We are excited to announce the discovery of
#GW190521
, observed by
@LIGO
and
@ego_virgo
on May 21st 2019: the most massive binary
#BlackHoles
merger detected yet! Read the full story at
@Rainmaker1973
@ProfBrianCox
One of the really cool things about binary black hole is that if two similar mass black holes merge, you always get about the same power: two black holes 5 times the mass of the Sun give the same power as two black holes 5 billion times the mass of the Sun
Happy birthday James Clerk Maxwell, whose discoveries on the nature of electromagnetic waves helped to "light" the way towards Albert Einstein's theories of relativity. 1/2
As members of the LIGO Scientific Collaboration, we condemn all forms of racism. We stand with our Black members, colleagues, and friends to strive for justice and equality in the face of systemic discrimination, hatred and racism.
#BlackLivesMatter
A week into the 3rd
@LIGO
@ego_virgo
Observing Run and our first candidate has been posted to GraceDB - the
#GravitationalWave
candidate event database: say hello to S190408an! More info, including a map of its likely sky location, at
#O3ishere
1/2
A very happy 80th birthday from
@LIGO
and
@ego_virgo
to
@NobelPrize
laureate Kip Thorne - one of the three recipients of the 2017 prize for Physics. Many happy returns, Kip!
Happy 80th birthday to Kip Thorne. In the mid-70s, despite widespread scepticism, Thorne was convinced that gravitational waves could be detected.
In 2015, Thorne and
@LIGO
scientists observed gravitational waves for the first time. He received the
#NobelPrize
in Physics 2017.
Happy 8th birthday to the one that started it all:
#GW150914
! After Einstein predicted the existence of
#GravitationalWaves
, it took 100 years to detect the first. Now, in
#O4
, we detect a gravitational-wave event about once every 3 days!
#GW190521
is a special discovery: it's the first clear detection of an "Intermediate Mass Black Hole"
#imbh
– a kind of cosmic “missing link” in the
#BlackHoles
landscape, which may have a key role in how supermassive
#BlackHoles
form
#imbh
Gravitational wave astronomy has revealed a previously unknown population of black hole binaries: two black holes which orbit each other. From our first two observing runs we discovered 10 binary black holes
#BlackHoleWeek
Our new paper describes not one but *two*
#NeutronStar
#BlackHole
binaries we detected in Jan 2020, in the second part of our 3rd Observing Run
#O3b
. Read the science summary at
#NSBH
(multiple translations also available)
Signal in LIGO/Virgo data. Most likely
#gravitationalwaves
from a source with one component in NS-BH mass gap. Observed 24 minutes ago. Find out more at:
The ratio of the
#GW190412
#blackholes
masses is "roughly equal to the ratio of filling in a regular Oreo to in a Mega Stuf Oreo," notes
@LIGO
&
@NorthwesternU
's
@cplberry
"Investigations of connections between Oreos and black hole formation are ongoing."
@melizeche
@Rainmaker1973
@ProfBrianCox
Therefore, when you divide the energy by the time, the mass cancels out! If you're interested in the details, it's the total mass of the binary that cancels. The ratio of masses does effect the answer
The dance of black holes and neutron stars
This Orrery created by
@actualdrdoctor
illustrates the masses of our O3b
#GWTC3
candidates. More massive binaries slowly waltz, while lower mass ones energetically swing
📰:
Signal in LIGO/Virgo data. Most likely binary source with at least one component between 3 & 5 solar masses (mass gap). Observed 22 minutes ago. Find out more at:
With a tip of the hat to its genius creator, our
@LIGO
colleague
@actualdrdoctor
, we *love* this meme capturing the essence of today's
#NSBH
discovery announcement.
#NeutronStar
#BlackHole
mergers in liquid form! (Note: other soft drink brands are available...)
@melizeche
@Rainmaker1973
@ProfBrianCox
1. All the properties of a black hole scale with its mass: Big black holes are *identical* to small ones except scaled up. They are not like other objects where you could count the number of atoms or LEGO bricks they are made of
For decades, astronomers have puzzled over a “mass gap” that lies between neutron stars and black holes. Now, in
#GW190814
,
@LIGO
and
@EGO_Virgo
have found an object of 2.6 solar masses that’s firmly in the mass gap. Read the full press release at
Today the LIGO-Virgo-KAGRA Collaboration is proud to announce GW230529, the first exceptional
#GravitationalWaves
event from our fourth observing run (
#O4
). You can learn more from
@astronerdika
's excellent infographic, or by visiting our detection page!
Our
@LIGO
@ego_virgo
@KAGRA_PR
#AdventCalendar
has reached its final door! Today marks the birthday of Isaac Newton, born 25 December 1642. Many happy revolutions, Isaac! We hope you've enjoyed following our calendar: we'll be back with more doors in 2021
The two merging
#BlackHoles
in
#GW190521
“weighed in” at 85 and 66 times the Sun's mass, making
#GW190521
easily the heaviest pair of merging
#BlackHoles
detected so far – even heavier than almost all of the merger *remnants* we’ve seen to date…
@melizeche
@Rainmaker1973
@ProfBrianCox
2. Luminosity is energy emitted divided by time over which it is emitted. The energy scales linearly with the mass (think E = mc²), twice the mass, twice the energy. The time is set by the orbital period. This *also* scales linearly with the total mass (think Kepler's law).
We have discovered the heaviest known neutron star, or maybe the lightest known black hole: “Either way it breaks a record.” The
@nytimes
reports on the LIGO &
@ego_virgo
detection of
#GW190814
@melizeche
@Rainmaker1973
@ProfBrianCox
If you were to see a picture of a black hole without a scale bar, it'd be impossible to tell how big it is. The luminosity during merger is one of their universal properties, the same no matter how you scale the system