Scientists are using stellar 'quakes' to peer inside stars
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The Mars Curiosity rover has found the largest organic molecules yet on the Red Planet. Organic molecules are the building blocks of life, although they can also be produced by geological processes. While there’s currently no way to prove whether these particular molecules were formed from processes associated with life, their very discovery shows thatContinue reading "Curiosity discovers largest organic molecules yet on Mars"
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Sky This Week is brought to you in part by Celestron. Friday, April 4This evening, the roughly half-illuminated face of the Moon hangs in Gemini, high in the south an hour after sunset. First Quarter Moon occurs at 10:15 P.M. EDT. The two brightest stars in Gemini are Castor (magnitude 1.6) and Pollux (magnitude 1.2).Continue reading "The Sky This Week from April 4 to 11: Catch your last views of Uranus"
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Author(s): Katherine Wright
Researchers have demonstrated a method for suppressing unwanted electrons in bright electron beam sources.
[Physics 18, s40] Published Thu Apr 03, 2025
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As World War II drew to a close, the Allies were eager to get their hands on one of the most technologically amazing yet terrifying weapons in Nazi Germany’s armamentarium: the V-2 rocket. A long-range, liquid-fueled supersonic guided missile, the V-2 could carry a 2,000-pound (910 kilograms) warhead a staggering 200 miles (320 kilometers) fromContinue reading "Megaroc: The British manned space program that almost was"
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Andrei Pleskatsevich, taken from Minsk, Belarus The Seagull Nebula is a region of nebulosity lying on the border between constellations Monoceros and Canis Major; the emission nebula forming the bird’s “head” carries the catalog designation IC 2177. The imager used a 3-inch f/4.5 scope and one-shot color camera to take 10 hours of exposure.
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Gitanjali Rao was honored as the inaugural recipient of the Stephen Hawking Medal Junior, an award created to inspire young innovators.
The post STARMUS Launches the Stephen Hawking Medal Junior at The Kennedy Center appeared first on Astronomy Magazine.
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Sky watchers The University of Arizona PressTucson, AZ Star Gazers: Finding Joy in the Night Sky, by prolific astronomy writer David H. Levy, is a collection of personal essays celebrating amateur and professional astronomy. Bringing together his decades of sky-watching experience, this 172-page book gives readers insight into Levy’s thoughts on James Webb Space Telescope,Continue reading "Spring for new astronomy products this month"
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Author(s): Katherine Wright
Transforming an MRI brain scan into a hyperbolic network of nodes allows researchers to detect brain connectivity disruption caused by Alzheimer’s disease.
[Physics 18, 70] Published Wed Apr 02, 2025
Author(s): Ryan Wilkinson
A new theory unveils the exotic low-energy excitations of quasicrystals formed of quantum particles.
[Physics 18, s39] Published Wed Apr 02, 2025
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The Federal Aviation Administration has completed its investigations looking into “mishaps” that occurred during Blue Origin’s New Glenn rocket launch and SpaceX’s Starship Flight 7 in January. On Jan. 16, Blue Origin’s New Glenn-1 reached orbit on its debut flight. While the launch was successful, the rocket lost its lower stage during its descent. Later thatContinue reading "FAA concludes Blue Origin, SpaceX January ‘mishap’ investigations"
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he first commercially built rocket to lift off from continental Europe came tumbling back to Earth within seconds. But its manufacturer considers the mission a success. The test flight, “Going Full Spectrum,” was the debut launch of Norwegian company Isar Aerospace’s Spectrum, a two-stage orbital launch vehicle designed to compete with SpaceX’s workhorse Falcon 9Continue reading "Debut flight of Isar Aerospace Spectrum rocket ends in explosion"
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From the editor: As the extraordinary pace of astronomical discovery carries on, we increasingly see that the stuff of life is spread throughout the cosmos. Life, even complex life, must be common out there. We know of several hundred billion stars in our galaxy, at least 100 billion galaxies, and planets around most of theContinue reading "Earth as a planet"
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My childhood fascination with the night sky led me to study astronomy and physics at university. By my second year, I was operating the telescope atop the physics building, tracking celestial objects — just like astronomy student Kate Dibiasky in the disaster movie Don’t Look Up.I never imagined I’d also soon find myself alerting othersContinue reading "Solving the climate equation"
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In many ways, Tony Fadell built the digital world we live in. At the turn of the millennium, his efforts to build a pocket-sized, hard-disk-based device that could hold 1,000 songs in MP3 format caught the attention of Apple. Within months, he had been hired by the firm, and less than a year after hisContinue reading "How to build climate solutions: An interview with Tony Fadell"
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Author(s): Charles Day
Observations by the JWST observatory of a star-free super-Jupiter reveal large-scale inhomogeneities in its atmosphere.
