#GW250114
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ligo.org
What a difference a decade makes! Announcing the clearest #GravitationalWave detection ever #GW250114

youtu.be/2XmZ8-XQ9jU

📓: doi.org/10.1103/kw5g...

🔭🧪⚛️☄️ #O4IsHere
GW250114 – The Clearest of Chirps
YouTube video by LIGO Virgo KAGRA
youtu.be
September 10, 2025 at 4:20 PM
qntm.org
Absolutely mind-boggling to me that this isn't a fully solved problem. "GW250114"? With "25" being the year number? Do you think gravitional wave observations aren't going to continue beyond this century?
GW250114 - Wikipedia
en.wikipedia.org
September 13, 2025 at 10:33 PM
wulfhelm.bsky.social
This week, Mr Pip has barked at

Cobbles

GW250114

Mr Tambourine Man

Lucozade

Somnambulists

Tertiary anything

Things in aspic

The Meiji Restoration

Nike footwear

Velcro

Staples

U bends

Spoke shaves

Daguerréotypes

Flock wallpaper

Board games

Parables

and

Clackmannanshire.
September 26, 2025 at 4:02 PM
johnbird001.bsky.social
The strongest gravitational wave signal yet. GW250114 was detected by both arms of the Laser Interferometer Gravitational-wave Observatory (LIGO) in Washington and Louisiana USA earlier this year.
October 10, 2025 at 8:47 PM
ligo.org
Yesterday's Astronomy Picture of the Day #APOD featured #GW250114! This artwork imagines the ultimate front-row seat as two black holes spiral together on their way toward producing the strongest gravitational-wave signal we've detected so far

apod.nasa.gov/apod/ap25092...

🎨A Simonnet 🔭🐚
This artwork imagines the ultimate front-row seat for GW250114, a powerful collision between two black holes observed in gravitational waves by the US National Science Foundation LIGO. It depicts the view from one of the black holes as it spirals toward its cosmic partner.
September 25, 2025 at 8:16 AM
ligo.org
#GW250114's source is much like that for our first detection GW150914. Progress with our detectors means that the signal is much louder. Therefore, we can make much better measurements

📊: doi.org/10.1103/kw5g...

#O4IsHere
Measured masses for GW150914 and GW250114. Both have black holes of around the same masses (roughly 35 times the mass of our Sun). However, the uncertainty on the measurements for GW250114 are much smaller. This is the type of thing that makes astrophysicists excited.
September 10, 2025 at 5:09 PM
spaceaday.bsky.social
GW250114: Rotating Black Holes Collide
GW250114: Rotating Black Holes Collide
September 24, 2025 at 4:00 PM
astronerdika.bsky.social
Mirror, mirror, reflecting our [LASER] beam...
What is the loudest [gravitational wave] signal that we've seen?

It’s #GW250114!

(Yes, it’s been two weeks since it was announced, but I can still celebrate! 🎉 )

#EinsteinWasRight #HawkingWasRight
@ligo.org @egovirgo.bsky.social
An infographic created by @astronerdika titled “MIRROR, MIRROR, reflecting our LASER beam… what’s the LOUDEST signal gravitational wave we’ve seen?” explaining the gravitational-wave discovery GW250114 and how the observation confirms Hawking’s area law. The visual shows the mirrors in a gravitational-wave interferometer speaking about the loudest event they have seen. There are several illustrations as follows: 1. A simplified diagram of a laser interferometer. A red laser beam from a labeled “LASER source” hits a beam splitter, travels down two perpendicular arms, reflects off round mirrors, and recombines at a labeled “detector.” A label near the top-right mirror reads: “the DETECTOR, signal seen by LIGO Hanford & LIGO Livingston.”
 2. An illustration of a binary black hole merger, with two black circles spiraling inward. They are labeled ~34 solar masses and ~32 solar masses. Surrounding spiral lines represent gravitational waves. A nearby caption reads: “the SOURCE, Discovered in 2025, on January 14, at 08:22:03 UTC.” 3. A prominent speech bubble with white text on a purple background states: “GW250114 is the loudest & clearest signal we’ve seen!” A smaller note below reads: “as of January 2025.” 4. Another speech bubble reads: “AND we saw that Hawking was right too!” 5. Visual explanation of Hawking’s Area Law. Two small circles labeled “this BH” + “this BH” are shown to the left of a “<” symbol, pointing to a larger circle labeled “the surface area of the merged BH.” Below there is the explanatory sentence: “GW250114’s remnant event horizon area is larger than the sum of the individual areas.” 6. A section titled “the PAPERS” lists two arXiv references: https://arxiv.org/abs/2509.08054 and https://www.arxiv.org/abs/2509.08099 Note: This infographic plays off the classic line from Snow White, “Mirror, mirror on the wall…” Here, the “mirrors” are the ones inside the laser interferometer, reflecting light to detect passing gravitational waves.
September 26, 2025 at 12:56 AM
nature.com
Nature research paper: GW250114 reveals signatures of post-merger black-hole horizon

