Эрдэмтэд манай нарны аймгийн хоёр өөр биетээс урьд өмнө бүртгэгдээгүй, химийн найрлага нь тодорхойгүй молекулын ул мөрийг олж илрүүлжээ.
Жэймс Вэбб сансрын дуран авайг ашиглан Плутон болон Санчир гарагийн дагуул Титаныг ажиглах явцад хэт ягаан туяаны мужид 5.11 микрометрийн орчимд үл мэдэгдэх шингээлтийн дохио илэрсэн байна. Зургаадугаар сарын 11-нд arXiv цахим хуудсанд нийтлэгдсэн уг судалгаагаар, энэхүү спектрийн онцлог нь нарны аймаг болон экзопланетуудад өмнө нь бүртгэгдсэн ямар ч химийн нэгдлийн шинж тэмдэгтэй таарахгүй байгааг тэмдэглэжээ.
Судлаачдын үзэж буйгаар уг дохио нь агаар мандалд бус, харин хоёр биетийн гадаргуу дээрх бодисоос үүдэлтэй байх магадлалтай юм. Плутон болон Титан нь метан, азотоор баялаг агаар мандалтай ч физик шинж чанараараа эрс ялгаатай ертөнцүүд юм. Тухайлбал, Плутон дээрх энэхүү шингээлтийн дохио нь Титаныг бодвол гурав дахин хүчтэй байгаа бол Титан дээр уг бодис нь гадаргуугийн дагуу жигд бус тархалттай байна.
Эрдэмтэд энэхүү нууцлаг молекулыг бензол, ацетилен эсвэл кетен зэрэг бодисын нэгдэл байж болзошгүй хэмээн таамаглаж байгаа ч одоогоор баттай нотолгоо алга байна. Энэхүү оньсого мэт үзэгдлийг тайлахын тулд NASA-гийн 2028 оноос эртгүй хөөргөхөөр төлөвлөж буй Dragonfly номлол чухал үүрэг гүйцэтгэнэ. 2034 онд Титаны агаар мандалд нэвтрэх уг төхөөрөмж нь гадаргуугийн бодисыг нарийвчлан шинжлэх спектрографтай тул уг молекулын учрыг олох боломжтой юм.
Дэлгэрэнгүйг эх сурвалжаас харах
↓Эх сурвалжийг нээх ↓
The James Webb Space Telescope has detected an unexplained infrared absorption signal, appearing as a distinct spectral feature, on both Pluto and Saturn’s largest moon, Titan.The finding points to the possible presence of an unknown molecule that has not been identified anywhere else in the solar system or on exoplanets, according to a new study posted on arXiv.
The discovery emerged after researchers examined infrared wavelengths that had received relatively little attention in previous observations. While comparing the spectra of Pluto and Titan, they identified a missing wavelength at approximately 5.11 micrometers, a signal that does not correspond to any known molecular signature documented in published planetary spectra.
The result is attracting attention because Pluto and Titan are very different worlds despite sharing atmospheres rich in methane and nitrogen. According to the researchers, the unexplained infrared absorption signal most likely originates from the surfaces of both bodies rather than from their atmospheres, making the finding even more difficult to explain.
A Spectral Signature Unlike Any Previously Recorded
Astronomers routinely identify the composition of distant objects by studying how matter absorbs electromagnetic radiation. Every element and molecule absorbs light at specific wavelengths, producing characteristic absorption lines that serve as chemical fingerprints.
The study uploaded to the preprint server arXiv on June 11 said that the scientists analyzed James Webb Space Telescope observations of Pluto and Titan while focusing on infrared wavelengths that had remained relatively unexplored. During that analysis, they detected a distinct absorption line centered around 5.11 micrometers in the spectra of both worlds.
The research team then compared the signal with existing studies of planetary spectra. As explained in the paper:
they “did not find any band referenced in these publications that corresponds to the location of the observed absorption in Titan and Pluto.”
As a result, the detected signal does not currently match any known chemical compound identified elsewhere in the solar system or on observed exoplanets. The telescope has already demonstrated its ability to identify chemical compounds in exoplanet atmospheres, around distant stars, and within primitive galaxies by analyzing electromagnetic spectra. This latest observation extends that capability to an unexpected molecular mystery much closer to home.
Pluto And Titan Share An Unexpected Common Feature
The detection is particularly surprising because Pluto and Titan differ significantly in their physical characteristics. Titan, Saturn’s largest moon, is larger than Mercury and is the only world besides Earth known to possess liquid rivers and oceans on its surface. Pluto, by contrast, is a frozen dwarf planet approximately half Titan’s size and located about four times farther from the Sun than Saturn’s moon.
Even with these differences, both bodies possess atmospheres dominated by methane and nitrogen. As explained by the researchers, the newly detected absorption feature appears to be associated with material on their surfaces rather than with atmospheric gases.
The observations also revealed differences between the two objects. Pluto’s absorption feature is roughly three times stronger than Titan’s, indicating that the unidentified material is likely much more abundant on Pluto. On Titan, the signal is not evenly distributed across the surface. Instead, the absorption is stronger on the moon’s trailing hemisphere than on its leading hemisphere as it orbits Saturn.
Scientists Are Testing Several Possible Explanations
The identity of the molecule responsible for the absorption feature remains unknown. The researchers proposed several possible candidates but emphasized that none has been confirmed. Based on the study, one possibility is benzene combined with another unidentified molecule. Other potential explanations include forms of acetylene ice or ketene ice. The authors noted that considerably more work will be required before any of these hypotheses can be validated.
The paper also points to a future opportunity to investigate the mystery more directly. NASA’s Dragonfly mission, scheduled to launch no earlier than 2028 and expected to fly through Titan’s atmosphere in 2034, will carry a spectrograph capable of identifying surface materials.
The observations from Dragonfly could help determine the identity of the unknown molecule on Titan and clarify whether the same material is also present on Pluto. However, the 5.11-micrometer absorption signal remains a mystery, as researchers have yet to identify any known substance capable of producing it.
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