Hexbyte Glen Cove ‘Tatooine-like’ exoplanet spotted by ground-based telescope

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The image is an illustration made by Amanda Smith of the 193cm telescope at the Observatoire de Haute-Provence which was used for this research. This was the telescope that discovered the first exoplanet, 51 Pegasi b, which led to the Nobel Prize in Physics in 2019. In the sky the Kepler-16 circumbinary planet system is represented, along with a depiction of the field of view of NASA’s Kepler spacecraft. Credit: Amanda Smith

A rare exoplanet which orbits around two stars at once has been detected using a ground-based telescope by a team led by the University of Birmingham.

The planet, called Kepler-16b, has so far only been seen using the Kepler space telescope. It orbits around two , with the two orbits also orbiting one another, forming a . Kepler-16b is located some 245 from Earth and, like Luke Skywalker’s home planet of Tatooine, in the Star Wars universe, it would have two sunsets if you could stand on its surface.

The 193cm telescope used in the new observation is based at the Observatoire de Haute-Provence, in France. The team were able to detect the planet using the radial velocity method, in which astronomers observe a change in the velocity of a star as a planet orbits about it.

The detection of Kepler-16b using the radial velocity method is an important demonstration that it is possible to detect circumbinary planets using more traditional methods, at greater efficiency and lower cost than by using spacecrafts.

Importantly the is also more sensitive to additional planets in a system, and it can also measure the mass of a planet—its most fundamental property.

Having demonstrated the method using Kepler-16b, the team plans to continue the search for previously unknown circumbinary planets and help answer questions about how planets are formed. Usually, planets formation is thought to take place within a —a mass of dust and gas which surrounds a young star. However, this process may not be possible within a circumbinary system.

Professor Amaury Triaud, from the University of Birmingham, who led the team, explains: “Using this standard explanation it is difficult to understand how circumbinary planets can exist. That’s because the presence of two stars interferes with the protoplanetary disc, and this prevents dust from agglomerating into planets, a process called accretion.

“The planet may have formed far from the two stars, where their influence is weaker, and then moved inwards in a process called disc-driven migration—or, alternatively, we may find we need to revise our understanding of the process of planetary accretion.”

Dr. David Martin, from the Ohio State University (U.S.), who contributed to the discovery, explains “Circumbinary provide one of the clearest clues that disc-driven migration is a viable process, and that it happens regularly.”

Dr. Alexandre Santerne, from the University of Marseille, a collaborator on the research explains: “Kepler-16b was first discovered 10 years ago by NASA’s Kepler satellite using the transit method. This system was the most unexpected discovery made by Kepler. We chose to turn our telescope and recover Kepler-16 to demonstrate the validity of our radial-velocity methods.”

Dr. Isabelle Boisse, also from the University of Marseille, is the scientist in charge of the SOPHIE instrument that was used to collect the data. She said: “Our discovery shows how ground-based telescopes remain entirely relevant to modern exoplanet research and can be used for exciting new projects. Having shown we can detect Kepler-16b, we will now analyse data taken on many other binary star systems, and search for new .”

The research is published in Monthly Notices of the Royal Astronomical Society.

More information:
BEBOP III. Observations and an independent mass measurement of Kepler-16 (AB) b – the first circumbinary planet detected with radial velocities, Monthly Notices of the Royal Astronomical Society, DOI: 10.1093/mnras/stab3712

‘Tatooine-like’ exoplanet spotted by ground-based telescope (2022, February 23)
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Hexbyte Glen Cove Researchers fabricate co-doped aluminosilicate fiber with high laser stability for multi-kW level laser thumbnail

Hexbyte Glen Cove Researchers fabricate co-doped aluminosilicate fiber with high laser stability for multi-kW level laser

Hexbyte Glen Cove

Schematic diagram of MOPA configuration. Credit: XIOPM

Multi-kilowatt (kW) (≥3kW) level fiber lasers with high stability are significant in many applications, and Yb-doped fiber is the key device in such fiber lasers. The incredible advances of the past few decades in fiber fabrication technology have led to an exponential increase in the output power of continuous-wave (CW) fiber lasers. However, with further scaling the output power, photodarkening (PD) was found to be one of the critical limit factors for long-term laser reliability under multi kW level output power.

PD effect is manifested as an evolution process of pump-induced excess loss depending on pump power and dopant concentrations. It can be attributed to color centers that derive from the cooperative energy transfer process which is from excited Yb3+ to the atomic defect precursors in the fiber core. Co-doping Ce can strongly improve the PD resistance in Yb/Al co-doped fiber, despite the mechanism of PD resistance realized by co-doping Ce still has not been well understood yet.

SHE Shengfei, together with collaborators from the Xi’an Institute of Optics and Precision Mechanics (XIOPM) of the Chinese Academy of Sciences, fabricated a 30/600 active fiber with high laser stability, named as Yb/Ce-AS@LAS fiber by low-temperature chelate gas phase deposition (LT-CGPD) technique to synthetically evaluated Ce addition in multi-kW level Yb doped fiber. And finally, based on the Ce co-doped Yb/Al fiber, they demonstrated an excellent result at 1,079.80 nm. The works were published in the Journal of Lightwave Technology.

The researchers fabricated serial co-doped Yb/Al fibers with gradient Ce concentration and proved that the Ce addition can effectively improve the PD resistance of the fiber.

With the master oscillator power amplifier (MOPA) configuration, they successfully achieved the highest CW laser power of 5.04 kW output at 1079.80 nm with a slope efficiency of 81.1%. Simultaneously, the long-term stability of high-power fiber amplifiers was effectively improved at the same time, indicating the suppressing effects of Ce addition on PD and additional thermal load.

They didn’t only break a fiber power record, but also paved a way towards better commercial high- fiber lasers, based on the self-made Yb/Ce co-doped aluminosilicate fiber fabricated by LT-CGPD technique.

More information:
Shengfei She et al. Yb/Ce Codoped Aluminosilicate Fiber With High Laser Stability for Multi-kW Level Laser, Journal of Lightwave Technology (2020). DOI: 10.1109/JLT.2020.3019740

Researchers fabricate co-doped aluminosilicate fiber with high laser stability for multi-kW level laser (2020, November 27)
retrieved 29 November 2020
from https://phys.org/news/2020-11-fabricate-co-doped-aluminosilicate-fiber-high.html

This document is subject to copyright. Apart from any fair dea

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