Meet The Stranger Exoplanets

Until now astronomers have found about four thousand confirmed planets outside our Solar System. Of these, Earth-like exoplanets often make headlines. Such as Proxima B the closest rocky planet to our Solar System. This Earth-like exoplanet was found with the HARPS instrument on ESO’s 3.6-meter telescope at La Silla Observatory. But ESO telescopes have helped find plenty of other exciting worlds some so exotic you would not dare to compare them with Earth. Meet the Stranger Exoplanets.


What are the strangest exoplanets ever found or studied with ESO telescopes? Watch this ESOcast to find out.

WASP-19b Stranger Exoplanets

Let’s start with WASP-19b or as we like to call it, the inferno world with titanium skies. This hot Jupiter-sized planet has an atmosphere with a rather strange chemical composition. It was the first exoplanet where astronomers detected titanium oxide thanks to ESO’s Very Large Telescope and its FORS2 instrument.

Artist’s impression of the Stranger Exoplanet WASP-19b.
An artist’s impression showing the stranger exoplanets WASP-19b, in which atmosphere astronomers detected titanium oxide for the first time. In large enough quantities, titanium oxide can prevent heat from entering or escaping an atmosphere, leading to a thermal inversion — the temperature is higher in the upper atmosphere and lower further down, the opposite of the normal situation. Credit:
ESO/M. Kornmesser

This element acts as a heat-absorber in the atmosphere of an inferno world. It can prevent heat from entering or escaping through the atmosphere leading to a thermal inversion. So on WASP-19b, the temperature could be higher in the upper atmosphere and lower further down, unlike what we see on our Solar System planets.

‘Lonely Planet’ Stranger Exoplanets

We move on from this upside-down world to present you the Lonely Planet. A few years ago ESO telescopes and their instruments helped identify an object that could be a planet without any ties to a star.

Stranger Exoplanets Loney Planet CFBDSIR J214947.2-040308.9
This artist’s impression shows a strange free-floating exoplanet CFBDSIR J214947.2-040308.9. This is the closest such object to the Solar System. It does not orbit a star and hence does not shine by reflected light; the faint glow it emits can only be detected in infrared light. Here we see an artist’s impression of an infrared view of the object with an image of the central parts of the Milky Way from the VISTA infrared survey telescope in the background. The object appears blueish in this near-infrared view because much of the light at longer infrared wavelengths is absorbed by methane and other molecules in the planet’s atmosphere. In visible light the object is so cool that it would only shine dimly with a deep red color when seen close-up. Credit: ESO

A free-floating world that rather than move around a star roams rogue through space. It could be that these planets have formed like other worlds around a parent star, but then have been kicked out of their home system. So our Lonely Planet may well be an orphaned world.

Yet Stranger Exoplanets ‘Evaporating Exoplanet’

Our next strange exoplanet is not orphaned at all. In fact it hung on to its parent star through thick and thin. The Evaporating Exoplanet is the first giant planet ever found to be orbiting a white dwarf, the remnant of a Sun-like star.

Evaporating Exoplanet
Researchers using ESO’s Very Large Telescope have, for the first time, found evidence one of the giant stranger exoplanets associated with a white dwarf star. The planet orbits the hot white dwarf, the remnant of a Sun-like star, at close range, causing its atmosphere to be stripped away and form a disc of gas around the star. This unique system hints at what our own Solar System might look like in the distant future. Credit: ESO

Astronomers think that this exoplanet survived the transition of its parent solar-type star to a red giant and then to a white dwarf. But that’s not all that is strange about this planet. Observations with ESO’s X-shooter on the VLT have hinted that this giant exoplanet is evaporating. It orbits the hot white dwarf at close range and the extreme ultraviolet radiation from the star strips away part of the planet’s atmosphere forming a disc around the white dwarf.

The Strangest Exoplanet WASP-76b

Our final alien world is even stranger WASP-76b an ultra hot giant exoplanet with a twist. This planet orbits very close to its parent star receiving thousands of times more radiation from it than the Earth does from the Sun. It is also tidally locked, meaning it has a day side that always faces the star and a much cooler night side.

Exoplanet WASP-76b
This illustration shows a night-side view of the strangest exoplanet WASP-76b. The ultra-hot giant exoplanet has a day side where temperatures climb above 2400 degrees Celsius, high enough to vaporize metals. Strong winds carry iron vapour to the cooler night side where it condenses into iron droplets. To the left of the image, we see the evening border of the exoplanet, where it transitions from day to night. Credit: ESO

The temperature difference on the planet is extreme. On the day side it is above 2400 degrees Celsius and everything including metals is vaporized. This is where things get really weird. Using the ESPRESSO instrument on the VLT, astronomers found that iron vapor from the ultra hot day side is carried to the cooler night side. There it condenses into iron droplets. In other words, this extreme exoplanet has a day side where metals evaporate and a night side where it rains iron.

Stranger Exoplanets conclusions

Will we find even stranger worlds? Well nobody knows. But astronomers keep on hunting for exoplanets. Stay tuned for future discoveries with ESO telescopes.

Credit: The Stranger Exoplanets Transcribed and produced by ESO

Directed by: Herbert Zodet and Bárbara Ferreira.
Editing: Herbert Zodet.
Web and technical support: Gurvan Bazin and Raquel Yumi Shida.
Written by: Bárbara Ferreira and Herbert Zodet.
Music: zero-project (zero-project.gr) — Into the darkness and STAN DART (www.stan-dart.com) – Supernova.
Footage and photos: ESO, M. Kornmesser, L. Calçada, Alexandre Santerne, B. Tafreshi (twanight.org), C. Malin (christophmalin.com), Gianluca Lombardi (glphoto.it), ESA/Hubble, L. L. Christensen, Space Engine (spaceengine.org), M. Zamani (mahdizamani.com), P. Delorme/Nick Risinger (skysurvey.org)/R. Saito/VVV Consortium.
Scientific consultants: Paola Amico and Mariya Lyubenova.

About the author

Jeramie has an Associate of Applied Science in Web Development and is currently studying Astronomy while writing online articles here as part of his learning and research process. If you find errors and inaccuracies, please make a comment or contact him directly. He feels discussion is also part of the learning process and welcomes respectful public comments under any article on CuriousAstronomer.com

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