Final answer:
The direct answer to the student's question cannot be provided due to missing information. Exoplanet positioning is often addressed through observation methods like transit photometry and radial velocity measurements, and understanding of orbital dynamics is enriched by Kepler's laws.
Step-by-step explanation:
The student's question seems to be missing vital information required to provide a direct answer regarding the position of an exoplanet. However, based on the provided context, we can delve into concepts of exoplanet observation and how one might determine a planet's position relative to its star. Without a specific diagram or additional details, it is important to note that the detection of exoplanets often involves methods such as transit photometry or radial velocity measurements, which can give us information about the exoplanet's orbit.
When considering questions about orbits and positioning of exoplanets, Kepler's laws of planetary motion often come into play. Kepler's second law, for example, states that a planet sweeps out equal areas in equal times. This means that an exoplanet in an elliptical orbit will move faster when it is closer to its star and slower when it is farther away. Therefore, if we're considering where an exoplanet spends most of its time during its orbit, it would generally spend more time farther from the star if its orbit is highly eccentric.
As for the direct answer to the question, it cannot be accurately provided without the diagram or specific details about the positions mentioned (Position 1, Position 2, etc.). However, the context suggests an interest in the dynamics of exoplanet orbits, which could be better explained with a complete scenario or visual representation.