This review presents an insight into our current knowledge of the atmospheres of the planets Venus, Mars, Jupiter, Saturn, Uranus and Neptune, the satellite Titan, and those of exoplanets. It deals with the thermal structure, aerosol properties (hazes and clouds, dust in the case of Mars), chemical composition, global winds, and selected dynamical phenomena in these objects. Our understanding of atmospheres is greatly benefitting from the discovery in the last 3 decades of thousands of exoplanets. The exoplanet properties span a broad range of conditions, and it is fair to expect as much variety for their atmospheres. This complexity is driving unprecedented investigations of the atmospheres, where those of the solar systems bodies are the obvious reference. We are witnessing a significant transfer of knowledge in both directions between the investigations dedicated to Solar System and exoplanet atmospheres, and there are reasons to think that this exchange will intensity in the future. We identify and select a list of research subjects that can be conducted at optical and infrared wavelengths with future and currently available ground-based and space-based telescopes, but excluding those from the space missions to solar system bodies.

这篇评论深入了解了我们目前对金星、火星、木星、土星、天王星和海王星、卫星泰坦以及系外行星大气层的了解。它涉及热结构、气溶胶特性（火星上的雾霾和云、灰尘）、化学成分、全球风以及这些物体中选定的动力学现象。我们对大气层的了解极大地受益于过去三十年中数千颗系外行星的发现。系外行星的特性涵盖了广泛的条件，并且可以合理地期望它们的大气层具有同样多的多样性。这种复杂性正在推动对大气层进行前所未有的研究，其中太阳系天体的大气层是明显的参考。我们正在见证太阳系和系外行星大气研究之间双向的重大知识转移，并且有理由认为这种交流在未来将会加强。我们确定并选择了一系列研究主题，这些主题可以使用未来和当前可用的地基和天基望远镜在光学和红外波长下进行，但不包括那些来自太阳系天体太空任务的研究主题。