17 April 2019
Spectrum of the helium hydride ion (HeH+), detected using the GREAT instrument on board the SOFIA airborne observatory, observing in the direction of the planetary nebula NGC 7027. The background image of NGC 7027 was generated using data acquired by the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) installed on board the Hubble Space Telescope. The obvious area of transition between the hot ionised gas (yellowish-white) and the cooler shell (red) is clearly visible. It is in this transition zone that HeH+ is formed (marked with molecule symbols in the artist’s impression). The area of the sky captured by the GREAT measurements has a diameter of 14.3 arc seconds and includes most of the radiation from the planetary nebula. The width of the HeH+ spectral line is the result of the propagation velocity of the expanding shell.
Composition: NIESYTO design; Image NGC 7027: William B. Latter (SIRTF Science Center/Caltech) und NASA/ESA; Spektrum: Rolf Güsten/MPIfR, Nature, 18. April 2019.
With the SOFIA airborne observatory, astronomical observations in the infrared and submillimetre wavelength ranges are carried out using the 2.5-metre telescope on board the modified Boeing 747SP, flying mostly above the disruptive effects of Earth’s atmosphere.
The GREAT far-infrared spectrometer is mounted on the telescope flange within the pressurised cabin of the SOFIA airborne observatory. The telescope dish is located in a sealed space at the rear of the aircraft; its airlock is only opened during flight.
DLR (CC-BY 3.0).
The helium hydride ion, to give HeH+ its full name, once posed something of a dilemma for science. Although its existence has been known from laboratory studies for almost 100 years, it had not been found in space, despite extensive searches. As a result, the chemical model calculations associated with it were called into question. But an international team of researchers led by Rolf Güsten of the Max Planck Institute for Radio Astronomy in Bonn has now succeeded in clearly detecting this ion in the direction of the planetary nebula NGC 7027. The proof was obtained using the German Receiver for Astronomy at Terahertz Frequencies (GREAT), a far-infrared spectrometer carried on board the Stratospheric Observatory for Infrared Astronomy (SOFIA). SOFIA is a joint project by the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) and NASA, the US space agency. The results were published in the 18 April 2019 issue of the scientific journal Nature.
"Over the last decade, people have had great hopes for space observatories such as Spitzer (NASA, launched 2003) and Herschel (ESA, launched 2009), but none of these telescopes were able to detect this ion. SOFIA has provided us with proof that this ion really can form in planetary nebulae. At present, there is no other telescope capable of observing at these wavelengths, so this observation platform will remain unique for many years to come," says Anke Pagels-Kerp, Head of the Space Science Department at the DLR Space Administration in Bonn.
In the late 1970s, astrochemical models suggested that a detectable quantity of HeH+ might be present within nebulae in the Milky Way. It was thought most likely to be found in what are known as planetary nebulae, which are shells of gas and dust that have been ejected from a Sun-like star in the last phase of their lifecycle. The high-energy radiation generated by the central star drives ionisation fronts into the envelope of ejected material. According to the model calculations, it is precisely here that the HeH+ ions are supposed to form. Yet despite its undisputed importance in the history of the early Universe, it had long proven impossible to find the HeH+ ion in interstellar space. Although it has been known to exist since 1925, specific searches for it in space have been unsuccessful over recent decades.
The molecule emits its strongest spectral line at a characteristic wavelength of 149.1 micrometres (corresponding to a frequency of 2.01 terahertz). Earth's atmosphere blocks all radiation in this wavelength range, preventing searches by ground-based observatories; therefore, the search must be conducted either from space or using high-flying observatories such as SOFIA. At an altitude of 13 to 14 kilometres, SOFIA operates above the absorbing layers of the lower atmosphere.
"SOFIA offers a unique opportunity to use the very latest technologies at any given time. The ongoing German-led development of the GREAT instrument has now made the detection of helium hydride possible. This underlines the importance of such instruments and the potential that their development holds for SOFIA in future," explains Heinz Hammes, SOFIA Project Manager at the DLR Space Administration.
After the Big Bang, chemistry began in the Universe
The HeH+ ion is very important by virtue of its role in the formation of the Universe; all chemistry began approximately 300,000 years after the Big Bang. Although the Universe was still in its early stages, the temperature had already fallen to under approximately 3700 degrees Celsius. The elements that formed in the Big Bang – such as hydrogen, helium, deuterium and traces of lithium – were ionised at first, due to the high temperatures. As the Universe cooled, they recombined with free electrons to create the first neutral atoms. This happened first with helium. At this point, hydrogen was still ionised and was present in the form of free protons, or hydrogen nuclei. These combined with the helium atoms to form the helium hydride ion HeH+, making it one of the very first molecular compounds in the Universe. As recombination advanced, HeH+ reacted with the newly-formed neutral hydrogen atoms, thus paving the way for the formation of molecular hydrogen and thus the chemical origins of the Universe.
"Thanks to recent advances in terahertz technology, it is now possible to perform high-resolution spectroscopy at the required far-infrared wavelengths," explains Rolf Güsten, Lead Author of the article. As a result of measurements performed using the GREAT spectrometer on board the SOFIA airborne observatory, the team can now announce the unambiguous detection of the HeH+ ion in the direction of the planetary nebula NGC 7027.
Rolf Güsten et al.: First detection of the helium hydride ion (HeH+) in space, published in the 18 April 2019 issue of Nature.
The Stratospheric Observatory for Infrared Astronomy (SOFIA) is a joint project by the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) and the National Aeronautics and Space Administration (NASA). The German contribution of the project is managed by the DLR Space Administration, using funds provided by the German Federal Ministry for Economic Affairs and Energy, the Federal State of Baden-Württemberg and the University of Stuttgart. The scientific operations are coordinated by the German SOFIA Institute (Deutsches SOFIA Institut; DSI) at the University of Stuttgart in Germany and the Universities Space Research Association (USRA) in the USA. The development of the German instruments is financed with funds from the Max Planck Society (Max-Planck-Gesellschaft; MPG), the German Research Foundation (Deutsche Forschungsgemeinschaft; DFG) and DLR.
The German Receiver for Astronomy at Terahertz Frequencies (GREAT) is a high-resolution spectrometer for astronomical observations at far-infrared wavelengths between 0.06 and 0.6 millimetres. This means that GREAT operates in a spectral range that is inaccessible to ground-based observatories due to absorption by Earth's atmosphere. The modular design of the instrument allows the short-term installation of new technologies. Using GREAT on board the SOFIA airborne observatory, more than 150 successful research flights have been carried out since 2011. GREAT is a joint endeavour by the Max Planck Institute for Radio Astronomy in Bonn and KOSMA/University of Cologne, in conjunction with the DLR Institute of Optical Sensor Systems in Berlin.
Last modified:25/04/2019 18:08:47