[Physics 18, 69] Published Tue Apr 01, 2025
Author(s): Philip Ball
The messy breakup of a liquid droplet that occurs when it hits a surface can be suppressed by giving the droplet an electrical charge.
[Physics 18, 74] Published Tue Apr 01, 2025
Author(s): Rachel Berkowitz
The fidelity of a complex system’s representation as a network model depends on the diversity of its interconnections.
[Physics 18, s43] Published Tue Apr 01, 2025
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Author(s): Daniele Marinazzo
A new study of complex systems supports a growing trend that focuses more on analyzing a system’s collective behavior rather than on trying to uncover the underlying interaction mechanisms.
[Physics 18, 71] Published Mon Mar 31, 2025
Author(s): David Ehrenstein
Measurements of millions of galaxies suggest that dark energy changes over time and is more complicated than previously thought.
[Physics 18, 72] Published Fri Mar 28, 2025
Author(s): Susan Curtis
Language models such as ChatGPT could help university educators provide more consistent and transparent grades for introductory-level physics exams.
[Physics 18, 67] Published Thu Mar 27, 2025
Author(s): Charles Day
An intense x-ray pulse from a free-electron laser sends a protein’s atoms flying off in directions that reveal the protein’s structure.
[Physics 18, s37] Published Thu Mar 27, 2025
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Next week, a crew of private astronauts is expected to go where no one has gone before. Chun Wang, the crypto entrepreneur who purchased the Fram2 mission from SpaceX in August, announced Friday that the three-to-five-day sojourn — the first human spaceflight to fly directly over the Earth’s poles — is scheduled to launch fromContinue reading "SpaceX’s Fram2 mission will aim for the poles"
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Author(s): Michael Schirber
Experiments with erbium ions show that they can be used to create entangled photons in the telecom band—an important step in building quantum repeaters.
[Physics 18, s41] Published Wed Mar 26, 2025
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After a scrubbed test flight on Monday, a German spaceflight company has determined its next opportunity to launch the first commercial orbital launch vehicle from mainland Europe. Munich-based Isar Aerospace postponed the debut launch of its Spectrum rocket, citing unfavorable winds at Norway’s Andøya Spaceport. On Tuesday, Isar said it will now target Thursday atContinue reading "German firm eyes Thursday for Europe’s first commercial orbital launch"
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Astronomers have finally identified the source of mysterious radio waves from deep space, tracing the signals back to an unusual stellar pair locked in a swift orbit, flashing out their location for the universe to hear. In research published March 12 in Nature Astronomy, a team of astrophysicists finally found the source of strange, minute-longContinue reading "This dead star is still sending us radio signals"
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The quest to send humans to Mars is on: US President Donald Trump talked about it in his inauguration speech this year. Such an epic endeavor could help to answer fundamental questions about the Red Planet, including the biggest question of all: Did Mars once host life — and does it still? Central to thoseContinue reading "Ghost rivers, hidden lakes: The long search for water on Mars"
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Author(s): Katherine Wright
New experiments with virtual reality suggest that locusts do not follow traditional rules of collective behavior.
[Physics 18, 66] Published Tue Mar 25, 2025
Greg Polanski from Kanata, Ontario, Canada The ever-popular Rosette Nebula (NGC 2237–9/46) lies 10° east of Betelgeuse and is an impressive telescopic sight. Deep imaging reveals the line of dark Bok globules — small dense clouds where baby stars are forming — that appear to lie suspended within the nebula. The imager took 12⅓ hoursContinue reading "Bathed in blue"
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To detect neutrinos, scientists use vast observatories located underground, shielded from cosmic ray interference. These detectors rely on Cherenkov radiation, a bluish light produced when high-speed muons, created by rare neutrino collisions, travel faster than light through water or ice. Photomultiplier tubes amplify this light, allowing astronomers to trace the neutrino’s path and energy.
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Author(s): Katrin Erath-Dulitz
The heating effect of microwaves has long been used to accelerate reactions. A new experiment shows that microwaves can also excite molecules into a less reactive state.
