spacetime itself – may help astronomers unlock how the biggest stars die.

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Could a tabletop experiment detect gravitational waves and determine the quantum nature of gravity?

This illustration shows the merger of two black holes and the gravitational waves that ripple outward as the black holes spiral toward each other. Could black holes like these (which represent those detected by LIGO on Dec. 26, 2015) collide in the dusty disk around a quasar's supermassive black hole explain gravitational waves, too? Credit: LIGO/T. Pyle
This illustration shows the merger of two supermassive black holes and the gravitational waves that ripple outward as the black holes spiral toward each other. Credit: LIGO/T. Pyle

Perhaps the most surprising prediction of general relativity is that of gravitational waves. Ripples in space and time that spread through the universe at the speed of light. Gravitational waves are so faint that for decades their detection was thought impossible. Even today, it takes an array of laser interferometers several kilometers long to see their effect. But what if we could detect them with a table-top experiment in a university lab?

In a recent paper published in the New Journal of Physics, a team of physicists proposes just such a device. Rather than using beams of light, they suggest using the quantum superposition of a single electron.

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Why Can Black Hole Binaries Have Dramatically Different Masses? Multiple Generations of Mergers

Simulated merger of two black holes. Credit: NASA's Goddard Space Flight Center

On the 12th of April, 2019, the LIGO and Virgo gravitational wave observatories detected the merger of two black holes. Named GW190412, one of the black holes was eight solar masses, while the other was 30 solar masses. On the 14th of August that year, an even more extreme merger was observed, when a 2.5 solar mass object merged with a black hole nearly ten times more massive. These mergers raise fundamental questions about the way black hole mergers happen.

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The Moon is an Ideal Spot for a Gravitational Wave Observatory

High-resolution view of the lunar surface (JAXA/SELENE)

In the coming years, multiple space agencies will be sending missions (including astronauts) to the Moon’s southern polar region to conduct vital research. In addition to scouting resources in the area (in preparation for the construction of a lunar base) these missions will also investigate the possibility of conducting various scientific investigations on the far side of the Moon.

However, two prominent scientists (Dr. Karan Jani and Prof. Abraham Loeb) recently published a paper where they argue that another kind of astronomy could be conducted on the far side of the Moon – Gravitational Wave astronomy! As part of NASA’s Project Artemis, they explain how a Gravitational-wave Lunar Observatory for Cosmology (GLOC) would be ideal for exploring GW in the richest and most challenging frequencies.

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A Black Hole Popping Out of a Traversable Wormhole Should Give Off a Very Specific Signal in Gravitational Waves

Artist view of colliding neutron stars. Credit: ESO/L. Calçada/M. Kornmesser

Gravitational wave astronomy has changed the way we view the cosmos. In only a few years we have observed the collisions of black holes and neutron stars, confirming our theoretical understanding of these strange objects. But as gravitational wave astronomy matures, it will allow us to probe the very nature of space and time itself. While that day is a long way off, it hasn’t stopped the theory folks from dreaming up new discoveries. For example, how it might look if a black hole and a wormhole interact.

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