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Active asteroid

Adapted from Wikipedia · Discoverer experience

Astronomers captured the huge cloud of dust and debris that flew from an asteroid after a spacecraft hit it — like a giant cosmic explosion seen from a telescope in Chile!

Active asteroids are small objects in space that move like asteroids but sometimes look like comets. They have features such as a fuzzy area around them or a tail, which are signs that material is leaving the object. However, they travel in paths similar to asteroids, usually staying within the orbit of the planet Jupiter.

Asteroid 596 Scheila displaying a comet-like appearance on 12 December 2010

These objects were first called main-belt comets in 2006 by astronomers David C. Jewitt and Henry Hsieh. This name suggested they were made of ice, like comets, and only found in the main group of asteroids. But as more of these objects were found, it became clear that not all of them fit this description.

The first active asteroid discovered is called 7968 Elst–Pizarro. It was first seen in 1979 as an asteroid. Later, in 1996, astronomers Eric Elst and Guido Pizarro noticed it had a tail and gave it the comet name 133P/Elst–Pizarro.

Orbits

Active asteroids move around the Sun in paths that stay closer than the planet Jupiter. Unlike comets, which travel far from the Sun, active asteroids have orbits that look much like regular asteroids.

Scientists describe these orbits using special measurements. One important measurement is called the semi-major axis, which must be within Jupiter’s orbit. Another is the Tisserand parameter, which helps tell asteroids apart from comets. The first active asteroids found all move in the outer part of the asteroid belt.

Activity

Some active asteroids show a dusty tail only when they are close to the Sun. This suggests that materials on their surface are turning into gas, pushing dust away. The activity of one active asteroid, called 133P/Elst–Pizarro, happens every time it gets close to the Sun. This activity lasts for a month or more and is thought to be caused by ice exposed by small crashes in the past few hundred years.

In 2010, an object called P/2010 A2 (LINEAR) was thought to be showing comet-like behavior, but it is now believed to be the remains of a crash between asteroids. Another asteroid, 596 Scheila, was seen covered in dust after being hit by another asteroid.

P/2013 R3

Disintegration of asteroid P/2013 R3 observed by the Hubble Space Telescope (6 March 2014).

Main article: P/2013 R3 (Catalina–PanSTARRS)

P/2013 R3 was discovered by two observers and was found to be breaking apart. Follow-up observations showed that this asteroid had split into pieces, with one main piece and three smaller pieces moving away from each other.

Dimorphos

Main article: Dimorphos

When a spacecraft called the Double Asteroid Redirection Test hit the asteroid moon Dimorphos, it caused the asteroid to lose a lot of material and create a long dust tail. This was the first time scientists were able to watch an asteroid become active from a crash. The impact changed Dimorphos's shape and rotation, and it is expected to settle back into a steady spin over time.

Composition

Some active asteroids have icy parts like traditional comets, while others are rocky like typical asteroids. Scientists think that these icy active asteroids might have brought water to Earth a long time ago. This is because the water in Earth's oceans has a special mix that doesn’t match what we usually find in comets. Some European scientists have suggested a mission to collect samples from an active asteroid named Caroline to learn more about its icy parts and dust.

