November 22, 2024

SOHO Chases Asteroid’s Tail – Unmasks “Rock Comet” Phaethon’s Sodium Glow

This illustration illustrates asteroid Phaethon being heated up by the Sun. The asteroids surface area gets so hot that sodium inside Phaethons rock might vaporize and vent into space, triggering it to brighten like a comet and remove small pieces of rocky particles. Credit: NASA/JPL-Caltech/IPAC
The SOHO observatory has actually challenged previous theories about Phaethon, a rock comet connected to the Geminid meteor shower, by suggesting that its brightness and tail are triggered by salt emission, not dust release. This discovery also suggests that some comets may be more similar to rocky asteroids. Future missions and resident science efforts aim to additional research study this interesting object.
The ESA/NASA SOHO observatory has overturned 14 years of thinking of the unusual Sun-skirting rock comet referred to as Phaethon that could resume the secret of how the Geminid meteor shower was born.
Every December, the Geminid meteor shower lights up Earths skies as our world plunges through a vast cloud of dust in space. Many of the yearly meteor showers are associated with comets, which leave clouds of dust trailing behind them in the type of their tails.

When Phaethon was discovered in 1983 by the joint US/UK/Netherlands IRAS satellite, astronomers thought the secret was fixed. This little 5.8 km-wide things circled around the Sun in an orbit really comparable to that of the Geminid dust cloud, offering near-certain proof that Phaethon was the meteor showers moms and dad body despite the fact that Phaethon was an asteroid, not a comet.
Comparing pictures of the asteroid Phaethon taken with various filters on SOHOs LASCO coronograph. On the left, the orange filter exposes the shining asteroid Phaethon with a surrounding cloud and little tail. The brightness of this emission in the orange filter suggests that sodium atoms from the surface area of the asteroid fluoresce with an orange glow in action to sunshine, as the asteroid passes near to the Sun at perihelion. On the right, the blue filter shows no indication of Phaethon, showing that the light emitted is undetected in this filter. These images were recorded in May 2022. Phaethon is believed to be the parent asteroid of the Geminids meteor shower, which lights up the night sky every December. Credit: ESA/NASA/Qicheng Zhang
Each orbit of Phaethon, lasting 524 days, consists of an uncommonly close technique to the Sun. At a closest approach (perihelion) distance of 21 million km, Phaethon is hidden from observatories in the world by the blinding glare of the Sun. Therefore, solar observatories provide the only method to capture vital images to study the severe activity of the asteroid at perihelion.
Considering that 2009, the NASA Solar Terrestrial Relations Observatory (STEREO) has observed an unexpected brightening of the asteroid a few hours after perihelion. At this close method, Phaethon also sports a tail, hundreds of kilometers in length, dealing with far from the Sun. This activity was originally believed to be triggered by the release of little dust grains from the cracking of the asteroids surface as it passes the Sun. This caused Phaethon being dubbed a rock comet.
Now, brand-new observations from SOHO recorded in May 2022 have shown for the very first time that, contrary to 14 years of previous thought, the emission of salt atoms is most likely responsible for this activity.
A two-hour sequence of the asteroid Phaethon from the viewpoint of ESAs SOHO observatory. The images were taken on May 15, 2022, when the asteroids orbit ventured close to the Sun, at a range of 21 million km.
As part of an unique observing plan developed by Qicheng Zhang and Karl Battams, long-exposure, filtered images were taken by SOHOs Large Angle and Spectrometric Coronagraph (LASCO) telescope. Phaethon and its tail are missing from images taken with LASCOs blue filter, which can identify dust. It is intense in the sodium-sensitive orange filter, using compelling proof that salt emission is taking place. The emission is brought on by fluorescence, when sodium atoms get thrilled by the Sun and radiance orange, comparable to a street lamp.
” Our distinct observing plan discovered the mysterious asteroid Phaethon for the first time in SOHO information,” states PhD trainee Qicheng Zhang, who led the study. “The unique filters of the 27-year-old LASCO electronic camera were utilized in an unique disruption to the routine observing schedule to reveal these hidden tricks. By digging in the treasure chest of SOHO, we showed that Phaethon shows up in LASCO images from 18 various orbits back to 1997.”
