Many eyes were trained toward the night skies with the recent, rare, super blue blood Moon. While such spectacular events in the solar system provide joy for laypeople, astronomers seek to find similar features—beginning with finding a moon—outside the solar system in ongoing efforts to detect conditions for life elsewhere.

An exomoon is a moon orbiting a planet outside our solar system. So far, astronomers have discovered and measured the characteristics of 3,728 planets outside the solar system.1 They have yet to make an undisputed detection of an exomoon.

An exomoon detection is imminent, however. Furthermore, astronomers have made sufficiently extensive observations to place meaningful limits on exomoon formation models. Such limits already are shedding light on moon design features that are critical for making life possible on a moon’s host planet.

In April of 2014 a paper was published in the Astrophysical Journal announcing the detection of a sub-Earth-mass moon orbiting a free-floating (detached from its host star) gas giant planet 3–4 times the mass of Jupiter.2 However, as the authors pointed out in their paper,3 their detection also could be explained by a Neptune-mass planet orbiting a very low-mass red dwarf star. Thus, their exomoon identification was not definitive. They simply detected an exomoon candidate.

In the January 2018 issue of the Astronomical Journal, two Columbia University astronomers and a citizen amateur astronomer published a paper in which they announced the discovery of a much stronger exomoon candidate and placed a limit on the existence of analogs of Jupiter’s large moons (known as Galilean moons) orbiting exoplanets.4 This paper was the sixth in a series of papers published by the “Hunt for Exomoons with Kepler” (HEK) project. Kepler is the spacecraft dedicated to finding exoplanets by the transit method.

Exomoon Candidate
The exomoon candidate that the three astronomers found apparently is orbiting the gas giant planet Kepler-1625b. Kepler-1625b is between 5.9 and 11.7 times the mass of Jupiter and orbits its host star with a period of 287 days. The moon, if it proves to be real, is about the size of Neptune (17 Earth masses) and would be orbiting its host planet at a distance of about ten times the diameter of the host planet (about one million miles).

It is possible, however, that Kepler-1625b is more massive than 11.7 times Jupiter’s mass. In that case it might be a brown dwarf star instead of a gas giant planet. Then, the three astronomers would have discovered a planet orbiting a brown dwarf star rather than a moon orbiting a planet. The three astronomers have scheduled time on the Hubble Space Telescope to determine which of the two scenarios is correct.

Galilean Moons
The team selected 284 exoplanets for which astronomers had the highest quality measurements of their physical and orbital properties. They then stacked the data from a total of 6,096 transit events that astronomers had observed for these 284 planets. Next, they performed a rigorous statistical analysis to characterize the exomoon population for the sample of the 284 planets.

The statistical analysis yielded a strong upper limit on the exomoon population for planets orbiting their host stars as close or closer than Earth orbits the Sun. Moons, at least moons as large as the Galilean moons, orbiting such planets must be rare, if they exist at all. The team’s finding is consistent with theoretical work showing that when planets migrate inward toward their host stars any closer than Earth is to the Sun, they lose any moons that they might have possessed.5 Thus, the trio concluded that their finding indicates that a large majority of the 284 planets in their sample experienced substantial inward migration.

The paper published by the three astronomers gives the first significant findings from exomoon astronomy. Therefore, it is fair to say that the discipline of exomoon astronomy has been launched. It is also fair to say that these initial exomoon astronomy findings provide yet more evidence for the rare solar system doctrine. The findings make a yet stronger case that the solar system is rare, and likely unique, in its property that its planets experienced exactly the right amounts of inward and outward migration to make advanced life possible within the planetary system.6