List

Identified members of this group (TJup>3.08) include:: 17 

NameSemi-major axis
(AU)
Perihelion
(AU)
EccentricityTJupOrbital
class
Diameter
(km)
Rotation
period
(hr)
CauseActivity
discovery
year
Recurrent?
1 Ceres2.7662.5500.0783.310main-belt (middle)939.49.07Water sublimation2014
493 Griseldis3.1162.5680.1763.140main-belt (outer)41.5651.94Impact2015
596 Scheila2.9292.450.1633.209main-belt (outer)159.7215.85Impact2011
2201 Oljato2.1740.6240.7133.299NEO (Apollo)1.8>26Sublimation1984
3200 Phaethon1.2710.1400.8904.510NEO (Apollo)6.263.60Thermal fracturing, dehydration cracking, and/or rotational disintegration2010
6478 Gault2.3051.8600.1933.461main-belt (inner)5.62.49Rotational disintegration2019
(62412) 2000 SY1783.1592.9090.0793.197main-belt (outer)10.383.33Rotational disintegration2014
65803 Didymos/Dimorphos1.6431.0130.3834.204NEO (Apollo)0.77 / 0.152.26Human-caused impact2022
101955 Bennu1.1260.8960.2045.525NEO (Apollo)0.484.29(unknown): 22 
Electrostatic lofting, impacts, thermal fracturing, or dehydration cracking
2019
(588045) 2007 FZ183.1762.7830.1243.188main-belt (outer)2023
2002 CW1162.6902.0680.2313.319main-belt (middle)0.52024
2008 BJ223.0712.9430.0423.199main-belt (outer)2022
2010 LH152.7441.7700.3553.230main-belt (middle)1.4832023
2015 BC5663.0622.9570.0343.201main-belt (outer)2023
2015 FW4122.7652.3190.1613.280main-belt (middle)2023
2015 VA1083.1282.4510.2173.160main-belt (outer)2023
P/2023 JN162.6962.3000.1473.351main-belt (middle)2023
107P/4015 Wilson–Harrington2.6250.9660.6323.082NEO (Apollo)6.927.15Sublimation1949
133P/7968 Elst–Pizarro3.1652.6680.1573.184main-belt (outer)3.83.47Sublimation/rotational disintegration1996
176P/118401 LINEAR3.1942.5780.1933.167main-belt (outer)4.022.23Sublimation2005
233P/La Sagra (P/2009 WJ50)3.0331.7860.4113.081main-belt (outer)3.02010
238P/Read (P/2005 U1)3.1622.3620.2533.153main-belt (outer)0.8Sublimation2005
259P/Garradd (P/2008 R1)2.7271.7940.3423.217main-belt (middle)0.60Sublimation2008
288P/(300163) 2006 VW1393.0512.4380.2013.203main-belt (outer)1.8 / 1.2Sublimation2011
311P/PanSTARRS (P/2013 P5)2.1891.9350.1163.660main-belt (inner)0.4>5.4Rotational disintegration2013
313P/Gibbs (P/2003 S10)3.1542.3910.2423.133main-belt (outer)2.0Sublimation2003
324P/La Sagra (P/2010 R2)3.0982.6210.1543.099main-belt (outer)1.1Sublimation2010
331P/Gibbs (P/2012 F5)3.0052.8790.0423.228main-belt (outer)3.543.24Rotational disintegration2012
354P/LINEAR (P/2010 A2)2.2902.0040.1253.583main-belt (inner)0.1211.36Impact2010
358P/PanSTARRS (P/2012 T1)3.1552.4100.2363.134main-belt (outer)0.64Sublimation2012
426P/PanSTARRS (P/2019 A7)3.1882.6750.1613.103main-belt (outer)2.42019
427P/ATLAS (P/2017 S5)3.1712.1780.3133.092main-belt (outer)0.901.4Sublimation/rotational disintegration2017
432P/PanSTARRS (P/2021 N4)3.0452.3020.2443.170main-belt (outer)2021
433P/(248370) 2005 QN1733.0672.3740.2263.192main-belt (outer)3.2Sublimation/rotational disintegration2021
435P/PanSTARRS (P/2021 T3)3.0182.0560.3193.090main-belt (outer)2021
455P/PanSTARRS (P/2021 S9)3.1562.1930.3053.087main-belt (outer)2017
456P/PanSTARRS (P/2021 L4)3.1652.7880.1193.125main-belt (outer)2021
457P/2020 O1 (Lemmon–PanSTARRS)2.6472.3290.1203.376main-belt (middle)0.841.67Sublimation/rotational disintegration2020
483P/PanSTARRS (P/2016 J1)3.1722.4490.2283.113main-belt (outer)Sublimation2016
P/2013 R3 (Catalina–PanSTARRS)3.0332.2050.2733.184main-belt (outer)~0.4Sublimation/rotational disintegration2013
P/2015 X6 (PanSTARRS)2.7552.2870.1703.318main-belt (middle)Sublimation2015
P/2016 G1 (PanSTARRS)2.5832.0410.2103.367main-belt (middle)Impact2016
P/2018 P3 (PanSTARRS)3.0071.7560.4163.096main-belt (outer)Sublimation2018
P/2019 A3 (PanSTARRS)3.1472.3130.2653.099main-belt (outer)2019
P/2019 A4 (PanSTARRS)2.6142.3790.0903.365main-belt (middle)0.342019
P/2021 A5 (PanSTARRS)3.0472.6200.1403.147main-belt (outer)0.30Sublimation2021
P/2021 R8 (Sheppard)3.0192.1310.2943.179main-belt (outer)2021
P/2022 R5 (PanSTARRS)3.0712.4700.1963.148main-belt (outer)2022
P/2023 S4 (Hogan)3.1342.5420.1893.185main-belt (outer)2023
P/2024 L4 (Rankin)2.2310.6720.6993.255NEO (apollo)Rotational disintegration?2024
P/2024 R2 (PANSTARRS)3.1382.3020.2663.104main-belt (outer)2024

Exploration

Asteroid 101955 Bennu seen ejecting particles on January 6, 2019, in images taken by the OSIRIS-REx spacecraft

JAXA’s DESTINY+ is a planned mission to visit 3200 Phaethon and collect dust. It is expected to launch in fiscal year 2028.

Castalia is an idea for a robot spacecraft to study 133P/Elst–Pizarro. This could help us learn about where Earth’s water came from. The idea was suggested in 2015 and 2016 to the European Space Agency, but it was not chosen at that time. The team is still working on the plan, and a possible launch date is October 2028.

In 2019, the OSIRIS-REx mission saw small pieces of rock and dust leaving 101955 Bennu when it flew close to this near-Earth asteroid. This was the first time scientists saw an asteroid acting like this up close. Since then, they have seen this happen at least 10 more times, though these events are smaller than ones seen from far away.

Images

The Crab Nebula is a beautiful cloud of glowing gas and dust left behind after a massive star exploded. This stunning image shows the colorful remnants spreading out in space.
A stunning photograph of Comet Hyakutake, showing its bright tail stretching across the night sky.
A stunning image of comet 67P taken by the Rosetta spacecraft from about 82 kilometers away. The comet appears as a rugged, irregularly shaped object floating in space.
A colorful illustration of the planets in our solar system, showing Mercury, Venus, Earth with the Moon, Mars, Jupiter, Saturn, Uranus, and Neptune.
A stunning view of our Earth from space, showing Africa, Antarctica, and the Arabian Peninsula as seen by astronauts aboard Apollo 17.
A stunning view of Earth rising over the lunar horizon, captured by astronauts during the Apollo 8 mission.
An artist's view of HE 1523-0901, one of the oldest stars in our galaxy, located about 7500 light years from Earth.

Related articles

This article is a child-friendly adaptation of the Wikipedia article on Active asteroid, available under CC BY-SA 4.0.

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