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Alpha Centauri A is the closest solar-type star to the Sun and offers an excellent opportunity to detect the thermal emission of a mature planet heated by its host star. The MIRI coronagraph on JWST can search the 1-3 AU (1"-2") region…

$\alpha$ Centauri A is the closest solar-type star to the Sun and offers the best opportunity to find and ultimately to characterize an Earth-sized planet located in its Habitable Zone (HZ). Here we describe initial results from an ALMA…

太阳与恒星天体物理 · 物理学 2021-06-23 Rachel Akeson , Charles Beichman , Pierre Kervella , Edward Fomalont , G. Fritz Benedict

Alpha Centauri is a triple stellar system, and it contains the closest star to Earth (Proxima Centauri). Over the last decades, the stars in Alpha Cen and their orbits have been investigated in great detail. However, the possible scenarios…

地球与行星天体物理 · 物理学 2024-01-30 Nicolás Cuello , Mario Sucerquia

Our nearest stellar neighbour, Proxima Centauri, is a low mass star with spectral typedM5.5 and hosting an Earth-like planet orbiting within its habitable zone. However, the habitability of the planet depends on the high-energy radiation of…

太阳与恒星天体物理 · 物理学 2020-09-02 S. Lalitha , J. H. M. M. Schmitt , K. P. Singh , P. C. Schneider , R. O. Parke Loyd , K. France , P. Predehl , V. Burwitz , J. Robrade

The Vega planetary system hosts the archetype of extrasolar Kuiper belts, and is rich in dust from the sub-au region out to 100's of au, suggesting intense dynamical activity. We present ALMA mm observations that detect and resolve the…

The presence of debris disks around $\sim$ 1-Gyr-old main sequence stars suggests that an appreciable amount of dust may persist even in mature planetary systems. Here we report the detection of dust emission from 55 Cancri, a star with…

We present 1.3 mm observations of the Sun-like star $\tau$ Ceti with the Atacama Large Millimeter/submillimeter Array (ALMA) that probe angular scales of $\sim1$'' (4 AU). This first interferometric image of the $\tau$ Ceti system, which…

Low mass stars might offer today the best opportunities to detect and characterise planetary systems, especially those harbouring close-in low mass temperate planets. Among those stars, TRAPPIST-1 is exceptional since it has seven…

地球与行星天体物理 · 物理学 2020-02-05 S. Marino , M. C. Wyatt , G. M. Kennedy , M. Kama , L. Matrà , A. H. M. J. Triaud , Th. Henning

A new planet has been recently discovered around Proxima Centauri. With an orbital separation of $\sim$$1.44$ au and a minimum mass of about $7$ $M_{\oplus}$, Proxima c is a prime direct imaging target for atmospheric characterization. The…

Proxima Centauri is known to host an earth-like planet in its habitable zone; very recently a second candidate planet was proposed based on radial velocities. At quadrature, the expected projected separation of this new candidate is larger…

Proxima Centauri is known as the closest star from the Sun. Recently, radial velocity observations revealed the existence of an Earth-mass planet around it. With an orbital period of ~11 days, the surface of Proxima Centauri b is temperate…

Proxima Centauri (Cen) has been the subject of many flaring studies due to its proximity and potential to host habitable planets. The discovery of millimeter flares from this M dwarf with ALMA has opened a new window into the flaring…

Proxima Centauri is the closest star to the Sun. This small, low-mass, mid M dwarf is known to host an Earth-mass exoplanet with an orbital period of 11.2 days within the habitable zone, as well as a long-period planet candidate with an…

The newly detected Earth-mass planet in the habitable zone of Proxima Centauri could potentially host life - if it has an atmosphere that supports surface liquid water. We show that thermal phase curve observations with the James Webb Space…

地球与行星天体物理 · 物理学 2016-11-23 Laura Kreidberg , Abraham Loeb

Millimeter emission from debris disks around stars of different ages provides constraints on the collisional evolution of planetesimals. We present ALMA 1.3 millimeter observations of a sample of 76 Solar-type stars in the ~115 Myr old…

地球与行星天体物理 · 物理学 2022-08-31 Devin Sullivan , David Wilner , Luca Matra , Mark C. Wyatt , Sean M. Andrews , Meredith A. MacGregor , Brenda Matthews

Due to its Earth-like minimum mass of 1.27 M$_{\text{E}}$ and its close proximity to our Solar system, Proxima Centauri b is one of the most interesting exoplanets for habitability studies. Its host star, Proxima Centauri, is however a…

地球与行星天体物理 · 物理学 2020-04-21 M. Scheucher , K. Herbst , V. Schmidt , J. L. Grenfell , F. Schreier , S. Banjac , B. Heber , H. Rauer , M. Sinnhuber

The discovery of a planet orbiting around Proxima Centauri, the closest star to the Sun, opens new avenues for the remote observations of the atmosphere and surface of an exoplanet, Proxima b. To date, three-dimensional (3D) General…

地球与行星天体物理 · 物理学 2021-03-24 Daniele Galuzzo , Chiara Cagnazzo , Francesco Berrilli , Federico Fierli , Luca Giovannelli

Most debris discs consist of a gas-poor, cold dust belt located tens to hundreds of astronomical units away from the host star. Many cold dust belts exhibit distinct structures attributed to the dynamic interaction of planetary systems.…

地球与行星天体物理 · 物理学 2024-04-09 Qiancheng Yang , Qiong Liu , Grant M. Kennedy , Mark C. Wyatt , Sarah Dodson-Robinson , Rachel Akeson , Nenghui Liao

We present new analyses of ALMA 12-m and ACA observations at 233 GHz (1.3 mm) of the Proxima Centauri system with sensitivities of 9.5 and 47 $\mu$Jy beam$^{-1}$, respectively, taken from 2017 January 21 through 2017 April 25. These…

地球与行星天体物理 · 物理学 2018-03-14 Meredith A. MacGregor , Alycia J. Weinberger , David J. Wilner , Adam F. Kowalski , Steven R. Cranmer
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