[Physics 18, 63] Published Mon Mar 24, 2025
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Astronomers have discovered more than 300 exoplanetary systems that have three or more known planets. Most of these planets are about the same size and spaced close together, earning them the moniker “peas in a pod.” They also orbit near their stars, in many cases closer than Mercury is to the Sun. Our solar system,Continue reading "Our solar system is not as unusual as we thought"
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Could the nearby star Sirius B explode as a type Ia supernova, like some other white dwarf stars in binary star systems have? Bruce MasonEncinitas, California A type Ia supernova occurs when a white dwarf — the cooling remnant of an aging star — draws hydrogen from a companion sun. When the dwarf reaches 1.4Continue reading "Will Sirius B explode as a type Ia supernova?"
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In this episode, Astronomy magazine Editor Dave Eicher invites you to view an unusual event: a partial eclipse of the Sun. Depending on where you are, you might see the Moon cover up to 90 percent of the bright solar disk. Remember, however, even 10 percent of the Sun is dangerous to look at, so wear approvedContinue reading "This Week in Astronomy with Dave Eicher: A Solar Eclipse"
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Greg Meyer from Phoenix, Arizona This dusty figure of the Baby Eagle Nebula (LBN 777) is part of the larger Taurus Molecular Cloud. The dust is dimly lit by young stars within the cloud; the brownish color gives away the presence of larger dust grains. This image comprises nearly 24 hours of LRGB exposure withContinue reading "Cosmic fledgling"
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Author(s): Mark Buchanan
Experiments suggest that cells pack in more ordered patterns as the relative sizes of their nuclei grow.
[Physics 18, 65] Published Fri Mar 21, 2025
Author(s): Matteo Rini
Microsoft’s announcement of achieving a milestone in a potentially transformative approach to quantum computing is met with skepticism by researchers attending the APS Global Summit.
[Physics 18, 68] Published Fri Mar 21, 2025
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The Large Magellanic Cloud (LMC) is one of the Milky Way’s closest neighbors. It’s a small, irregular galaxy that orbits the Milky Way, and is an easy naked-eye object from the Southern Hemisphere. As one of the only galaxies outside our own where telescopes can resolve individual stars and small scale structures, astronomers love toContinue reading "Our near galactic neighbor might have a supermassive black hole"
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Sky This Week is brought to you in part by Celestron. Friday, March 21By 10 P.M. local daylight time, the constellation Canes Venatici the Hunting Dogs is some 45° high in the east. Nestled under the curve of the Big Dipper’s handle, this seemingly innocuous star pattern hosts several popular deep-sky objects. One of thoseContinue reading "The Sky This Week from March 21 to 28: Galilean moon action"
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چه چیزی باعث از بین رفتن توان ستارهزایی در کهکشانهای کمجرم یا کوتوله میشود؟ این سوالی است که منجمان مدتها معتقد بودند پاسخ دقیق به آن را یافتهاند، اما نتایج جدید نشان میدهد که ما هنوز از تصویری دقیق و واقعبینانه دور هستیم.
کهکشانهای کوتوله، که جرم ستارهای آنها حدود یک تا دو میلیارد برابر جرم خورشید یا کمتر است، از رایجترین انواع کهکشانها در کیهان محسوب میشوند. به عنوان مثال، در گروه محلی۱ بیش از ۶۰ کهکشان کوتوله وجود دارد و این تعداد، با بهتر شدن حساسیت تلسکوپها، روز به روز در حال افزایش است. دادههای رصدی وجود تعداد زیادی از کهکشانهای کوتولهی قرمز و خاموش۲ در مراکز پرتراکم کیهان مانند مرکز گروهها و خوشههای کیهانی را تایید میکند، در حالیکه کهکشانهایی که در محیطهای خلوتتر (مانند اطراف گروه محلی یا در محیطهایی خارج از خوشهها) رصد شدهاند، غالبا حاوی گاز و در حال ستارهزایی هستند. بر اساس این مشاهدات این باور کلی به وجود آمده است که محیط تنها عامل خاموششدن ستارهزایی در کهکشانهای کوتوله است.
