694 Amy Apr 2026

Ekard is no mere pebble; it is a "silent giant" of the main belt. With an estimated diameter of approximately (about 76 miles), it is larger than 99% of all known asteroids. To put its size in perspective, it is roughly comparable to the size of the state of Connecticut. Key characteristics include:

Classified as a main-belt asteroid, it orbits at a safe distance from Earth—roughly 0.87 AU (about 81 million miles) at its closest point—and poses no threat of impact. Scientific Significance 694 Amy

For astronomers, 694 Ekard is a valuable subject for . By studying its "light curve"—the way its brightness varies as it rotates—scientists have been able to model its three-dimensional shape and determine its thermal inertia. These measurements, which range between 100–140 J m⁻² K⁻¹ s⁻¹/², help researchers understand the texture and composition of its surface, comparing it to substances like lunar regolith or coarse sand. Ekard is no mere pebble; it is a

694 Ekard stands as a fascinating bridge between the historical era of visual discovery and the modern era of precision astrophysics. From its whimsical origin story at Drake University to its status as one of the largest residents of the asteroid belt, it continues to provide essential data about the "rocky relics" of our solar system's origins. While it may not be a target for human exploration anytime soon, it remains a vital piece of the celestial puzzle, drifting silently in the dark. These measurements, which range between 100–140 J m⁻²

Ekard is a fast spinner, completing a rotation on its axis in just 5.93 hours .

Furthermore, Ekard has been the subject of multiple . In 2009 alone, four separate events were observed where the asteroid passed in front of a star, allowing observers to refine its diameter and shape with high precision. Conclusion