go.nature.com/3SnYbkt
GW250114 reveals signatures of post-merger black-hole horizon - Nature
The observation of a direct wave after the merger of two black holes reveals signatures associated with the remnant black-hole horizon, establishing an observational channel to directly measure frame-dragging effects in black-hole ergospheres and probe the horizon surface gravity.
go.nature.com
July 1, 2026 at 9:02 AM
fanapod.baldanders.info
#apod 2025-09-24
GW250114: Rotating Black Holes Collide
Web page: https://apod.nasa.gov/apod/ap250924.html
apod.7205381.bin
September 24, 2025 at 6:30 AM
apod.shinyakato.dev
🔭 GW250114: Rotating Black Holes Collide

Illustration Credit: Aurore Simonnet (SSU/EdEon), LVK, URI; LIGO Collaboration

apod.nasa.gov/apod/ap25092...
Artwork depicts a colorful version of two black holes nearing collision from between the black holes. Swirling gas is depicted with wavey lined depicting gravitational waves ringing and an artificial grid depicting spacetime shown distorting. Please see the explanation for more detailed information.
September 24, 2025 at 8:00 AM
herbstwind.bsky.social
Es war das stärkste jemals gemessene Gravitationswellensignal GW250114 wurde von beiden Armen des Laser Interferometer Gravitational-wave Observatory (LIGO) in Washington und Louisiana, USA, zwei Schwarze Löcher jedes mit einer Masse von etwa 33 Sonnenmassen kollidierten
October 20, 2025 at 3:28 AM
ligo.org
"This detection will quickly 'become one of my favourites', says David Reitze, executive director of the LIGO laboratory"

@jennaahart.bsky.social reviews some of our greatest discoveries, including the new #GW250114 in Nature News

www.nature.com/articles/d41...

#GW10Years 🧪⚛️🔭
Artistic interpretation of a binary black hole. It is probably more colourful than the real thing. Credit: Aurore Simonnet (SSU/EdEon)
September 12, 2025 at 7:41 PM
ligo.org
Happy birthday to #GW250114 our loudest detection to date!

In this video, @drbecky.bsky.social explains how we used the signal to test one of Hawking's fundamental ideas about black holes

www.youtube.com/watch?v=_fLO...

🧪⚛️🔭
FINALLY: evidence for Hawking's AREA THEOREM of black holes
YouTube video by Dr. Becky
www.youtube.com
January 14, 2026 at 11:43 AM
drnereide.bsky.social
🧵
On 14 January 2025, the LIGO's detectors captured GW250114, a gravitational wave signal (GWS) caused by two black holes' coalescence, each about 30 times the size of our Sun.

With a signal-to-noise ratio of 80, as opposed to 26 for GW150914...

Image Credits: Maggie Chiang/Simons Foundation

🔭 🧪
The illustration shows gravitational waves (GWs) that emanate from colliding black holes. GWs bear clues about these unseen objects.
September 29, 2025 at 6:54 PM
ligo.org
When a black hole is formed in a merger it emits a set of #GravitationalWave frequencies, ringing like a bell

Measuring these tests the nature of black holes. #GW250114 lets us measure multiple overtones, and they agree with theory