This sequence of images, taken by SOHOs LASCO coronagraph, depicts the asteroid Phaethon at perihelion throughout different orbits around the Sun. The radiant asteroid is covered by a cloud and followed by a little tail that shines vibrantly in the orange filter of LASCO. The fluorescence of sodium in reaction to the Sun causes this brightening.These images were reconsidered after LASCO effectively identified Phaethon in images taken in May 2022. The exceptional outcomes reveal that Phaethon has been observed at perihelion by LASCO for more than 20 years. Credit: ESA
Phaethon is not the only object near the Sun to be launching sodium. The world Mercury likewise shows a brilliant sodium tail that peaks around 2 weeks after perihelion– something that the joint ESA/JAXA BepiColombo mission will examine when in orbit around Mercury. Observations of Mercurys sodium tail from the STEREO H1-1 heliospheric imager were utilized as a calibration requirement, like a standard lamp, to study this emission from Phaethon to support Zhangs theory.
SOHO has observed numerous small Sun-skirting objects that are categorized as comets– icy bodies which appear to lighten up when really close to the Sun. These can be difficult to distinguish from asteroids like Phaethon which shine briefly. The salt identified in this study has actually opened the possibility that possibly the so-called comets found by SOHO are more like rocky asteroids similar to Phaethon.
This composite image illustrates a collection of a few of the brightest comets observed by the LASCO coronagraph on the ESA/NASA SOHO observatory. Practically all of these comets were discovered by citizen scientists, who take part in the Sungrazer task. By studying LASCO images, anybody can report brand-new comets and make brand-new discoveries.Although LASCO research studies the external atmosphere of the Sun, called the corona, it is likewise an effective comet hunter. In its 26 years of operation, SOHO has actually observed over 4500 comets, making it the most successful comet hunter in history. Credit: ESA/NASA/R. Pickard
This research study shines more light on the occasions which could have formed the Geminid meteoroids, which vary in size from sand grains to pea-sized. Salt activity on the surface area is not enough to lift these particles and add to the stream. Rather, a unidentified and unseen interruption of Phaethon, possibly over two thousand years ago, is assumed to have produced the shower.
The fresh layers of unpredictable sodium which contribute to the brightening observed today suggest that another mass-loss event might have resurfaced Phaethon more recently, maybe less than 1000 years back. Therefore, the precise origin of the Geminids meteoroids may be much better understood by studying Phaethon.
There is fantastic interest in Phaethon due to its unique activity and mystical history, which make it a necessary and intriguing source of up-close future study. Thus, JAXA is preparing to send a flyby objective called DESTINY+ to image the surface of Phaethon in 2028 and discover more about its history.
In addition to future missions, citizen researchers can play their part in exposing new discoveries using SOHO. Over 4500 Sun-skirting things have been recognized in SOHO images, the majority with the aid of the Sungrazer Project. Citizen scientist comet hunters can sift through SOHO and STEREO information to recognize new objects.
Karl Battams, primary investigator of both LASCO and the Sungrazer project, describes, “SOHO is the most prominent comet hunter in history, with a substantial brochure of discoveries still awaiting in-depth analysis. Both SOHO and STEREO are distinctively put to be able to consistently observe objects incredibly close to the Sun. The future of asteroid and comet research studies is bright thanks to these and future encounter objectives that will help us reveal more about these vibrant things.”
” Since its launch in 1995, SOHO and its instruments continue to provide exciting science, using the objective in various methods to study asteroids and comets in addition to its main target, the Sun,” adds Bernhard Fleck, ESAs SOHO project scientist.
For more on this discovery, see Asteroids Comet-Like Tail Is Not Made of Dust.
Recommendation: “Sodium Brightening of (3200) Phaethon near Perihelion” by Qicheng Zhang, Karl Battams, Quanzhi Ye, Matthew M. Knight and Carl A. Schmidt, 25 April 2023, The Planetary Science Journal.DOI: 10.3847/ PSJ/acc866.

The asteroids surface gets so hot that salt inside Phaethons rock might vent and vaporize into space, causing it to lighten up like a comet and dislodge little pieces of rocky debris. Comparing images of the asteroid Phaethon taken with different filters on SOHOs LASCO coronograph. A two-hour sequence of the asteroid Phaethon from the perspective of ESAs SOHO observatory.” Our unique observing strategy discovered the strange asteroid Phaethon for the first time in SOHO data,” states PhD student Qicheng Zhang, who led the research study. The salt determined in this study has opened the possibility that perhaps the so-called comets found by SOHO are more like rocky asteroids similar to Phaethon.