زمانی که یک کهکشان با سرعت زیاد درون محیط متراکم و داغ گاز خوشهای حرکت میکند، تحت نیرویی به نام فشار ترمزی۳ قرار می گیرد. این نیرو در اثر برخورد و حرکت کهکشان در میان گاز میان خوشهای، بر آن اعمال میشود و میتواند گاز سرد درون کهکشان را از آن خارج کند. هر چقدر جرم کهکشان بیشتر باشد، چاه پتانسیل عمیقتری خواهد داشت و خارج کردن گاز سرد از آن سختتر خواهد بود. چاه پتانسیل کمعمق کهکشانهای کوتوله، آنها را به یک قربانی بسیار ساده برای محیطهای متراکم و شلوغ کیهان تبدیل میکند. مثال بارز این پدیده، کهکشان کوتولهی مسیه ۱۱۰ در فاصله ۲/۷۱ میلیون سال نوری از خورشید است. این کهکشان کوتوله حدود چند میلیارد سال قبل، یعنی درست زمانی که وارد خوشهی محلی میشدهاست، تمامی گاز خود را از دست دادهاست. مسیه ۱۱۰ امروز یک کهکشان کوتولهی خاموش است که با نور قرمز و توزیع نوری کاملا یکنواخت، در تصاویر نجومی خودنمایی میکند.
چرا درک بهتر فرایند خاموششدن کهکشانهای کوتوله تا این اندازه اهمیت دارد؟ پاسخ ساده به این سوال این است که هر آنچه که بتواند ستارهزایی را در کهکشانهای کوتوله متوقف کند، میتواند (با نسبتهای متغیر) سبب خاموششدن کهکشانهای بزرگتر نیز شود. در واقع، مطالعهی آغاز و پایان ستارهزایی در این کهکشانها میتواند یک تصویر دقیق از تمامی فرایندهایی که ستارهزایی در کهکشانها را مدیریت میکند، ارائه دهد. از طرف دیگر، بر اساس مدل استاندارد کیهانشناسی Lambda-CDM، این کهکشانهای کوتوله (یا نمونههای همجرم آنها) بودند که ابتدا در عالم شکل گرفتند و سپس، با ادغامشدن، کهکشانهای بزرگتر را شکل دادند. بنابراین، درک بهتر این کهکشانها در واقع درک بهتر آجرهایی است که عالم امروزی را بنا کردهاند.
اگر محیط تنها عامل خاموششدن ستارهزایی در کهکشانهای کوتوله باشد، بنابراین هیچ کهکشان کوتولهی خاموشی نباید در کمتراکمترین نقاط کیهان، یعنی تهیجاها۴ و رشتههای کیهانی۵ وجود داشته باشد. تهیجاهای کیهانی مناطق وسیعی از کیهان، با ابعاد حدودی ۱۰ تا ۱۰۰ مگاپارسک، هستند که در مقایسه با خوشههای کهکشانی، چگالی مادهی بسیار کمتری دارند. رشتههای کیهانی در مرز میان تهیجاها قرار گرفتهاند. برای راستیآزمایی این فرضیه، ما به سراغ ۴۲ تهیجای کیهانی در بازهی انتقال به سرخ ۰/۰۰۵ تا ۰/۰۵، که کاتالوگ آنها توسط تیم CAVITY جمعآوری شدهاست، رفتهایم. برای بررسی کوتولهها در رشتههای کیهانی نیز از کاتالوگ کهکشانهای رشتهای Dominguez-Gomez et al. 2023 استفاده کردیم. هدف ما پیداکردن تنهاترین کوتولهها در کمتراکمترین نقاط کیهان بود. بنابراین، کهکشانهای کوتولهای را در این تهیجاها و رشتهها انتخاب کردیم که هیچ کهکشان همسایهای، تا فاصلهی ۱ مگاپارسکی، از آنها حضور نداشته باشد. دلیل این انتخاب، مطالعاتی هستند که ثابت کردهاند یکی از علتهای خاموشی در کهکشانهای کوتوله، نزدیکی یا همسایگی با کهکشانهای دیگر است. سپس در این مطالعه به بررسی تاریخچهی ستارهزایی در این کهکشانها با کمک تکنیکهای طیفسنجی، با استفاده از دادههای طیفی Sloan Digital Sky Survey پرداختیم. طیفسنجی یک ابزاری کلیدی و دقیق برای بررسی کهکشانهاست و به ما کمک میکند تا تخمینی از سن، درصد فراوانی آهن (عناصر سنگینتر از هلیوم) و روند ستارهزایی در کهکشان داشته باشیم.
