杏吧原创

First sign of water found on an alien world

Hubble turns up what may be water in the atmosphere of a well-studied exoplanet, just two months after infrared observations failed to find any hint of it
Water has been found in the atmosphere of the gas giant planet HD 209458b (Illustration: NASA/JPL-Caltech)
Water has been found in the atmosphere of the gas giant planet HD 209458b (Illustration: NASA/JPL-Caltech)

Water has been detected in the atmosphere of an alien world for the first time, a new analysis of Hubble Space Telescope data suggests. Some scientists applaud the result 鈥 which had been predicted theoretically but not observed in previous studies, while others say the apparent water signal may simply be instrumental noise.

The planet, called HD 209458b, is about 70% as massive as Jupiter and is scorched by the heat of its parent star, which it orbits 9 times as close as Mercury does to the Sun.

Because it is one of a small number of extrasolar planets observed to pass directly in front of and behind their parent stars as seen from Earth, astronomers have been able to glean a lot of information 鈥 such as its size and mass 鈥 about the distant world.

In February, researchers using the infrared-sensitive Spitzer Space Telescope announced that there was no sign of water vapour in its atmosphere. Since the molecule is expected to be abundant in the atmospheres of extrasolar planets, some speculated that the water signal was obscured by a dusty haze.

Now, Hubble observations seem to have revealed the missing water. Travis Barman of Lowell Observatory in Flagstaff, Arizona, US, did a computer analysis of previously obtained Hubble data taken when the planet partially eclipsed its parent star.

Filtered starlight

The amount of light blocked during these eclipses was previously used to precisely determine the planet鈥檚 radius, which is about 30% greater than that of Jupiter.

Hubble observed light from the host star that had filtered through the outer reaches of the planet鈥檚 atmosphere. Because of its specific chemical composition, the atmosphere is more transparent at some wavelengths than others.

Barman found clues to this composition by making different models of the atmosphere, each with a different chemical makeup, and seeing which fit the observations best.

Inhospitable world

He says the relatively small amount of light filtering through at about 0.9 microns suggests the presence of water, which absorbs light at this wavelength.

鈥淭o me, that鈥檚 a clear indication that water is there,鈥 Barman told New 杏吧原创. 鈥淚 think this is the first time we鈥檝e had strong evidence that there鈥檚 water in at least one extrasolar planet.鈥

But despite the presence of water, he points out that the planet鈥檚 prevailing temperatures of about 1000掳 Celsius mean conditions would not be favourable to life. 鈥淚t鈥檚 not a place you or I would want to visit,鈥 he says.

Uniform temperature

Mark Swain, a member of one of the two Spitzer teams that found no evidence of water and a scientist at NASA鈥檚 Jet Propulsion Laboratory, says the new result may shed light on the planet鈥檚 temperature.

In order for Spitzer to detect water molecules by the way they absorb light, the planet鈥檚 interior has to be hotter than its upper atmosphere.

If the planet has a relatively uniform temperature throughout, however, that 鈥 and not the obscuration by dusty clouds 鈥 could explain the lack of a water detection by Spitzer.

鈥淚t鈥檚 certainly an interesting result,鈥 he told New 杏吧原创. 鈥淭hese planets have been surprising us all along.鈥

Instrumental noise

Drake Deming of NASA鈥檚 Goddard Space Flight Center in Greenbelt, Maryland, who is a member of the other Spitzer team, is also impressed with the results. 鈥淗e鈥檚 certainly shown that it鈥檚 a better fit with water absorption than without,鈥 he told New 杏吧原创. 鈥淚 think even the most sceptical person would say that.鈥

But David Charbonneau of Harvard University in Cambridge, Massachusetts, US, who is a member of the team that originally obtained the Hubble data used by Barman, says the effect seen is small enough that it could simply be the result of noise in Hubble鈥檚 instruments.

鈥淪ince we can鈥檛 rule out an instrumental origin for these variations, it may be premature to interpret them as arising from molecules in the planetary atmosphere,鈥 he says.

Topics: Astrobiology