Spacecraft have visited the asteroids and increased our knowledge of these space critters that are so close to us, yet so far away.

Today's spacecraft exploring asteroids are the precursors to mining missions and have propelled us on our way to becoming capable of influencing the course of asteroids in the solar system!

Spacecraft Target Asteroids!

Many space probes have been sent to explore asteroids or as secondary targets for primary missions to comets. Comet missions are not discussed in the NEA pages. For information and links on comets please use Astra's Comets page.

Active Asteroid Missions and Flybys

Information on asteroid missions has been extracted from the websites that are linked in the short mission descriptions below. This section contains information on all asteroid missions, not necessarily Earth crossers. Please contact Astra with any omissions.

Other Links for Asteroid Missions

Active Asteroid Missions

OSIRIS-REx

Origins Spectral-Interpretation Resource-Identification Security Regolith Explorer (OSIRIS-REx)

The OSIRIS-REx spacecraft launched Sept. 8, 2016, from Cape Canaveral. It reached its target asteroid 101955 Bennu in September 2018. The plan is that it will land and bring back a sample (60 grams or 2.1 ounces) to aid investigation of solar system planet formation and the origin of life. It is hoped that the data collected will also increase our knowledge of asteroids that can impact Earth. The landing on Bennu is planned for October 20, 2020. Samples should be returned to Earth by September 24, 2023.

OSIRIS-REx began its two-year cruise home carrying with it the first asteroid sample on May 10, 2021.

OSIRIS-REx has discovered that Bennu contains material that came from the asteroid Vesta. The material from Vesta is brighter than that on the dark asteroid Bennu. Spectral analysis shows that pyroxene is present in the material. As soon as the spacecraft arrived at Bennu, scientist Carl Hergenrother spotted particles flying off the asteroid. Bennu is releasing particles into space on a regular basis, particles 0.5 - 1 cm in size. Most of these fall back to the surface of the asteroid.

The Planetary Society ran a contest "Name that asteroid!" to find a name for the asteroid that mission planners choose for the OSIRIS-REx mission, 1999 RQ36. The asteroid was renamed Bennu by a 9 year old boy, Michael Puzio. Bennu was a large heron that was symbol of the Egyptian god, Osiris. More information can be found on the Planetary Society site and the OSIRIS-REx page.

Messages to Bennu
NASA and the Planetary Society invited people from around the world to submit their names for a round-trip voyage to asteroid Bennu, the target of the OSIRIS-REx mission.

Find OSIRIS-REx mission news from University of Arizona at: OSIRIS-REx Status

HAYABUSA 2

Hayabusa2's Sample-Return Capsule is expected to land on Earth on December 6, 2020!

JAXA logo for Hayabusa 2 asteroidmission

Hayabusa is the Japanese word for peregrine falcon. The Hayabusa2 spacecraft sent 5 target markers, 5 rovers, an impacter, and collected multiple samples from the asteroid 162173 Ryugu (type C) to be returned to Earth. Hayabusa 2 is the second asteroid mission, a follow-on to the Hayabusa mission that explored the asteroid Itokawa. Hayabusa 2 is possibly the most complex asteroid mission ever launched as of 2020. JAXA continues to build on the successful missions they have sent to deep space.

Hayabusa 2 arrived at Ryugu on June 27, 2018. In September 2018, the spacecraft deployed the MIcro-Nano Experimental Robot Vehicle for Asteroid (MINERVA-II1) to the asteroid’s surface. MINERVA-II1 carried Rover1A, (HIBOU) and Rover1B (OWL) that hopped across the surface of the asteroid gathering information on temperature, acceleration, and taking images of the surface. The rovers were identical and both had 2 cameras. In October 2018, Mobile Asteroid Surface Scout (MASCOT) was deployed. MASCOT was a joint French-German lander that also hopped to move. It made three hops, operating ~17 hours on Ryugu's surface, an hour longer than expected. The data on the asteroid’s composition it collected was sent back to Earth via the Hayabusa 2 spacecraft.