این جستجو سبب شد تا ما گروهی کمیاب از کهکشانهای کوتولهی پرجرم و خاموش را پیدا کنیم که در تنهاترین و کمچگالترین نقاط کیهان حضور دارند. ستارهزایی در این کهکشانها بیش از ۲ میلیارد سال پیش متوقف شدهاست و هیچ گازی در این کهکشانها وجود ندارد. این کهکشانها از نظر برخی خصوصیات مانند اندازه و جرم، تفاوتی با سایر کهکشانهای کوتولهی خاموش در خوشهها ندارند، اما وجه مشترک تمامی آنها، میزبانی از خوشههای ستارهای هستهای۶ است. خوشههای ستارهای هستهای، مجموعهای فشرده از ستارگان هستند که در مرکز بسیاری از کهکشانها، از جمله کهکشانهای کوتوله و حتی در راه شیری پیدا میشوند. این خوشهها از لحاظ جرم و چگالی، درخشانترین و متراکمترین خوشههای ستارهای در کهکشان میزبان خود محسوب میشوند.
در شکل ۲، ما تاریخچهی ستارهزایی این کهکشانها را با نمونههای مشابه (از نظر جرم) در خوشههای بزرگ کیهانی مقایسه کردیم. آنچه که قابل توجه است، شباهت میزان ستارهزایی در برخی از این کهکشانهای کوتولهی خاموش در تهیجاها و رشتهها با گروهی از کهکشانهای کوتوله است که امروزه در مرکز خوشههای کیهانی قرار دارند. کهکشانی که امروز در مرکز یک خوشهی کیهانی قرار داشته باشد، بیش از ۵ میلیارد سال را در آن خوشه زندگی کردهاست و این به معنای قرارگرفتن در معرض تمامی محرکهای محیطی برای بیش از ۵ میلیارد سال است. به بیان دیگر، ما شاهد دو گروه از کهکشانهای کوتوله در محیطهایی کاملا متفاوت با فعالیتهای ستارهزایی کاملا مشابه هستیم. هر دو گروه بیش از ۴ میلیارد سال پیش به ستارهزایی خود خاتمه دادهاند. از سویی دیگر، کهکشانهای کوتولهای که امروزه در اطراف خوشهها قرار دارند (یعنی مدت زمان بسیار کمی را در معرض محرکهای محیطی بودهاند) اما حضور یک خوشه ستارهای هستهای در آنها تایید شدهاست، در ستارهزایی، رفتاری مشابه با کهکشانهای خاموش تهیجاای و رشتهای دارند. سوالی که پیش میآید این است: در نبود محرکهای محیطی، چه چیزی سبب از بین رفتن ستارهزایی در این کهکشانها میشود؟
شکل ۲. نمودار درصد جرم ستارهای تشکیلشده در کهکشانها بر حسب زمان. در تصویر فوق، متوسط فعالیت ستارهزایی کهکشانهای کوتولهی خاموش و منزوی (نشان داده شده با خطوط ممتد) را با فعالیت ستارهزایی کهکشانهای کوتولهی خاموش خوشهای مقایسه کردهایم. کهکشانهای کوتولهای که در مرکز خوشهها قرار دارند با خطچین و کهکشانهای کوتولهای که در خوشهها، میزبان خوشههای ستارهای هستهای هستند، با نقطهچین مشخص شدهاند. خطوط بنفش کهکشانهایی که ستارهزایی سریعی داشتهاند و خطوط صورتی کهکشانهایی که هاله و جمعیت ستارهای خود را در بازهی زمانی طولانیتری شکل دادهاند، نمایش میدهد.
در سال های اخیر، فعالیت هستههای کهکشانی فعال۷ به عنوان یکی از فرآیندهای خاموشی ستارهای در کهکشانهای کوتوله مورد بحث بودهاست. فعالیت هستهای کهکشانی فعال به فعالیتهای شدید و پرانرژی در مرکز برخی از کهکشانها اطلاق میشود که معمولا ناشی از حضور یک سیاهچالهی پرجرم است. یک سیاهچاله با جذب ماده، انرژی زیادی را به صورت تابش در طول موجهای مختلف تابش میکند. این تابش با افزایش دمای گاز میانستارهای و به بیرون راندن بخشی از این گاز، به خاموشی فعالیت ستارهزایی در کهکشان منجر میشود. بر اساس دادههای موجود، ما نتوانستیم حضور یا عدم حضور سیاهچاله در مرکز این کهکشانهای کوتولهی خاموش را تایید کنیم. از آنجایی که در این بازهی جرمی، معمولا یافتن سیاهچالههای مرکزی و تمیزدادن آنها از خوشههای ستارهای هستهای کار دشواری است، برای بررسی و مطالعهی این موضوع به دادههای رصدی بهتری نیاز است.
