Astronomy or Astrophysics? A Guide to Help You Decide What to Study

Astronomy and astrophysics are closely related fields that often overlap, but they have distinct focuses and approaches. Here’s a breakdown of the differences between the two:

Astronomy

Astronomy is the broader science that involves the study of celestial objects and phenomena beyond Earth’s atmosphere. It includes the observation and analysis of stars, planets, comets, galaxies, and other celestial bodies. Primarily observational, using telescopes and other instruments to gather data about the universe. Includes planetary astronomy, stellar astronomy, galactic astronomy, and observational cosmology.

Astrophysics

Astrophysics is a branch of astronomy that applies the principles of physics and chemistry to understand how celestial objects and phenomena work. Focuses on celestial bodies’ underlying physical processes and properties, such as their formation, evolution, and behavior. Combines observational data with theoretical models and simulations to explain the physical mechanisms at play. Includes cosmology (the study of the universe’s origin and evolution), stellar dynamics, planetary science, and high-energy astrophysics.

Key Differences

Astronomy is often more observational, cataloging and describing what is seen in the sky. Astrophysics seeks to explain these observations through physical theories. Astronomers might spend more time on practical aspects like telescope design, data collection, and image processing. Astrophysicists might spend more time on theoretical work and modeling.

In summary, while astronomy and astrophysics are intertwined, astronomy is more focused on the observation and cataloging of celestial objects, whereas astrophysics is dedicated to understanding the physical processes that govern these objects and phenomena.

The Sub-Neptune Radius Valley: A Preview of Our New Module “The Solar System and Exoplanets”

Excited for the second year of our new Physics with Astrophysics degree program at the University of Lincoln! Right now, I’m fully immersed, working on one of our new modules called “The Solar System and Exoplanets.” We’re diving deep into how planets form and trying to unravel the mystery of the huge variety of exoplanets we keep discovering. Check out this quick video for a taste of what we’re digging into in the module.


The apparent lack of planets with radii 1.5–2 times that of Earth is known as the Sub-Neptune radius valley. First noted in 2011, a bimodality in the Kepler exoplanet population was ascribed to the lack of substantial gas atmospheres on close-in, low-mass planets. It was mentioned that this trait could support the growing theory that atmospheric mass loss could be caused by photoevaporation. This would result in a population of planets with thick envelopes dominated by helium and hydrogen with bigger radii at higher separations from their parent stars, and a population of naked, rocky cores with lower radii at small separations.

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