Image Credit: NASA Jet Propulsion Laboratory
99942 Apophis is a massive Potentially Hazardous Asteroid (PHA) approximately 350 meters in diameter. While high-precision modeling has ruled out a terrestrial impact for the next century, its upcoming transit remains a landmark event due to its immense scale and extreme proximity. It is a once-in-a-millennium encounter that places a 27 billion kilogram celestial body deep within the Earth-Moon system.
On April 13, 2029, Apophis will pass within 30,600 kilometers of the Earth’s surface – closer than the geostationary satellites used for global telecommunications. This proximity is unprecedented for an object of this magnitude. As it passes, Earth’s gravitational pull will exert intense tidal forces on the asteroid, potentially triggering “asteroid quakes” and physically altering its surface regolith in real-time.
The 2029 close approach of the asteroid Apophis represents a historic intersection of deep-space research and public observation. From a scientific perspective, the asteroid’s proximity makes it a "low-hanging fruit" for study; the exceptionally low energy change, or delta-V, required for a spacecraft to rendezvous with it offers a high-efficiency opportunity for exploration. This encounter will also permanently redefine the asteroid’s identity, as Earth’s gravitational "slingshot" shifts its trajectory from an Aten-type to an Apollo-type orbit for the first time in millennia.
Beyond its orbital mechanics, the event will be a global spectacle. Reaching a visual magnitude of 3.1, Apophis will be bright enough to see with the naked eye – shining as clearly as the stars in the Big Dipper. While the most dramatic views will occur over Africa and Western Europe, observers in the United States will be able to spot the asteroid as a fast-moving "star" appearing immediately after sunset.
Image Credit: NASA Jet Propulsion Laboratory
Preliminary Render of TERP RAPTOR
Mission Goal: First-of-its-kind dual-flyby mass measurement, high resolution surface images, and first arrival at Apophis.
Form Factor: 12U CubeSat (roughly the size of a microwave).
Primary Payloads: Monochrome Snapshot Imager for surface detail, and Retroreflector Panels for precise tracking & mass measurement.
Status: Currently in the advanced conceptual design phase, with a targeted encounter for late 2028.
Asteroid mass is the most important physical characteristic to measure for planetary defense missions.
Our laser-based technique will measure asteroid mass 7 times more accurately than cameras and spectrometers alone.
This demonstration will be the first ever high-speed flyby mass measurement of an asteroid of Apophis's size.
The data our mission provides about Apophis's mass, shape, and surface features will help us understand the asteroid's gravity field and rotational dynamics. This information will give other missions to Apophis, like ESA's RAMSES and NASA's OSIRIS-APEX, a significant head-start in refining their proximity operations plans before they reach the asteroid.
The images we collect will also be shared publicly. When Apophis makes its flyby of Earth on April 13th, 2029, the world will know what the bright light zooming across sky actually is.