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相关论文: Have mirror planets been observed?

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Due to their extremely small luminosity compared to the stars they orbit, planets outside our own Solar System are extraordinarily difficult to detect directly in optical light. Careful photometric monitoring of distant stars, however, can…

The hundreds of exoplanets that have been discovered in the past two decades offer a new perspective on planetary structure. Instead of being the archetypal examples of planets, those of our Solar System are merely possible outcomes of…

地球与行星天体物理 · 物理学 2015-06-18 David S. Spiegel , Jonathan J. Fortney , Christophe Sotin

We search for signatures of planets in 43 intensively monitored microlensing events that were observed between 1995 and 1999. Planets would be expected to cause a short duration (~1 day) deviation on the smooth, symmetric light curve…

Prior to the 1990s, speculations about the occurrence of planets around other stars were based only on planet formation theory, observations of circumstellar disks, and the knowledge that at least one seemingly ordinary star is the host of…

地球与行星天体物理 · 物理学 2024-01-31 Joshua N. Winn , Erik Petigura

We demonstrate that microlensing can be used for detecting planets in binary stellar systems. This is possible because in the geometry of planetary binary systems where the planet orbits one of the binary component and the other binary star…

天体物理学 · 物理学 2009-11-13 Dong-Wook Lee , Chung-Uk Lee , Byeong-Gon Park , Sun-Ju Chung , Young-Soo Kim , Ho-Il Kim , Cheongho Han

If planetary systems are ubiquitous then a fraction of stars should possess a transiting planet when being microlensed. This paper presents a study of the influence of such planets on microlensing light curves. For the giant planets…

天体物理学 · 物理学 2009-11-07 Geraint F. Lewis

Motivated by recent measurements of the free-floating planet mass function at terrestrial masses, we consider the possibility that the solar system may have captured a terrestrial planet early in its history. We show that $\sim 1.2$…

地球与行星天体物理 · 物理学 2023-12-15 Amir Siraj

We investigate compact objects formed by dark matter admixed with ordinary matter made of neutron star matter and white dwarf material. We consider non-self annihilating dark matter with an equation-of-state given by an interacting Fermi…

高能天体物理现象 · 物理学 2022-02-21 Laura Tolos , Juergen Schaffner-Bielich , Yannick Dengler

Since 1995, more than 500 exoplanets have been detected using different techniques, of which 11 were detected with gravitational microlensing. Most of these are gravitationally bound to their host stars. There is some evidence of…

The discovery of planetary systems beyond our solar system has challenged established theories of planetary formation. Planetary orbits display a variety of unexpected architectures, and free-floating planets appear ubiquitous. The recent…

地球与行星天体物理 · 物理学 2024-05-06 Yihan Wang , Rosalba Perna , Zhaohuan Zhu

We report the detection of eighteen Jovian planets discovered as part of our Doppler survey of subgiant stars at Keck Observatory, with follow-up Doppler and photometric observations made at McDonald and Fairborn Observatories,…

Mirror matter is predicted to exist if parity (i.e. left-right symmetry) is a symmetry of nature. Remarkably mirror matter is capable of simply explaining a large number of contemporary puzzles in astrophysics and particle physics…

高能物理 - 唯象学 · 物理学 2008-11-26 R. Foot

Four planets have recently been discovered by gravitational microlensing. The most recent of these discoveries is the lowest-mass planet known to exist around a normal star. The detection of planets in gravitational microlensing events was…

天体物理学 · 物理学 2009-11-11 Nicholas James Rattenbury

Recent observations have revealed two new classes of planetary orbits. Rossiter- Mclaughlin (RM) measurements have revealed hot Jupiters in high-obliquity orbits. In addition, direct-imaging has discovered giant planets at large (~ 100 AU)…

地球与行星天体物理 · 物理学 2015-05-20 Sourav Chatterjee , Eric B. Ford , Frederic A. Rasio

Are there other planetary systems in our Universe? Indirect evidence has been found for planets orbiting other stars in our galaxy: the gravity of orbiting planets makes the star wobble, and the resulting periodic Doppler shifts have been…

天体物理学 · 物理学 2007-05-23 Edward A. Baltz , Paolo Gondolo

The Einstein rings and proper motions of nearby stars tend to be large. Thus, every year some foreground stars within a few hundred parsecs of Earth induce gravitational lensing events in background stars. In some of these cases, the events…

地球与行星天体物理 · 物理学 2015-06-04 Rosanne Di Stefano , James Matthews , Sebastien Lepine

The study of extra-solar planetary systems has emerged as a new discipline of observational astronomy in the past few years with the discovery of a number of extra-solar planets. The properties of most of these extra-solar planets were not…

Specially-designed microlensing searches, some of which have been underway for several years, are sensitive to extrasolar planets orbiting the most common stars in our Galaxy. Microlensing is particularly well-suited to the detection of…

天体物理学 · 物理学 2007-05-23 Penny D. Sackett

Mirror matter type dark matter can exist on the Earth's surface, potentially in enhanced concentrations at various anomalous impact sites. Mirror matter fragments can draw in heat from the ordinary matter environment, radiate mirror photons…

凝聚态物理 · 物理学 2008-11-26 R. Foot , S. Mitra

This talk was given at the Tunguska-2001 international conference but it is not about the Tunguska event. Instead we tried to give some flavor of mirror matter, which is predicted to exist if parity is an unbroken symmetry of nature, to…

天体物理学 · 物理学 2007-05-23 Z. K. Silagadze