Asteroid

Phaethon

The rocky asteroid behind the Geminid meteor shower, which passes closer to the Sun than Mercury and brightens as it does.

Radar image of Phaethon from the Arecibo Observatory, 17 December 2017
Image: Arecibo Observatory/NASA/NSF

At a glance

Size
~5–6 km — one of the largest known PHAs
Impact risk
Not on NASA's impact-risk list
Close approaches and the impact-risk list

Missions to Phaethon

Dates marked expected are agency estimates.

From discovery to the flyby

  1. Between April 2028 and March 2029 expected
    Launch (H3, shared with Ramses)
    DESTINY+
  2. In 2029 expected
    Flyby of Apophis, a rehearsal for Phaethon
    DESTINY+
  3. Between April 2030 and March 2031 expected
    Flyby of Phaethon, parent of the Geminids
    DESTINY+

Dates marked expected are agency estimates.

Most meteor showers come from comets. The Geminids, which peak in mid-December and are among the best and most reliable showers of the year, come instead from an asteroid: 3200 Phaethon.[1] Under perfect conditions, about 120 Geminid meteors an hour can be seen at the peak, each one a fragment of debris from Phaethon's orbit burning up in Earth's atmosphere.[1]

Discovery and size

Phaethon was discovered on 11 October 1983 by NASA's Infrared Astronomical Satellite, IRAS.[2] The astronomer Fred Whipple recognized it as the source of the Geminids.[1] Size estimates range from about 5 km to 6 km, so it is one of the larger potentially hazardous asteroids known.[1][2] Radar images from the Arecibo Observatory in December 2017 showed a roughly ball-shaped body with a large depression near its equator.[2] At that pass, on 16 December 2017, Phaethon came within about 10.3 million km, some 27 times the distance to the Moon; it will not come closer until 2093.[2]

An asteroid that behaves like a comet

Phaethon's elongated orbit, which takes 524 days, carries it well inside the orbit of Mercury, where the Sun heats its surface to about 750 °C.[3] Near the Sun it brightens, as comets do, although any ice near its surface would have been baked away long ago.[3] A 2021 study proposed that sodium in its rock vaporizes and vents through cracks, enough to brighten it and to eject small pieces of rock; this would also explain why Geminid meteors contain little sodium.[3] Scientists still debate whether Phaethon is best described as an asteroid or as a dead or rocky comet.[1]

A mission to fly past it

Japan's DESTINY+ mission will make a high-speed flyby of Phaethon and study interplanetary dust, which brings carbon and organic matter to Earth and of which Phaethon is one source.[4] It is aiming for launch in Japan's fiscal year 2028, sharing an H3 rocket with ESA's Ramses spacecraft, and it will first fly past Apophis as a rehearsal.[4][5]

Sources

  1. [1]NASA, Geminids — science.nasa.gov, retrieved October 26, 2026
  2. [2]NASA Jet Propulsion Laboratory, Arecibo Radar Returns with Asteroid Phaethon Images — jpl.nasa.gov, retrieved October 26, 2026
  3. [3]NASA Jet Propulsion Laboratory, Fizzing Sodium Could Explain Asteroid Phaethon's Cometlike Activity — jpl.nasa.gov, retrieved October 26, 2026
  4. [4]JAXA Institute of Space and Astronautical Science, DESTINY+ — destiny.isas.jaxa.jp, retrieved October 26, 2026
  5. [5]JAXA Institute of Space and Astronautical Science, Deep Space Exploration Technology Demonstrator DESTINY+ — isas.jaxa.jp, retrieved October 26, 2026

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