🎞️: Pfeiffer/Buonanno/Mitman/@sxs.bsky.social

#O4IsHere ⚛️🔭☄️
September 10, 2025 at 6:07 PM
herbstwind.bsky.social
Es handelte sich um das stärkste jemals gemessene Gravitationswellensignal GW250114 Analysen ergaben, dass das Ereignis entstand, als zwei Schwarze Löcher mit jeweils etwa 33 Sonnenmassen zu einem größeren Schwarzen Loch mit einer Masse von etwa 63 Sonnenmassen verschmolzen das ist Gigantisch
May 11, 2026 at 3:30 AM
natureportfolio.nature.com
A paper in Nature identifies the wave component of the gravitational-wave signal produced from the collision between two black holes. Observations of the binary black hole merger event called GW250114 provides information about the remnant black hole event horizon. go.nature.com/4vqAMNJ ⚛️🔭🧪
This is figure 1, which shows a sketch of the wave emission near the merger stage of a binary black-hole coalescence.
July 4, 2026 at 1:50 AM
ligo.org
Loud signals are perfect for testing Einstein's theory of general relativity.

The previous loudest signal was #GW230814 with a signal-to-noise ratio of 42. #GW250114 has a signal-to-noise ratio of 80. This enables some extremely precise tests!

bsky.app/profile/ligo...

#O4IsHere
ligo.org LIGO Scientific Collaboration @ligo.org · Sep 10
Our detailed study of #GW230814 is out

arxiv.org/abs/2509.07348

We can precisely test general relativity with this loud signal. Most tests show agreement with Einstein's theory, but some…

The deviations can be explained by detector noise. Having multiple detectors is important!

🔭🧪⚛️☄️ #GWTC4
September 10, 2025 at 5:38 PM
pcoffeebreak.bsky.social
Episodio 523 de Coffee Break:

Posible biomarcador en la roca marciana
Continúa Órbita Laika y se cancela El Cazador de Cerebros en TVE
España apuesta por el TMT
La lengua de los hunos
Contaminación en vacunas para COVID
Gravitondas GW231123 y GW250114

señalyruido.com
September 12, 2025 at 10:40 AM
ripleyguru.bsky.social
GW250114: Precision Test of Einstein’s No?Hair Theorem and Hawking’s Area Law
https://ripley.guru/main/article/gw_precision_test_einstein_hawking
GW250114: Precision Test of Einstein’s No?Hair Theorem and Hawking’s Area Law
September 12, 2025 at 1:18 AM
ligo.org
"Strongest black hole collision yet confirms theories of Einstein, Hawking"

Adrian Cho of @science.org writes about our discovery of #GW250114

www.science.org/content/arti...

#O4IsHere #EinsteinWasRight #HawkingWasRight #KerrWasRight 🔭🧪⚛️☄️
A comparison of GW250114 with our first detection GW150914. The stretching of space in the new black hole merger (top) is similar to that in the first one ever spotted (bottom), but because of reductions in the noise in the detectors, the signal stands out far more clearly. Graphic by C. Bickel/Science. Data from us
September 11, 2025 at 4:51 PM
pauleric70.bsky.social
😲👏💙😎

Astronomers have, for the first time, probed the event horizon region of a black hole using gravitational waves. Analyzing the loudest detected signal so far — GW250114 from a binary black hole merger — researchers from OzGrav/ANU identified a previously under-explored "direct wave" component
June 26, 2026 at 4:03 AM
natureportfolio.nature.com
A paper in Nature identifies the wave component of the gravitational-wave signal produced from the collision between two black holes. Observations of the binary black hole merger event called GW250114 provides information about the remnant black hole event horizon. go.nature.com/4vqAMNJ ⚛️🔭🧪
This is figure 1, which shows a sketch of the wave emission near the merger stage of a binary black-hole coalescence.
June 25, 2026 at 7:46 PM
cplberry.bsky.social
Preprint out today: A short review of science to come from GWTC-4.0 and GWTC-5.0 put together with @daniel-williams.co.uk

arxiv.org/abs/2609.03859

Catch up on some of the recent advances in gravitational-wave astronomy

🔭☄️🧪⚛️ #GWTC4 #GWTC5
Timeline of LIGO Virgo KAGRA observing runs, showing the increase in detector range and increase in the number of detections Comparison of our first detection GW150914 and recent loud detection GW250114. While the sources are similar, GW250114 is much louder because of advances in our detectors. This means that measurements of source properties are much more precise. The inferred mass distribution of binary black holes from GWTC-3.0, GWTC-4.0 and GWTC-5.0. As we have built larger catalogues, the precision of the inferred distribution has improved. Timeline of observing runs and data releases. GWTC-6.0 will release in December this year, so expect more science!
September 4, 2026 at 11:40 AM