Mysteries of the TOI-406 System Revealed
Two intriguing planets await discovery beyond our Solar System.
G. Lacedelli, E. Pallè, R. Luque, C. Cadieux, J. M. Akana Murphy, F. Murgas, M. R. Zapatero Osorio, H. M. Tabernero, K. A. Collins, C. N. Watkins, A. L'Heureux, R. Doyon, D. Jankowski, G. Nowak, È. Artigau, N. M. Batalha, J. L. Bean, F. Bouchy, M. Brady, B. L. Canto Martins, I. Carleo, M. Cointepas, D. M. Conti, N. J. Cook, I. J. M. Crossfield, J. I. Gonzàlez Hernàndez, P. Lewin, N. Nari, L. D. Nielsen, J. Orell-Miquel, L. Parc, R. P. Schwarz, G. Srdoc, V. Van Eylen
― 5 min read
Table of Contents
- Meet TOI-406
- The Big Question: What's Inside?
- The Science Quest
- Getting to Know the Planets
- The Dynamic Duo
- The Measurements
- The Race Against Time
- Hot Topics: Atmospheres in the Limelight
- Planet Comparisons
- The Galactic Gossip: Composition
- Things That Go Bump in the Night
- The Stellar Spotlight
- The Science of Observation
- An Eye on the Future
- Conclusion: A Bright Future Ahead
- Original Source
- Reference Links
In the universe, among the stars, we stumble upon something exciting: the TOI-406 system. This particular system has caught the attention of researchers because it houses two Planets that offer a glimpse into the mysteries of formation and evolution of small planets beyond our own Solar System. Grab your telescope; we’re going to meet some intriguing neighbors!
Meet TOI-406
TOI-406 is not your average star. It’s an M-dwarf which means it’s cooler and smaller than our Sun. However, what makes it special is that it has two orbiting planets. These planets are part of a special class called Sub-Neptunes-a group that is a bit smaller than Neptune and larger than Earth. Think of them as the middle-aged siblings in the planetary family!
The Big Question: What's Inside?
Are these sub-Neptunes just rocky cores? Or do they have thick Atmospheres hugging their surfaces? This is the million-dollar question-a bit of an enigma causing astronomers to scratch their heads. To get some clarity, scientists need a whole lot of planets to study, complete with their mass and radius details, not unlike getting to know the neighbors before deciding if they’ll be good friends.
The Science Quest
The goal of digging into the TOI-406 system is simple: to figure out what makes these sub-Neptunes tick. By looking at how many sub-Neptunes there are and how their sizes and masses vary, researchers hope to understand how these planets formed and evolved. It’s like piecing together a cosmic jigsaw puzzle-but without the picture on the box!
Getting to Know the Planets
The Dynamic Duo
TOI-406 has two planets: let’s call them Planet B and Planet C. They are orbiting the star at different distances, and they both have their own unique characteristics:
- Planet B: This one is more Earth-like. It has a radius and mass suggesting it might be rocky, even possibly having a thin atmosphere.
- Planet C: This planet is another story. It could be a watery world or a gas-rich planet. The odds are truly in favor of it being a bit more mysterious.
Measurements
TheResearchers gathered data from a variety of sources, including fancy telescopes and satellites that could tell them more about the planets' orbits and sizes. They used photometry-fancy talk for measuring light-and radial velocity to build a more complete picture of these two planets.
The Race Against Time
The hunt for knowledge didn’t happen overnight. Scientists had to wait and watch for the right moments when the planets would pass in front of their host star, causing a tiny dip in brightness-like a cosmic game of hide-and-seek!
Hot Topics: Atmospheres in the Limelight
One of the more fascinating things about TOI-406 c is its potential for atmospheric studies. With the right equipment, researchers will be able to look for signs of water or other gases. Imagine having a front-row seat to some cosmic weather reports!
Planet Comparisons
In the cosmic neighborhood, TOI-406 c shares some similarities with other known planets. In fact, it’s on the rarer side of things-a sort of VIP in the world of small, cool planets. It’s like being invited to an exclusive planetary gala!
Composition
The Galactic Gossip:The idea that planets can be made of different materials is essential to understanding their formation. There are two main theories floating around:
- Some scientists think sub-Neptunes could be formed from icy materials far from a star, and later, as they got closer, they turned into watery worlds.
- Others believe they may have lost their original atmospheres, making them rocky instead.
Planet B seems to fit the first theory, while Planet C could be on the fence, sharing traits of both worlds. It’s like they are siblings with different tastes in music!
Things That Go Bump in the Night
As with any good cosmic tale, there’s always the chance of external forces influencing our planets. The researchers couldn't rule out the possibility of a third planet lurking nearby, silently observing the action. It's like the shy friend at a party that everyone knows about but no one really sees!
The Stellar Spotlight
Characterizing the TOI-406 system is an essential step on the way to answering some fundamental questions about how stars and their planets come to be. It’s a bit like being on a cosmic detective case where each new piece of data brings us closer to solving the mystery.
The Science of Observation
Scientists worked hard to gather all the necessary data. They used various telescopes around the world to compile information. For example, the ESPRESSO instrument provided high-precision spectroscopic data to help detect the subtle movements of the planets caused by their host star.
An Eye on the Future
What’s next for the TOI-406 system? With advancements in telescope technology, future observations will help researchers gain a deeper understanding of the atmospheres of these planets. The aim is to find out if there are any signs of life-tiny green aliens included!
Conclusion: A Bright Future Ahead
The exploration of the TOI-406 system is just the beginning. With its diverse planetary population, this star system offers a treasure trove of information that could reshape our understanding of planets beyond our own. The more we learn, the closer we get to answering questions about our place in the universe. So who knows? Maybe one day we’ll find someone waving back at us from a distant planet!
