Yes, it is highly likely that we will eventually obtain high-resolution and detailed images of exoplanets in the future. While current technology and observational methods have allowed us to detect and characterize many exoplanets indirectly, such as through the transit method or radial velocity measurements, directly imaging these distant worlds presents a significant challenge.
Obtaining detailed images of exoplanets is challenging due to several factors. First, exoplanets are incredibly faint compared to their host stars, making it difficult to isolate their light from the overwhelming glare of the star. Second, the vast distances between us and these planets make it even more challenging to capture detailed images.
However, advancements in technology and observational techniques are continually being made, and there are several ongoing efforts to improve our ability to directly image exoplanets. Instruments like the James Webb Space Telescope (JWST), which is scheduled to launch in late 2021, will have the capability to observe and characterize exoplanet atmospheres, providing valuable information about their composition.
Additionally, new ground-based observatories and space missions specifically designed for exoplanet imaging are being planned. These future missions, equipped with advanced adaptive optics, coronagraphs, and other innovative technologies, aim to overcome the technical difficulties and capture higher-resolution images of exoplanets.
While it is difficult to predict an exact timeline, given the rapid pace of technological advancements, it is reasonable to expect that we will eventually achieve the capability to capture detailed images of exoplanets in the coming decades. These images will greatly enhance our understanding of these distant worlds and provide valuable insights into their atmospheres, surfaces, and potential habitability.