The spacecraft contained a device called Small Carry-on Impactor (SCI) that launched a 30-cm copper sphere impacting the surface and creating a crater 10m in diameter. It was launched toward Ryugu on April 4, 2019 and hit the surface traveling ~4,500 mph. Some of the debris was later collected by the orbiting Hayabusa spacecraft on July 11, 2019. To observe the impact, Hayabusa 2 carried a Deployable Camera (DCAM3) that separated from the main spacecraft to take the images. During the impact the spacecraft stayed safely on the opposite side of the asteroid while the camera watched the impact. What Hayabusa2 taught us about asteroids is that they are easily smashed to small pieces, making it hard if not impossible to protect Earth by smashing up an oncoming asteroid, instead its orbit must be changed before it reaches the home planet.

The Sample-Return Capsule (SRC) is bringing samples back to Earth. The spacecraft is landed in the Woomera Prohibited Area in Australia northwest of Adelaide on December 6, 2020. The spacecraft is guided by optical navigation. Because it is anticipated that the spacecraft will have half of the fuel (xenon) for the ion engine left, it will be sent on a second mission. Check future missions below.

Learn more at JAXA about Hayabusa2

 

WISE

Now: NEOWISE reactivated by NASA to a new mission detecting Near Earth Asteroids!

WISE details on Astra's NEA Page

The Small Bodies Assessment Group - SBAG was established by NASA in March 2008 to establish scientific priorities and mission opportunities for exploration of near Earth asteroids and other small bodies. It provides input on the usability of asteroids and comets for human space exploration and other activities. SBAG reports its findings to NASA, but does not make recommendations.

Future Asteroid Missions

NASA Future Asteroid Missions

Lucy - 8 Trojan asteroids

Lucy is NASA's first space mission to study the Trojan asteroids that orbit around the Sun in Jupiter's orbit, leading or following the planet. The mission name comes from the fossilized human ancestor that was named "Lucy" by her discoverers. NASA hopes the Lucy mission will revolutionize our knowledge of the formation of the solar system.

Lucy will measure more than 46 feet (14 meters) including solar panels. It will have a 6.5-foot (2-meter) high gain antenna to communicate with Earth. Lucy is scheduled to launch in October 2021. It will utilize boosts from Earth's gravity to complete a 12-year journey to eight different asteroids.

The first instrument to be discussed is the Lucy Thermal Emission Spectrometer (L’TES) built by Arizona State University. It will measure the surface temperature of the Trojan asteroids. The Lucy LOng Range Reconnaissance Imager (L’LORRI) is a high resolution camera made by the Johns Hopkins University that will provide detailed images of the Trojan asteroids. L’Ralph is an instrument provided by NASA’s Goddard Space Flight Center it includes L’Ralph Linear Etalon Imaging Spectral Array (LEISA), an infrared imaging to help identify different silicates, ices and organics that may be on the surface of the Trojan asteroids, and L’Ralph Multi-spectral Visible Imaging Camera (MVIC), that will take color images of the Trojans asteroids.

DART - Double Asteroid Redirection Test Mission

DART is a planetary defense test of technologies for preventing an impact of Earth by a hazardous asteroid. It will test the possibility of redirecting an asteroid by forcing a collision with a spacecraft. DART will be the first demonstration of the impactor technique to change the orbit of an asteroid in space.

Because this is a defense mission details are covred on the NEA Detection and Planetary Defense DART section.

16 Psyche - Main asteroid belt

16 Psyche is a main belt asteroid orbiting between Mars and Jupiter. Psyche is large, about 226 km in diameter and is an M-type (metallic) asteroid. Because of its high iron and nickel content (it is similar to Earth’s core), it may be that Psyche is the exposed core of an ancient planet that lost its rocky outer layers due to violent collisions billions of years ago. Because of its high metal content, this asteroid could be a very valuable resource. Psyche orbits the sun every 1,830 days (5.01 years) and its distance from the Sun varies from 2.53 AU to 3.31 AU. Its orbit is between Mars and Jupiter and so never comes close to Earth and it is no threat to our planet.

The mission will be launched in August 2022. After launch, the spacecraft will travel using solar-electric propulsion. With the help of a gravity assist from Mars, the spacecraft should in arrive at Psyche in early January 2026. The Psyche mission will also test a new laser communication technology, called Deep Space Optical Communication, that encodes data in photons to communicate.