And there you have it, an overview of the cosmic wonders waiting on the horizon. With a bit of luck and lots of observation, the secrets of the universe will slowly unveil themselves just like the pages of a captivating novel.
Title: Characterisation of TOI-406 as showcase of the THIRSTEE program: A 2-planet system straddling the M-dwarf density gap
Abstract: The exoplanet sub-Neptune population currently poses a conundrum, as to whether small-size planets are volatile-rich cores without an atmosphere, or rocky cores surrounded by a H-He envelope. To test the different hypotheses from an observational point of view, a large sample of small-size planets with precise mass and radius measurements is the first step. On top of that, much more information will likely be needed, including atmospheric characterisation and a demographic perspective on their bulk properties. We present here the concept and strategy of the THIRSTEE project, which aims to shed light on the composition of the sub-Neptune population across stellar types by increasing their number and improving the accuracy of bulk density measurements, as well as investigating their atmospheres and performing statistical, demographic analysis. We report the first results of the program, characterising a new two-planet system around the M-dwarf TOI-406. We analyse TESS and ground-based photometry, together with ESPRESSO and NIRPS/HARPS RVs to derive the orbital parameters and investigate the internal composition of the 2 planets orbiting TOI-406, which have radii and masses of $R_c = 1.32 \pm 0.12 R_{\oplus}$, $M_c = 2.08_{-0.22}^{+0.23} M_{\oplus}$ and $R_b = 2.08_{-0.15}^{+0.16} R_{\oplus}$, $M_b = 6.57_{-0.90}^{+1.00} M_{\oplus}$, and periods of $3.3$ and $13.2$ days, respectively. Planet c is consistent with an Earth-like composition, while planet b is compatible with multiple internal composition models, including volatile-rich planets without H/He atmospheres. The 2 planets are located in 2 distinct regions in the mass-density diagram, supporting the existence of a density gap among small exoplanets around M dwarfs. With an T$_{\rm eq}$ of only 368 K, TOI-406 b stands up as a particularly interesting target for atmospheric characterisation with JWST in the low-temperature regime.
Authors: G. Lacedelli, E. Pallè, R. Luque, C. Cadieux, J. M. Akana Murphy, F. Murgas, M. R. Zapatero Osorio, H. M. Tabernero, K. A. Collins, C. N. Watkins, A. L'Heureux, R. Doyon, D. Jankowski, G. Nowak, È. Artigau, N. M. Batalha, J. L. Bean, F. Bouchy, M. Brady, B. L. Canto Martins, I. Carleo, M. Cointepas, D. M. Conti, N. J. Cook, I. J. M. Crossfield, J. I. Gonzàlez Hernàndez, P. Lewin, N. Nari, L. D. Nielsen, J. Orell-Miquel, L. Parc, R. P. Schwarz, G. Srdoc, V. Van Eylen
Last Update: 2024-12-13 00:00:00
Language: English
Source URL: https://arxiv.org/abs/2409.11083
Source PDF: https://arxiv.org/pdf/2409.11083
Licence: https://creativecommons.org/licenses/by/4.0/
Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.
Thank you to arxiv for use of its open access interoperability.
Reference Links
- https://orcid.org/0000-0002-4197-7374
- https://orcid.org/0000-0003-0987-1593
- https://orcid.org/0000-0002-4671-2957
- https://orcid.org/0000-0001-9291-5555
- https://orcid.org/0000-0001-8898-8284
- https://orcid.org/0000-0001-9087-1245
- https://orcid.org/0000-0001-5664-2852
- https://orcid.org/0000-0001-8621-6731
- https://orcid.org/0009-0005-6135-6769
- https://orcid.org/0000-0001-5485-4675
- https://orcid.org/0000-0002-7031-7754
- https://orcid.org/0000-0002-7030-9519
- https://orcid.org/0000-0003-4733-6532
- https://orcid.org/0000-0003-2404-2427
- https://orcid.org/0000-0002-0810-3747
- https://orcid.org/0000-0003-2239-0567
- https://orcid.org/0000-0002-1835-1891
- https://orcid.org/0000-0002-0264-7356
- https://orcid.org/0000-0003-0828-6368
- https://orcid.org/0009-0001-2825-6185
- https://orcid.org/0000-0003-2066-8959
- https://orcid.org/0000-0001-8227-1020
- https://orcid.org/0000-0001-5542-8870
- https://tess.mit.edu/followup
- https://mast.stsci.edu/portal/Mashup/Clients/Mast/Portal.html
- https://github.com/jlillo/tpfplotter
- https://archive.stsci.edu/missions/tess/doc/EXP-TESS-ARC-ICD-TM-0014.pdf
- https://exofop.ipac.caltech.edu/tess/target.php?id=153065527
- https://asas-sn.ifa.hawaii.edu/skypatrol/
- https://github.com/mzechmeister/serval
- https://dace.unige.ch/publications/
- https://github.com/njcuk9999/lbl
- https://github.com/hmtabernero/SteParSyn/
- https://github.com/gomesdasilva/ACTIN2
- https://github.com/nathanchara/l1periodogram
- https://github.com/hpparvi/PyTransit
- https://github.com/hpparvi/ldtk
- https://github.com/LucaMalavolta/PyORBIT
- https://github.com/hpparvi/PyDE
- https://github.com/hippke/tls
- https://zenodo.org/records/10719523
- https://github.com/philippbaumeister/ExoMDN
- https://www.cosmos.esa.int/gaia
- https://www.cosmos.esa.int/web/gaia/dpac/consortium