Featured image credit: Frizaven

Endnotes
  1. Exoplanet TEAM, The Extrasolar Planets Encyclopaedia, The Catalog (January 31, 2018), http://exoplanet.eu/catalog/.
  2. D. P. Bennett et al., “MOA-2011-BLG-262Lb: A Sub-Earth-Mass Moon Orbiting a Gas Giant Primary or a High Velocity Planetary System in the Galactic Bulge,” Astrophysical Journal 785 (April 7, 2014): id. 155, doi:10.1088/0004-637X/785/2/155.
  3. Bennett et al., “MOA-2011-BLG-262Lb,” 12.
  4. A. Teachey., D. M. Kipping, and A. R. Schmitt, “HEK. VI. On the Dearth of Galilean Analogs in Kepler, and the Exomoon Candidate Kepler-1625b I,” Astronomical Journal 155 (December 22, 2017): id. 36, doi:10.3847/1538-3881/aa93f2.
  5. Fathi Namouni, “The Fate of Moons of Close-In Giant Exoplanets,” Astrophysical Journal Letters 719 (July 28, 2010): L145–L147, doi:10.1088/2041-8205/719/2/L145; Christopher Spalding, Konstantin Batygin, and Fred C. Adams, “Resonant Removal of Exomoons during Planetary Migration,” Astrophysical Journal 817 (January 19, 2016): id. 18, doi:10.3847/0004-637X/817/1/18.
  6. Hugh Ross, Improbable Planet: How Earth Became Humanity’s Home (Grand Rapids: Baker, 2016), 43–77.

 

Check out more from Dr. Hugh Ross @Reasons.org

 

About The Author

Dr. Hugh Ross

Reasons to Believe emerged from my passion to research, develop, and proclaim the most powerful new reasons to believe in Christ as Creator, Lord, and Savior and to use those new reasons to reach people for Christ. I also am eager to equip Christians to engage, rather than withdraw from or attack, educated non-Christians. One of the approaches I’ve developed, with the help of my RTB colleagues, is a biblical creation model that is testable, falsifiable, and predictive. I enjoy constructively integrating all 66 books of the Bible with all the science disciplines as a way to discover and apply deeper truths. 1 Peter 3:15–16 sets my ministry goal, "Always be prepared to give an answer to everyone who asks you to give the reason for the hope that you have. But do this with gentleness and respect, keeping a clear conscience." Hugh Ross launched his career at age seven when he went to the library to find out why stars are hot. Physics and astronomy captured his curiosity and never let go. At age seventeen he became the youngest person ever to serve as director of observations for Vancouver's Royal Astronomical Society. With the help of a provincial scholarship and a National Research Council (NRC) of Canada fellowship, he completed his undergraduate degree in physics (University of British Columbia) and graduate degrees in astronomy (University of Toronto). The NRC also sent him to the United States for postdoctoral studies. At Caltech he researched quasi-stellar objects, or "quasars," some of the most distant and ancient objects in the universe. Not all of Hugh's discoveries involved astrophysics. Prompted by curiosity, he studied the world’s religions and "holy books" and found only one book that proved scientifically and historically accurate: the Bible. Hugh started at religious "ground zero" and through scientific and historical reality-testing became convinced that the Bible is truly the Word of God! When he went on to describe for others his journey to faith in Jesus Christ, he was surprised to discover how many people believed or disbelieved without checking the evidence. Hugh's unshakable confidence that God's revelations in Scripture and nature do not, will not, and cannot contradict became his unique message. Wholeheartedly encouraged by family and friends, communicating that message as broadly and clearly as possible became his mission. Thus, in 1986, he founded science-faith think tank Reasons to Believe (RTB). He and his colleagues at RTB keep tabs on the frontiers of research to share with scientists and nonscientists alike the thrilling news of what's being discovered and how it connects with biblical theology. In this realm, he has written many books, including: The Fingerprint of God, The Creator and the Cosmos, Beyond the Cosmos, A Matter of Days, Creation as Science, Why the Universe Is the Way It Is, and More Than a Theory. Between writing books and articles, recording podcasts, and taking interviews, Hugh travels the world challenging students and faculty, churches and professional groups, to consider what they believe and why. He presents a persuasive case for Christianity without applying pressure. Because he treats people's questions and comments with respect, he is in great demand as a speaker and as a talk-radio and television guest. Having grown up amid the splendor of Canada's mountains, wildlife, and waterways, Hugh loves the outdoors. Hiking, trail running, and photography are among his favorite recreational pursuits - in addition to stargazing. Hugh lives in Southern California with his wife, Kathy, and two sons.



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