Japanese Aerospace Exploration Agency (JAXA)

Hayabusa 2

JAXA is now considering to send this successful spacecraft on a new mission after samples from the surface of an asteroid to the earth. Possible Targets: Asteroid 2001 AV43 or 1998 KY26 - Read the article at JAXA. The target 1998 KY26 has been chosen for the target, the above resource gives rationalization for the choice.

This mission is a follow on to the successful Hayabusa mission

B612 Foundation

Sentinel Mission - Sentinel is a mission the NEA population in the inner solar system is the first step to protecting the Earth from asteroid impacts and help to open this space next frontier. Sentinel will operate in the infrared in a mission expected to span 6.5 years, after 4 years to build and test. It will locate and follow the trajectories of asteroids larger than 140 meters.

The B612 Foundation's Sentinel Mission is a infrared (IR) survey mission. It is intended to discover 90 percent of NEAs larger than 140 meters. It is expected to discover many asteroids down to a diameter of 30 meters.

Future Asteroid Mission: Don Quijote

Don Quijote is an asteroid deflection precursor mission concept, being considered by ESA. The Don Quijote mission concept consists of two spacecraft that launch on separate trajectories. Sancho, the orbiter spacecraft, measures the target asteroid's position, shape, mass, and gravity field for several months before and after the impact. The impactor spacecraft, Hidalgo, will hit the target asteroid at a relative speed of about 10 km/s.

This mission is being considered under ESA's General Studies Program. Also see the Sancho Study.

Available Papers on Asteroid Missions

Click on the link to navigate to the on-line papers that discuss Asteroid Missions:

Mission opportunities with low delta V for NEA targets. This paper discusses 250 asteroids larger than 1 km considered easier to reach than the Moon's surface.

Written in 1978, Gene Shoemaker and Eleanor Helin discuss the possibility of crewed missions to an NEA.

Presented at the 29th International Electric Propulsion conference in 2005. It discusses a low cost launch of a deep space mission to a carefully selected asteroid.

Written in 2002 for Meteoritics and Planetary Science.The authors identify 234 NEOs with having a calculated DV requirement of less than 7 km/sec as candidates for physical characterization and mission targets.

Asteroid Retrieval Mission papers

Completed Asteroid Missions

Wide-field Infrared Survey Explorer

We thought it was all over!

NASA announced that it would Reactivate WISE for NEA searchers the week of 8/18/2013! The spacecraft was successfully revived in September 2013 after 31 months of hibernation. NASA's new mission home page can be found at WISE Mission Home.

Read about NEOWISE first discovery on December 29, 2013 - an NEA now designated 2013 YP139

WISE was a NASA-funded Explorer mission to study the solar system, the Milky Way, and the Universe in the infrared spectrum. WISE discovered over 153,000 asteroids. The WISE Mission launched on Dec. 14, 2009.

WISE found a new class of asteroid, the Earth Trojan.

WISE All-Sky Data Release provides access to WISE data. To look at data collected on asteroids, the WISE Moving Object Pipeline Subsystem (WMOPS) provides indepth information. Astronomers seeking data on individual asteroids, will want to check WISE Related Minor Planet Electronic Circulars (MPECs) for a list of the WISE discoveries.

The WISE mission website also offers educational videos at the NASA/JPL WISE Youtube channel!

Dawn Mission - Journey to the Beginning of the Solar System

Dawn revealed that Ceres is geologically active—or was very recently.

The Dawn mission was part of NASA's Discovery Program operating until November 2018. Dawn orbited the main asteroid belt, Vesta, and is now journeying to Ceres. These are the two largest known asteroids and it is believed the they survived the early epoch of bombardment so evident on the surface of Earth's moon. The investigation showed that Ceres was active more recently than it was previous believed. At Vesta , Dawn showed that it was a more complex than expected.

The Dawn Mission launched on September 27, 2007. Dawn arrived at Vesta in June 2011 and reached Ceres in 2015 becoming the first to visit a dwarf planet and orbit two asteroids.

Asteroid Mappers - Citizen scientists help to map the surface of Vesta. Investigate and analyze high-resolution Dawn images of Vesta, including craters and other features, from your own computer!

