Astronomers discover three 'Qatar' exoplanets

June 29, 2016 by Tomasz Nowakowski, weblog

Artist's impression of the newly discovered planets Qatar-3b, Qatar-4b and Qatar-5b. Credit: QNA
(—An international team of astronomers has discovered three new exoplanets using a Qatar-based planet-searching survey. The newly discovered gas giant exoworlds belong to the so-called "hot Jupiter" family of planets and were designated Qatar-3b, Qatar-4b and Qatar-5b. The findings were presented in a paper published June 23 on

The planets were identified by the Qatar Exoplanet Survey (QES), operated by the Qatar Environment and Energy Research Institute (QEERI), which is part of Hamad Bin Khalifa University (HBKU) in Doha, Qatar. The survey utilizes a robotic wide-field camera system located in New Mexico to search for gas giant planets that transit relatively bright host stars. The project proved its planet-searching capabilities in 2010 and 2011 when it detected the Qatar-1b and Qatar-2b exoplanets.

Recently, an international group of astronomers, led by Khalid Al-Subai, QEERI's acting executive director, spotted three new planetary transits via QES. The scientists also conducted follow-up spectroscopic observations to determine the physical characteristics of the newly detected planets. For this purpose, they employed the Tillinghast Reflector Echelle Spectrograph (TRES) at the Fred L. Whipple Observatory on Mount Hopkins, Arizona and the 1.23m Zeiss Telescope at the Calar Alto Observatory in Spain.

The three detected planets are typical "hot Jupiters"—gas giant planets similar in characteristics to the solar system's biggest planet. These have orbital periods of less than 10 days and high surface temperatures, as they orbit their parent stars very closely. In the case of the three new alien worlds discovered by QES, the equilibrium temperature ranges from 1,400 to 1,700 K.

"We report the discovery of Qatar-3b, Qatar-4b, and Qatar-5b, three new transiting planets identified by the Qatar Exoplanet Survey. The three planets belong to the hot Jupiter family," the scientists wrote in the paper.

According to the research, Qatar-4b is the biggest and most massive of the newly found trio. With a radius of about 1.55 Jupiter radii, it is nearly six times more massive than our solar system's largest planet. It orbits its 13-billion-year-old sun-sized host star Qatar-4, every 1.8 days.

Qatar-3b and Qatar-5b are of similar size and mass. They both are about slightly larger than Jupiter (1.1 Jupiter radii) and have approximately 4.3 Jupiter masses. Their orbital periods are also comparable as Qatar-3b orbits its parent star every two and a half days, while it takes Qatar-5b nearly three days to fully circle its stellar companion.

"All three are short-period planets with masses and radii in the expected regime for hot Jupiters," the paper reads.

The stars, orbited by the newly discovered , are only a bit larger than the sun and have a mass ranging from 0.95 to 1.15 solar masses. The research also reveals that Qatar-5 is one of the most metal-rich host stars known to date.

The discovery proves that ground-based surveys like QES could be quite productive when it comes to exoplanet searching. The findings presented in the study could contribute to a more complete census of "hot Jupiters" and other close orbiting large . The authors of the paper believe that future observations of this class of celestial bodies may provide a key to understanding their origin and planetary system architecture more generally .

Explore further: Astronomers discover seven new giant exoplanets

More information: Qatar Exoplanet Survey : Qatar-3b, Qatar-4b and Qatar-5b, arXiv:1606.06882 [astro-ph.EP]

We report the discovery of Qatar-3b, Qatar-4b, and Qatar-5b, three new transiting planets identified by the Qatar Exoplanet Survey (QES). The three planets belong to the hot Jupiter family, with orbital periods of PQ3b=2.5079204 days, PQ4b=1.8053949 days, and PQ5b=2.8792319 days. Follow-up spectroscopic observations reveal the masses of the planets to be MQ3b=4.31MJ, MQ4b=5.85MJ, and MQ5b=4.32MJ, while model fits to the transit light curves yield radii of RQ3b=1.096RJ, RQ4b=1.552RJ, and RQ5b=1.107RJ. No evidence of eccentric orbit is seen in the radial velocity curve of any of the planets. The host stars are typical main sequence stars with masses and radii MQ3=1.145M⊙, MQ4=0.954M⊙, MQ5=1.128M⊙ and RQ3=1.272R⊙, RQ4=1.115R⊙ and RQ5=1.076R⊙ for the Qatar-3, 4 and 5 respectively. All three new planets can be classified as heavy hot Jupiters (M > 4 MJ), while Qatar-5 is among the most metal-rich stars known to host a planet.

Related Stories

Astronomers discover seven new giant exoplanets

April 21, 2016

(—Using the SuperWASP-South Observatory in South Africa, a team of European astronomers has discovered seven new giant planets orbiting distant stars. According to a new study, the smallest of the newly detected ...

Astronomers discover a giant planet spinning up its star

June 7, 2016

(—A giant "hot Jupiter" exoplanet has recently been detected by an international team of astronomers led by Kaloyan Penev of Princeton University. The newly found alien world, designated HATS-18b, is an interesting ...

Qatar-led international team finds its first alien world

December 14, 2010

In an exciting example of international collaboration, a Qatar astronomer teamed with scientists at the Harvard-Smithsonian Center for Astrophysics (CfA) and other institutions to discover a new alien world. This "hot Jupiter," ...

Astronomers detect five new 'hot Jupiters'

February 16, 2016

(—Giant exoplanets, like the so-called 'hot Jupiters' that are similar in characteristics to the solar system's biggest planet and orbit very close to their host stars, are excellent targets for astronomers in ...

Astronomers discover two new 'hot Jupiter' exoplanets

March 10, 2016

(—A team of Chilean astronomers recently detected two new "hot Jupiters" using the data from NASA's Kepler spacecraft operating in a new mission profile called K2. The planets, designated EPIC210957318b and EPIC212110888b, ...

Recommended for you

Exoplanet stepping stones

November 20, 2018

Astronomers have gleaned some of the best data yet on the composition of a planet known as HR 8799c—a young giant gas planet about 7 times the mass of Jupiter that orbits its star every 200 years.

Encouraging prospects for moon hunters

November 20, 2018

Astrophysicists of the University of Zürich, ETH Zürich and the NCCR PlanetS show how the icy moons of Uranus were born. Their result suggests that such potentially habitable worlds are much more abundant in the Universe ...

Gravitationally lensed quasars

November 19, 2018

The path of light is bent by mass, an effect predicted by Einstein's theory of gravity, and when a massive galaxy or cluster lies along our line-of-sight to a more distant galaxy its matter will act as a lens to image the ...


Please sign in to add a comment. Registration is free, and takes less than a minute. Read more

Click here to reset your password.
Sign in to get notified via email when new comments are made.