Twitter #EarthquakeCup is in full swing

In the grand tradition of #MammalMarchMadness, the exceedingly popular Twitter-poll-based geeky sciencey alternative to the US’s eponymous basketball tournament, which grew to extraordinary popularity after its inception by evolutionary biologist @Mammals_Suck […milk] (a.k.a. Katie Hinde), natural scientists have spawned a staggering array of spinoff competitions in their own fields. As it sweeps through the subdisciplines of geology, the phenomenon has arrived at earthquakes. Having a poll-based competition among history’s “greatest” …

The post Twitter #EarthquakeCup is in full swing appeared first on The Trembling Earth.

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‘Oumuamua likely came from a binary star system

New research finds that ‘Oumuamua, the rocky object identified as the first confirmed interstellar asteroid, very likely came from a binary star system.


“It’s remarkable that we’ve now seen for the first time a physical object from outside our Solar System,” says lead author Dr Alan Jackson, a postdoc at the Centre for Planetary Sciences at the University of Toronto Scarborough in Ontario, Canada.

thumb Oumuamua artistArtist’s impression of ‘Oumuamua. Credit: ESO / M. Kornmesser. Click for a larger image


A binary star system, unlike our Sun, is one with two stars orbiting a common centre.


For the new study, published in the journal Monthly Notices of the Royal Astronomical Society, Jackson and his co-authors set about testing how efficient binary star systems are at ejecting objects. They also looked at how common these star systems are in the Galaxy.


They found that rocky objects like ‘Oumuamua are far more likely to come from binary than single star systems. They were also able to determine that rocky objects are ejected from binary systems in comparable numbers to icy objects.


“It’s really odd that the first object we would see from outside our system would be an asteroid, because a comet would be a lot easier to spot and the Solar System ejects many more comets than asteroids,” says Jackson, who specializes in planet and solar system formation.


Once they determined that binary systems are very efficient at ejecting rocky objects, and that a sufficient number of them exist, they were satisfied that ‘Oumuamua very likely came from a binary system. They also concluded that it probably came from a system with a relatively hot, high mass star since such a system would have a greater number of rocky objects closer in.


The team suggest that the asteroid was very likely to have been ejected from its binary system sometime during the formation of planets.


‘Oumuamua, which is Hawaiian for ‘scout’, was first spotted by the Haleakala Observatory in Hawaii on 19 October 2017. With a radius of 200 metres and travelling at a blistering speed of 30 kilometres per second, at its closest it was about 33,000,000 km from Earth.


When it was first discovered researchers initially assumed the object was a comet, one of countless icy objects that release gas when they warm up on approaching the Sun. But it didn’t show any comet-like activity as it neared the Sun, and was quickly reclassified as an asteroid, meaning it was rocky.


Researchers were also fairly sure it was from outside our Solar System, based on its trajectory and speed. An eccentricity of 1.2 – which classifies its path as an open-ended hyperbolic orbit – and such a high speed meant it was not bound by the gravity of the Sun.


In fact, as Jackson points out, ‘Oumuamua’s orbit has the highest eccentricity ever observed in an object passing through our Solar System.


Major questions about ‘Oumuamua remain. For planetary scientists like Jackson, being able to observe objects like these may yield important clues about how planet formation works in other star systems.


“The same way we use comets to better understand planet formation in our own Solar System, maybe this curious object can tell us more about how planets form in other systems.”


Media contacts


Dr Robert Massey

Royal Astronomical Society

Tel: +44 (0)20 7292 3979

Mob: +44 (0)7802 877 699


Dr Morgan Hollis

Royal Astronomical Society

Tel: +44 (0)20 7292 3977

Mob: +44 (0)7802 877 700


Science contact


Dr Alan Jackson

CPS Postdoctoral Fellow

Centre for Planetary Sciences

University of Toronto

Tel: +1 416 208 5099 (4 hours behind GMT)


Image and caption


Artist’s impression of ‘Oumuamua. Credit: ESO / M. Kornmesser


Further information


The new work appears in: “Ejection of rocky and icy material from binary star systems: Implications for the origin and composition of 1I/`Oumuamua”, A. Jackson, D. Tamayo, N. Hammond, M. Ali-Dib, H. Rein, Monthly Notices of the Royal Astronomical Society (2018), in press (DOI: 10.1093/mnras/sly033).


A copy of the paper is available here


Notes for editors


The Royal Astronomical Society (RAS), founded in 1820, encourages and promotes the study of astronomy, solar-system science, geophysics and closely related branches of science. The RAS organizes scientific meetings, publishes international research and review journals, recognizes outstanding achievements by the award of medals and prizes, maintains an extensive library, supports education through grants and outreach activities and represents UK astronomy nationally and internationally. Its more than 4,000 members (Fellows), a third based overseas, include scientific researchers in universities, observatories and laboratories as well as historians of astronomy and others.


The RAS accepts papers for its journals based on the principle of peer review, in which fellow experts on the editorial boards accept the paper as worth considering. The Society issues press releases based on a similar principle, but the organisations and scientists concerned have overall responsibility for their content.


Follow the RAS on Twitter, Facebook and Instagram


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LGBTSTEM DAY – 5 July 2018

Pride in STEM, House of STEM, and InterEngineering are proud to announce the launch of the first ever International Day of LGBT+ people in Science, Technology, Engineering, and Maths, called LGBTSTEM Day, to be celebrated on 5 July 2018.



The purpose of LGBTSTEM Day is to improve the visibility and representation of LGBT+ people in STEM, help them access and share resources, and build a stronger LGBT+ community.


The LGBT+ Physical Sciences Network, formed in 2016 by the Royal Astronomical Society and the Institute of Physics, support LGBTSTEM Day and will contribute to the event in a number of ways.


The LGBT+ Physics Sciences Network, with the Royal Astronomical Society, believe that professional membership organisations can offer support and experiences of current good practice with regard to successful LGBT+ networks in places of work and study. Facilitating and helping to connect the LGBT+ physical sciences community is an important step in this process and we believe that LGBTSTEM Day will enable this.


How to get involved


There’s no such thing as too small a gesture to promote and support LGBT+ people in STEM. You can start by following and contributing to the #LGBTSTEMday hashtag on social media — share stories, images and videos of yourself or your role models — and help boost the visibility of other LGBT+ people in science, tech, engineering, and maths. Make sure you tag in @RAS_outreach and @IOPDiversity to connect with the LGBT+ Physical Sciences Network.


If you or your organisation want to get involved, please download our LGBTSTEM Day Toolkit or get in touch via email or on social media.



Pride in STEM is a UK-based charitable trust working to promote and support LGBT+ people working in STEM.


House of STEM is an Irish-based Network dedicated to connecting and supporting LGBTQ+ scientists in the Republic of Ireland.


InterEngineering is an organisation dedicated to connecting, informing and empowering LGBT+ engineers and supporters.


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