OSIRIS-REx to study Asteroid Apophis

Context (LM): The former OSIRIS-REx spacecraft sets off on a (seven-year, 4 billion-mile journey) journey to study asteroid Apophis.

Asteroid Apophis

Asteroid Apophis is better known as the ‘God of Chaos’.
It is a near-Earth object (NEO) estimated to be about 1,100 feet (340 meters) across.
Asteroid Apophis is made of silicate materials and nickel-iron (different from carbon-rich, “C-type” Bennu).
It originated in the main asteroid belt between Mars and Jupiter.

Why Study Apophis?

Discovered in 2004, Apophis gained notoriety as one of the most hazardous asteroids that could impact Earth.
Apophis is expected to “safely pass close to Earth on April 13, 2029, the closest approach to Earth by an asteroid of this size that scientists have known about in advance.
Apophis’ close encounter with Earth is expected to change the asteroid’s orbit and the length of its 30.6-hour day.
It was officially taken off from NASA’s Potentially Hazardous Asteroids list (PHAs).

PHAs are currently defined based on parameters that measure the asteroid’s potential to make threatening close approaches to the Earth.
All asteroids with a Minimum Orbit Intersection Distance (MOID) of 0.05 au or less and an absolute magnitude (H) of 22.0 or less are considered PHAs.

Asteroids

Asteroids are small, rocky objects that orbit the Sun like planets, but they are much smaller than planets and are irregular shaped (not all round like planets).
Formed around 4.6 billion years ago, they are remnants of protoplanetary disk- the cloud of gas and dust from which the sun and planets formed.
Size: Some are tiny, only a few metres across while others can be several kilometres wide.
Types:
1. C-type (Carbonaceous) Asteroids: They make up 75% of the known asteroids.
2. S-type (Silicate or Stony) Asteroids: They account for 17% of known asteroids.
3. M-type (Metallic) Asteroids: They are made up of nickel-iron and are found in the middle region of the asteroid belt.
Asteroids are divided into three categories:
1. Asteroids in the main asteroid belt, between Mars and Jupiter.
2. Trojans (name comes from Greek mythology), which are asteroids that share an orbit with a larger planet.
3. Near-Earth Asteroids (NEA): It has orbits that pass close to the Earth.
  - Earth Crossers: Those that cross the Earth’s orbit. More than 10,000 such asteroids are known, of which over 1,400 are classified as potentially hazardous asteroids (PHAs).

OTHER ASTEROID MISSIONS

Galileo mission (NASA)

It was the first spacecraft to fly past asteroids Gaspara in 1991 and Ida in 1993.

Near Earth Asteroid Rendezvous (NEAR) mission (NASA)

It was the first spacecraft to successfully orbit Eros, an asteroid near Earth, and also land on the asteroid.

Mission Lucy (NASA)

For exploring Jupiter Trojan asteroids.

Dawn Mission (NASA)

It aims to study 2 out of 3 protoplanets in the asteroid belt between Mars and Jupiter i.e. Vesta and Ceres (Pallas is 3^rd).

Dawn is the 1^st to visit any dwarf planet (i.e. Ceres), the first to orbit a body in the region between Mars and Jupiter (Vesta), and the only mission ever to orbit two extra-terrestrial targets.

Hera Mission (European Space Agency [ESA])

It is an asteroid deflection mission which is scheduled to be launched in 2024 to measure the impact crater produced by the DART collision and study the change in the asteroid’s orbital trajectory. It will arrive at the Didymos system in 2027.

AIDA mission (NASA & ESA)

It is a technology demonstration of the kinetic impactor concept to deflect a small asteroid and to characterize its physical properties.

Kinetic impaction involves sending one or more large, high-speed spacecraft into the path of an approaching near-earth object.
This could deflect the asteroid into a different trajectory, steering it away from Earth’s orbital path.

Hayabusa Mission (Japan Aerospace Exploration Agency [JAXA])

By Japan Aerospace Exploration Agency (JAXA).

Hayabusa brought back samples from asteroid “Itokawa” to help elucidate the origin of the solar system.
Hayabusa 2 targets asteroid “Ryugu” to study the origin and evolution of the solar system.