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Modelling techniques for the propagation of light pollution in the atmosphere allow the computation of maps of artificial night sky brightness in any direction of the sky, involving a large number of details from satellite data. Cinzano et…

天体物理仪器与方法 · 物理学 2020-07-02 Pierantonio Cinzano , Fabio Falchi

The visual perception of the natural night sky in many places of the world is strongly disturbed by anthropogenic light. Part of this artificial light is scattered in the atmosphere and propagates towards the observer, adding to the natural…

天体物理仪器与方法 · 物理学 2023-05-02 Salvador Bará , Carmen Bao-Varela

Ground-based optical astronomy necessarily involves sensing the light of astronomical objects along with the contributions of many natural sources ranging from the Earth's atmosphere to cosmological light. In addition, astronomers have long…

天体物理仪器与方法 · 物理学 2022-08-31 John C. Barentine

Presence of dust in galaxies removes half or more of the stellar energy from the UV-optical budget of the Universe and has profound impact on our understanding of how galaxies evolve. Measures of opacity in local galaxies are reviewed…

天体物理学 · 物理学 2008-11-26 Daniela Calzetti

Artificial light at night is a pollutant that is rising fast, as demonstrated by Kyba et al. (1) work by analyzing ten of thousands observations by citizen scientists in the last 12 years. The study found that the dimmest stars are…

天体物理仪器与方法 · 物理学 2023-07-03 Fabio Falchi , Salvador Bará

The selective light absorption in space has been raised in astronomical literature. The substance producing the absorption must have some mass; thus the question is how large it is. We develop a dynamical model of the Milky Way system,…

星系天体物理 · 物理学 2022-03-29 E. Öpik

Artificial light at night has affected most of the natural nocturnal landscapes worldwide and the subsequent light pollution has diverse effects on flora, fauna and human well-being. To evaluate the environmental impacts of light pollution,…

天体物理仪器与方法 · 物理学 2020-02-24 Andreas Jechow , Franz Hölker , Christopher C. M. Kyba

Massive stars are at the core of our observations of the Universe up to the reionization epoch, both through their intense ionizing fluxes and through the energetic end products that release fresh elements into the interstellar medium. Our…

Europe and a number of countries in the world are investing significant amounts of public money to operate and maintain large, ground-based astronomical facilities. Even larger projects are under development to observe the faintest and most…

天体物理仪器与方法 · 物理学 2010-11-30 F. Patat

Unfettered access to dark night skies is rapidly diminishing, due to light pollution and satellite mega-constellations tracks. Scientists should wake up and do more to stand up to Big Light and Big Space and preserve this natural resource.

物理与社会 · 物理学 2023-07-10 Fabio Falchi , Salvador Bará , Pierantonio Cinzano , Raul C. Lima , Martin Pawley

Under stable atmospheric conditions, the zenithal brightness of the urban sky varies throughout the night following the time course of the anthropogenic emissions of light. Different types of artificial light sources (e.g. streetlights,…

The sustained increase of emissions of artificial light is causing a progressive brightening of the night sky in most of the world. This process represents a threat for the long-term sustainability of the scientific and educational activity…

天体物理仪器与方法 · 物理学 2020-12-29 Fabio Falchi , Salvador Bará

The interpretation of observations over different wavelength domains, which now exist over a large fraction of the sky, will be used to determine relationships between a nebula and its' illuminating source. The illuminating source of a high…

天体物理学 · 物理学 2009-10-31 F. Zagury

Diffuse glow has been observed around brightly lit cities in nighttime satellite imagery since at least the first publication of large scale maps in the late 1990s. In the literature, this has often been assumed to be an error related to…

天体物理仪器与方法 · 物理学 2020-05-12 Alejandro Sánchez de Miguel , Christopher C. M. Kyba , Jaime Zamorano , Jesús Gallego , Kevin J. Gaston

There is a longstanding discussion about whether low mass stars can form from pristine gas in the early Universe. A particular point of interest is whether we can find surviving pristine stars from the first generation in our local…

星系天体物理 · 物理学 2019-05-08 Mattis Magg , Ralf S. Klessen , Simon C. O. Glover , Haining Li

If stars at the lower end of the main sequence are responsible for the microlensing events observed in the Galactic bulge, then light from the lensing star contributes to the observed brightness. The background and lensing stars generally…

天体物理学 · 物理学 2009-10-22 Marc Kamionkowski

Results of the first comprehensive light pollution survey in Hong Kong are presented. The night-sky brightness was measured and monitored around the city using a portable light sensing device called the Sky Quality Meter over a 15-month…

天体物理仪器与方法 · 物理学 2012-03-05 Chun Shing Jason Pun , Chu Wing So

Recent observations suggest appreciable star formation activity in early-type galaxies down to redshift $z\sim 0.5$. If so, there is likely to be dust in these galaxies. We consider the possibility that obscuration by dust can reconcile the…

天体物理学 · 物理学 2007-05-23 M. Fukugita , P. J. E. Peebles

Evidence of the negative impact of light pollution on ecosystems is increasing every year. Its monitoring and study requires the identification, characterisation and control of the emitting sources. This is the case of urban centres with…

Measuring the brightness of the night sky has become an increasingly important topic in recent years, as artificial lights and their scattering by the Earths atmosphere continue spreading around the globe. Several instruments and techniques…

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