Deep Impact - Comet Impact Mission

Launched on January 12, 2005, Deep Impact was highly successful at Comet Borrelly. Comets are composed of ice, gas and dust, and are believed to have formed in the solar system's most distant and coldest regions. They are thought to be time capsules that hold clues about the formation and evolution of the solar system. Deep Impact is a NASA Discovery Mission and is the first space mission to probe beneath the surface of a comet. The impactor weighed 370 kg or 816 lbs. The impact created a cloud of a fine, powdery material, not the water, ice, and dirt that was expected.

Deep Space has been given new tasks under the mission name of EPOXI. First it is to fly past comet Hartley 2 in in 2010. While travelling to Hartley 2, the spacecraft observed planets around other stars. Here is a link to a paper encouraging the Deep Impact new task, 2020-Jan-4 flyby of Potentially Hazardous Asteroid 163249 (2002 GT).

Rosetta

ESA reactivated Rosetta on 10 year journey to its target, Comet 67P/Churyumov-Gerasimenko on January 20, 2014.
Sleeping Beauty awakes!

Rosetta was successfully launched on March 2,2004 from French Guiana. It made four gravity assists orbits, one by Mars and three by Earth, to reach it's target, Comet 67P/Churyumov-Gerasimenko. On its 10 year journey to the comet, the spacecraft flew by two asteroids: 2867 Steins on September 5, 2008) and 21 Lutetia on July 10, 2010).

Find out about Rosetta's NEA explorations during its journey to the comet by clicking on 2867 Steins and 21 Lutetia.

You can follow Rosetta on Facebook and Twitter. . .

Hayabusa

Launched on May 9, 2003, the Hayabusa spacecraft explored 25143 Itokawa (1998 SF36). This asteroid was named after the late Dr. Hideo Itokawa, considered the father of Japan's space development program. The HAYABUSA mission used an ion engine spacecraft to capture and return a sample from the asteroid. (1500 grains) It returned to Earth on June 13, 2010, dropping the sample in a capsule that landed in Australia

HAYABUSA, was the first Japanese mission to an asteroid. The Hayabusa 2 mission is a follow-on mission to asteroid 162173 Ryugu.

Near Earth Asteroid Rendezvous Mission

NEAR Spacecraft - The NEAR spacecraft visited the asteroids 253 Mathilde and 433 Eros (1898 DQ). The robotic space probe was designed by the Johns Hopkins University Applied Physics Laboratory for NASA. In June 1997, the NEAR Shoemaker spacecraft flew within 1200 km of Mathilde, a 61 km diameter asteroid. It first flew by the Aten asteroid, Eros, (diameter 34 km) in December of 1998 and entered orbit on February 2000, becoming the first spacecraft to orbit an asteroid. It was renamed "NEAR Shoemaker", in honor of planetary scientist Eugene Shoemaker who dream of taking a geological sample from the surface of Eros. The successful mission closed with a soft landing on the asteroid February 12, 2001.

Full details can be found in the paper Near Earth Asteroid Rendezvous: Mission Summary by Andrew F. Cheng the principal investigator. To investigate the orbit of Eros, go to the JPL's Small Body Database

Stardust - NASA Comet Sample Return Mission

Launched on February 7, 1989 with a primary mission objective to return a sample from the comet Wild 2, the Stardust visited the asteroid AnneFrank on November 2. 2002. The sample was returned to Earth in 2006.

Galileo - Jupiter Probe visits asteroids

Spacecraft Galileo at Jupiter visiting IO courtesy NASALaunched on October 18, 1989, the Galileo spacecraft's primary mission was to explore the planet Jupiter as an orbiter and an impactor. On August 28, 1993 the spacecraft visited the asteroid 243 Ida, discovering that Ida had a small companion named Dactyl. Ida is 58 km long and 23 km wide. The successful mission was concluded in 2003 when the spacecraft made a controlled impact on the atmosphere of Jupiter. Images and artwork are courtesy NASA.

Image of Ida and Dactyl from Galileo courtesy NASA

This image was used to help establish that 243 Ida had a moon.

Deep Space 1 - First Comet Flyby

Deep Space 1 launched on October 24, 1998. Its primary mission was to encounter Comet Borrelly and return science data and images from a comet. It performed a flyby of asteroid 9969 Braille (1992 KD) on July 28, 1999. The mission ended on December 18, 2001.