This site uses cookies. By continuing to use this site you agree to our use of cookies. To find out more, see our Privacy and Cookies policy.
Skip to the content

Share this

Free weekly newswire

Sign up to receive all our latest news direct to your inbox.

Physics on film

100 Second Science Your scientific questions answered simply by specialists in less than 100 seconds.

Watch now

Bright Recruits

At all stages of your career – whether you're an undergraduate, graduate, researcher or industry professional – can help find the job for you.

Find your perfect job

Physics connect

Are you looking for a supplier? Physics Connect lists thousands of scientific companies, businesses, non-profit organizations, institutions and experts worldwide.

Start your search today


LIGO paints a clearer picture of its merging black holes

Illustration of two black holes spiralling into each other to create a larger black hole (Courtesy: Caltech/MIT/LIGO Lab)

Illustration of two black holes spiralling into each other to create a larger black hole. (Courtesy: Caltech/MIT/LIGO Lab)

By Hamish Johnston

Physicists working on the LIGO gravitational-wave detectors have released more information about the merging black holes that they announced the discovery of earlier this year. Dubbed GW150914, we now know that the gravitational wave was created by the merger of one black hole that was 36 times as massive as the Sun with a smaller black hole that weighed in at 29 solar masses. The result of the merger was a black hole at 62 solar masses and a spin angular momentum of 0.67, where 1.0 is the maximum value of spin a black hole can have.

According to the team, the black hole created by the GW150914 merger is the largest “stellar-mass” black hole known to astronomers. This doesn’t include the much larger supermassive black holes that are known to inhabit the centres of most galaxies.

LIGO scientists have also calculated that the collision occurred about 410 MPc (about one billion light-years) from Earth and GW150914 is likely to have come from the southern sky.

If you want to know more, the analysis is presented in a paper in Physical Review Letters: “Properties of the binary black hole merger GW150914”.

This entry was posted in General and tagged , , . Bookmark the permalink.
View all posts by this author  | View this author's profile


  1. M. Asghar

    Quote from reference(96)of the paper:”we find no evidence for violations of general relativity in the genuinely strong-field regime of gravity.” Important result showing that one can use the “numerical gravity” to deal with the GW’s emitted in a strong gravitational field region.


  • Comments should be relevant to the article and not be used to promote your own work, products or services.
  • Please keep your comments brief (we recommend a maximum of 250 words).
  • We reserve the right to remove excessively long, inappropriate or offensive entries.

Show/hide formatting guidelines

Tag Description Example Output
<a> Hyperlink <a href="">google</a> google
<abbr> Abbreviation <abbr title="World Health Organisation" >WHO</abbr> WHO
<acronym> Acronym <acronym title="as soon as possible">ASAP</acronym> ASAP
<b> Bold <b>Some text</b> Some text
<blockquote> Quoted from another source <blockquote cite="">IOP</blockquote>
<cite> Cite <cite>Diagram 1</cite> Diagram 1
<del> Deleted text From this line<del datetime="2012-12-17"> this text was deleted</del> From this line this text was deleted
<em> Emphasized text In this line<em> this text was emphasised</em> In this line this text was emphasised
<i> Italic <i>Some text</i> Some text
<q> Quotation WWF goal is to build a future <q cite="">
where people live in harmony with nature and animals</q>
WWF goal is to build a future
where people live in harmony with nature and animals
<strike> Strike text <strike>Some text</strike> Some text
<strong> Stronger emphasis of text <strong>Some text</strong> Some text