Didier Queloz is a Swiss astrophysicist renowned for his contributions to the field of exoplanet research. He is best known for his work in the discovery of the first exoplanet orbiting a sun-like star, which he achieved in 1995 alongside Michel Mayor. This groundbreaking discovery was significant in the field of astronomy, as it opened up new avenues for the study of planets outside our solar system and sparked interest in the search for potentially habitable worlds.

J. Hans D. Jensen is likely referring to Johannes Hans Daniel Jensen, a German physicist who was awarded the Nobel Prize in Physics in 1963 for his work on the structure of atomic nuclei. Jensen's contributions played a significant role in the development of nuclear physics and understanding how protons and neutrons are arranged within the nucleus. He was known for his research in nuclear shell models, which helped explain the behavior of atomic nuclei.

Lists of minor planets by name are collections or databases that categorize and provide information on minor planets (also known as asteroids) according to their designated names. Minor planets are small celestial bodies that orbit the Sun and are not classified as comets. These lists typically include the name of the minor planet, its numerical designation, discovery date, and sometimes additional information such as its orbital characteristics, physical properties, and the name of the astronomer or observatory that discovered it.

Mars-crossing minor planets are asteroids that have orbits that can cross the orbit of Mars. This means that their paths around the Sun bring them into the vicinity of Mars' orbit. These asteroids can potentially be classified as part of the broader group of near-Earth objects (NEOs) since their orbits may bring them close to Earth as well.

A "lost minor planet" refers to an asteroid or similar small celestial body that was once observed and cataloged but has not been seen or located in recent years, making it difficult to determine its current orbit and position. This can happen due to a variety of reasons, including factors such as faint brightness, observational limitations, or changes in the minor planet's orbital path over time.

The list of fast rotators among minor planets refers to celestial bodies, primarily asteroids, that have relatively short rotation periods, meaning they complete a full spin on their axis in a short amount of time. These fast rotators can have rotation periods of less than about 5 hours. Studying fast rotators is significant because their rapid spins can affect their shapes, sizes, and surface features due to the centripetal forces at play.

The term "slow rotators" in the context of minor planets refers to asteroids that have a long rotation period, meaning they take a significant amount of time—often more than 10 hours—to complete a full rotation on their axis. This characteristic can be influenced by various factors, including the object's size, shape, and internal structure.

Neptune, the eighth planet from the Sun, has a total of 14 known moons. The most notable of these moons are: 1. **Triton**: This is the largest moon of Neptune and the seventh-largest moon in the solar system. Triton is unique because it has a retrograde orbit, meaning it orbits Neptune in the opposite direction of the planet's rotation. It is composed mostly of water ice and has a thin atmosphere.

The naming of moons, or natural satellites, typically follows specific conventions set by the International Astronomical Union (IAU), which is the organization responsible for naming celestial bodies. Here are some key points regarding how moons are named: 1. **Naming Conventions**: Moons are often named after mythological figures, particularly from Roman and Greek mythology. For example, many of Jupiter's moons are named after lovers and descendants of Zeus (the Greek equivalent of Jupiter).

On Venus, "coronae" are large, circular features that are believed to be formed by volcanic and tectonic processes. They typically consist of a ring of mountains surrounding a depression and are thought to represent the interaction of magma with the planet's lithosphere. The study of coronae on Venus is essential for understanding its geological history and the processes that shape its surface. There are over 100 identified coronae on the planet, and they vary widely in size, shape, and geological complexity.

Venus, often referred to as Earth's "sister planet" due to its similar size and composition, has a surface marked by numerous craters. These craters vary widely in size and age, providing insights into the geological history of the planet. The following is a list of notable craters on Venus: 1. **Maxwell Montes** - The largest mountain range on Venus, it includes several craters.

In planetary geology, "montes" refers to mountain ranges or mountain-like features on a planet's surface. Venus has several mountainous regions characterized by its distinct geology. The following is a list of some notable montes on Venus: 1. **Maxwell Montes** – The tallest mountain range on Venus, located in the Ishtar Terra region. 2. **Phoebe Region** – Home to Phoebe Mons, another prominent mountainous feature.

The "terrae" on Venus refer to large landmasses or highland regions on the planet's surface. These elevated areas are analogous to continents on Earth and are characterized by various geological features. Here is a list of the major terrae on Venus: 1. **Aphrodite Terra** - One of the largest highland regions, it covers a significant portion of the planet and is located in the southern hemisphere.