Laser 'ruler' holds promise for hunting exoplanets

Phys.Org ^ | 02-17-2015 | Provided by Institute of Physics

[Red Badger]

The hunt for Earth-like planets around distant stars could soon become a lot easier thanks to a technique developed by researchers in Germany.

In a paper published today, 18 February, in the New Journal of Physics, the team of researchers have successfully demonstrated how a solar telescope can be combined with a piece of technology that has already taken the physics world by storm—the laser frequency comb (LFC).

It is expected the technique will allow a spectral analysis of distant stars with unprecedented accuracy, as well as advance research in other areas of astrophysics, such as detailed observations of the Sun and the measurement of the accelerating universe by observing distant quasars.

The LFC is a tool for measuring the colour—or frequency—of light, and has been responsible for generating some of the most precise measurements ever made. An LFC is created by a laser that emits continuous pulses of light, containing millions of different colours, often spanning almost the entire visible spectrum.

When the different colours are separated based on their individual frequencies—the speed with which that particular light wave oscillates—they form a "comb-like" graph with finely spaced lines, or "teeth", representing the individual frequencies.

This "comb" can then be used as a "ruler" to precisely measure the frequency of light from a wide range of sources, such as lasers, atoms or stars.

In their study, the researchers, from the Max Planck Institute of Quantum Optics, the Kiepenheuer Institute for Solar Physics and the University Observatory Munich, performed an analysis on the Sun by combining sunlight from the Kiepenheuer Institute's solar telescope in Tenerife with the light of an LFC. Both sources of light were injected into a single optical fibre which then delivered the light to a spectrograph for analysis.

Lead author of the study Rafael Probst, of the Max Planck Institute of Quantum Optics, said: "An important aspect of our work is that we use a single-mode fibre, which takes advantage of the wave nature of light to enable a very clean and stable beam at its output. This type of fibre is quite common in telecom and laser applications, but its applications in astronomy are still largely unexplored. The LFC at the solar telescope on Tenerife is the first installation for astronomical use based on single-mode fibres.

"Our results show that if the LFC light and the sunlight are simultaneously fed through the same single-mode fibre, the obtained calibration precision improves by about a factor of 100 over a temporally separated fibre transmission.

"We then obtain a calibration precision that keeps up with the best calibration precision ever obtained on an astrophysical spectrograph, and we even see considerable potential for further improvement."

Indeed, the researchers envisage using the new technique to not only study the star at the centre of our solar system, but stars much further away from us, particularly to find Earth-like planets that may be orbiting around them.

When a planet orbits a star, the star does not stay completely stationary, but instead moves in a very small circle or ellipse. When viewed from a distance, these slight changes in speed cause the star's light spectrum to change—a process known as a Doppler shift.

If the star is moving towards the observer, then its spectrum would appear slightly shifted towards the blue end of the spectrum; if it is moving away, it will be shifted towards the red end of the spectrum.

The researchers believe that an LFC would allow them to measure these Doppler shifts much more accurately and therefore increase the chances of spotting Earth-sized, habitable planets.

With conventional calibration techniques, the researchers state that they could measure a change in speed of roughly 1 m/s over large time periods; an LFC could enable measurements with an accuracy of 1 cm/s.

"In astronomy, LFCs are still a novelty and non-standard equipment at observatories. This however, is about to change, and LFC-assisted spectroscopy is envisioned to have a flourishing future in astronomy. Our present work shows how future astronomical LFCs could be utilized," Probst concludes.

Explore further: New optical device designed to measure gravitational pull of a planet should speed the search for Earth-like exoplanets

More information: 'Comb-calibrated solar spectroscopy through a multiplexed single-mode fiber channel' R A Probst et al 2015 New J. Phys. 17 023048. 18 February, 2015. iopscience.iop.org/1367-2630/17/2/023048

Journal reference: New Journal of Physics Provided by Institute of Physics

Read more at: http://phys.org/news/2015-02-laser-ruler-exoplanets.html#jCp

[Red Badger]

A "Laser Frequency Comb". Credit: Rafael Probst

Vacuum Tower Telescope in Tenerife. Credit: Prof. Wolfgang Schmidt

This could be huge........................

[Red Badger]

Space, astronomy and exoplanet ping!.........................

[Red Badger]

This method could also be used to find GRAVITY WAVES.........................Easily........................

[JoeFromSidney]

This method could also be used to find GRAVITY WAVES

The search for gravity waves has been going on for a long time. When I was assigned to Air Force Office of Scientific Research, back in the 1960s, we were supporting the work of a gravity wave researcher at University of Maryland. One day I visited his lab. I saw that he had an auto license plate attached to the outside of his instrument. He remarked that it was the only licensed gravity wave detector in Maryland.

[Red Badger]

To use it as a Gravity Wave Detector, ironically, you would have to find a star with no planets, or some that were too small to be a problem.

Fix the star’s light onto the detector for a long period of time, monitored 24 / 7 / 365.

Examine the red / blue shift to get a ‘constant’ value to be used as the ‘reference’.

If it changes, to the red or blue direction, with no planets interfering, then a gravity wave must have passed between you, the observer, and the star being studied...........................sound okay?................

[SunkenCiv]

Thanks Red Badger.

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