Planet Nine Candidate from IRAS and AKARI Data
Researchers for objects that moved slowly between IRAS and AKARI detections. IRAS and AKARI are far-infrared, all-sky surveys completed 23 years apart. They looked in the Kuiper belt.
They produced all possible candidate pairs including one IRAS source and one AKARI source whose angular separations were limited between 42β² and 69.6β², corresponding to the heliocentric distance range of 500 β 700 AU and the mass range of 7β 17Mβ. There were 13 candidate pairs obtained after the selection criteria. After image inspection, they **found one good candidate** , of which the IRAS source is absent from the same coordinate in the AKARI image after 23 years and vice versa. However, AKARI and IRAS detections are not enough to determine the full orbit of this candidate.
9 detections are required to evaluate a linked Keplerian orbit with improved processing speed and reduce the number of false positives.
They will need the new and better space telescopes to re-examine the candidate to see if they can confirm that is planet 9 or not.
The IRAS and AKARI detections alone are not enough to decide a precise orbit. The DECam, with a large field of view, is a prospective option for the follow-up observation. It enables the possibility of detecting faint moving objects even in optical wavelengths and determining the full orbit of
our candidate, since the exposure time to observe targets as faint as 26 AB mag at DECam is approximately one hour. The verification of Planet Nineβs existence via future observational studies will contribute to our understanding of the evolution and structural dynamics of the solar system.
Brian Wang
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Planet Nine Candidate from IRAS and AKARI Data Researchers for objects that moved slowly between ...
https://www.nextbigfuture.com/2025/05/planet-nine-candidate-from-iras-and-akari-data.html
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Result Details
03.05.2025 07:43 β π 1 π 1 π¬ 0 π 0
A far-infrared search for planet nine using AKARI all-sky survey | Publications of the Astronomical Society of Australia | Cambridge Core
A far-infrared search for planet nine using AKARI all-sky survey - Volume 42
Check out this popular article in #PASA Chen, Goto, Yamamura, Nakagawa, Wu, Phan, Hashimoto, Uno, Ho, Kim: "A Far-Infrared Search for Planet Nine Using AKARI All-Sky Survey"
Read for free thanks to #OpenAccess
cup.org/44rkqbk
30.06.2025 13:50 β π 1 π 1 π¬ 0 π 0
@astrominh.bsky.social I just wonder after submission, if the Editorial Board makes a decision that the paper is not eligible for publication in PASA Letter, do authors have to manually submit their paper again to the usual PASA?
27.06.2025 13:07 β π 0 π 0 π¬ 0 π 0
The PASA Editorial Board and I are proud to announce PASA is now accepting Letter submissions!
21.05.2025 09:25 β π 8 π 2 π¬ 1 π 0
@plutokiller.com I'm just wonder if it's possible that the orbital clustering of minor KBOs is driven by the gravity of two planets? Have you ever simulated this scenario?
03.05.2025 08:29 β π 0 π 0 π¬ 2 π 0
@plutokiller.com Although we haven't estimated it yet in this work, I would say that all IRAS and AKARI sources before pairing up were required to have high flux quality (fqual value) at 60, 65, 90, and 100 micron. By this way we can remove unreliable sources from the beginning.
03.05.2025 08:23 β π 0 π 0 π¬ 0 π 0
@mbmocam.bsky.social Using Machine Learning to speed up the data analysis is a good idea. We'll consider applying it to our next studies.
03.05.2025 08:13 β π 3 π 0 π¬ 0 π 0
@mbmocam.bsky.social JWST can be used for deeper researches on P9 unless we know where it is on its orbit. Due to the uncertainty of P9's heliocentric distance, I think it's currently better to search by using all-sky surveys with larger field of view.
03.05.2025 08:10 β π 1 π 0 π¬ 0 π 0
@astrafoxen.bsky.social
Anyway, thank you for raising an important point. It is worth checking and discussing in more detail in the follow-up studies.
01.05.2025 04:00 β π 6 π 0 π¬ 1 π 0
@astrafoxen.bsky.social
However, the angular resolution of IRAS is 1.2β at 60um. Within a radius of 1.2', there are even more sources that raise the difficulty in determining which source is the true counterpart of our IRAS source.
01.05.2025 04:00 β π 3 π 0 π¬ 0 π 0
@astrafoxen.bsky.social
To be specific, in Section 6 of that paper, they classified objects based on the AKARI-IRC or AKARI-FIS detections, which are absent in the output result. Additionally, the WISE image shows nearby sources around the IRAS position.
01.05.2025 03:59 β π 3 π 0 π¬ 0 π 0
@astrafoxen.bsky.social
The IRAS source in our candidate indeed matches with a WISE source when checking the IRAS-PSC/FSC Combined Catalogue (Abrahamyan et al. 2015). However, the classification method presented in that paper seems to be insufficient to conclude that our IRAS source is a galaxy.
01.05.2025 03:57 β π 3 π 0 π¬ 0 π 0
Having meticulously identified this candidate from two million IRAS+AKARI objects, I believe it still merits immediate and thorough follow-up observations to determine its planetary status and orbital characteristics.
01.05.2025 03:55 β π 3 π 0 π¬ 1 π 0
Thank you for a very important point. While our candidate is at a higher orbital inclination than predicted by your simulations, however, the detection of a giant planet would still be an interesting discovery regardless of its precise orbit.
01.05.2025 03:55 β π 1 π 0 π¬ 1 π 0
Dear Prof. Brown, Iβm Terry - the 1st author of the paper. Thank you for reading our paper! I started this research motivated by your paper and presentations. It is a great pleasure to have your comments on my paper.
01.05.2025 03:55 β π 10 π 0 π¬ 1 π 0
https://arxiv.org/abs/2504.17288
arXiv abstract link
A Search for Planet Nine with IRAS and AKARI Data
https://arxiv.org/pdf/2504.17288
Terry Long Phan, Tomotsugu Goto, Issei Yamamura, Takao Nakagawa, Amos Y.-A. Chen, Cossas K.-W. Wu, Tetsuya Hashimoto, Simon C.-C. Ho, Seong Jin Kim.
25.04.2025 07:29 β π 4 π 2 π¬ 2 π 0
A Search for Planet Nine with IRAS and AKARI Data
The outer solar system is theoretically predicted to harbour an undiscovered planet, often referred to as P9. Simulations suggest that its gravitational influence could explain the unusual clustering ...
I have a couple of thoughts about the new paper the finds a candidate Planet Nine in some old data. First, it is difficult to tell how seriously to take this because a false alarm probability is never discussed, and second, if it is real, it is not Planet Nine. Read on:
π§΅ππ§ͺ
arxiv.org/abs/2504.17288
26.04.2025 20:43 β π 145 π 30 π¬ 16 π 3
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