مطالعات اخیر ثابت کردهاند که کهکشانها، فارغ از جرم و محل سکونتشان، دو نوع ستارهزایی را در طول زندگی خود تجربه میکنند: ستارهزایی کوتاهمدت و بلندمدت. در شکل ۲، این دوگانگی در فعالیت ستارهزایی، حتی در یک نمونهی کوچک کهکشانهای خاموش تهیجاای و رشتهای، مشهود است.
کهکشانهایی که هاله و جمعیت ستارهای خود را خیلی سریع شکل میدهند، فارغ از محیط امروزیشان، رفتار ستارهزایی مشابهی دارند. این امر در مقایسهی بین کهکشانهای تهیجا و خوشهای در شکل ۲، قابل تشخیص است. این بدان معناست که این کهکشانها در یک بازهی زمانی خیلی کوتاه، بخش بزرگی از جمعیت ستارهای خود را تشکیل دادهاند. ستارهزایی در این بازهی کوتاه، به معنای تشکیل بادهای ستارهای و فعالیتهای ابرنواختری۸ شدید است. این فعالیتها میتوانند با افزایش دمای گاز میان ستارهای و به بیرون راندن بخش زیادی از گاز، سبب خاموش شدن کهکشانهای کوتوله شوند. البته نقش کلیدی بادهای ستارهای در خاموشی کهکشانهای کوتولهی کم جرم تا به حال اثبات شده است اما نقش این فرایند برای کهکشانهای کوتولهی پرجرم، هنوز به درستی درک نشدهاست. ستارهزایی شدید، فعالیتهای ابرنواختری و بادهای ستارهای پس از آن، میتوانند سبب خاموشی کهکشانهای کوتوله در تهیجاها و حتی در مرکز خوشههای کیهانی شوند اما بررسی دقیقتر این موضوع، منوط به بررسی داده های دقیقتر و مناسبتر است.
همچنین کهکشانهای کوتولهای که هاله و جمعیت ستارهای خود را در بازهی زمانی طولانیتری ساختهاند، اما میزبان یک خوشهی ستارهای هستهای هستند، فارغ از محیطی که در آن زندگی می کنند رفتار ستارهزایی مشابهی را از خود نشان میدهند. این امر میتواند بدان معنا باشد که شکلگیری یا حضور یک خوشهی ستارهای هستهای ممکن است به خاموشی کهکشانهای کوتولهی میزبان منجر شود. از یک زاویهی دیگر، میتوان گفت که شکلگیری خوشهی ستارهای هستهای، خود نتیجهی یک فرآیند خاموشی (مثل انفجارهای ابرنواختری یا حضور فعالیتهای هستهای کهکشانی) است و پیدا کردن آنها، مانند یافتن رد پای فرآیندهای خاموشی، به غیر از محرکهای محیطی، در این کهکشانهاست.
آنچه که سبب خاموشی کهکشانهای کوتولهی پرجرم منزوی۹ در تهیجاها و رشتهها شدهاست، هنوز برای ما مشخص نیست. در این مقاله و با استناد به دادهها و نتایجی که بهدست آوردیم، تنها میتوانستیم حدسهایی را در خصوص فرآیندهای مسئول ارائه دهیم و یافتن پاسخ دقیقتر، وابسته به ارزیابی و بررسی دادههای بهتر است. یافتن این جمعیت بسیار کمیاب از کهکشانهای کوتولهی خاموش در انزوا بدان معناست که بر خلاف باورهای رایج قبلی، محیط تنها عامل خاموشی کهکشانهای کوتوله نیست و ما هنوز از یک تصویر واقعبینانه از فیزیک باریونی در کهکشانها و فرایندهای مسئول در خاموشی کهکشانهای کوتوله بسیار فاصله داریم.
۱. Local group
۲. Quenched
۳. Ram pressure
۴. Voids
۵. Filaments
۶. Nuclear star cluster
۷. Active galactic nuclei
۸. Supernova feedback
۹. Isolated dwarf galaxy
شکل بالای صفحه: کهکشان کوتولهی مسیه ۱۱۰ در فاصله ۲/۷۱ میلیون سال نوری از خورشید. منبع: https://www.starkeeper.it/M110.htm
عنوان اصلی مقاله: The Puzzle of isolated and quenched dwarf galaxies in cosmic voids
نویسندگان: .Bahar Bidaran et al.
لینک اصلی مقاله: https://arxiv.org/pdf/2408.05273
گردآوری: بهار بیداران
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You know, after decades of pointing optics toward the sky, I consider myself a knowledgeable observer. But while researching the Pleiades a few months back, I was surprised to learn that it wasn’t the brightest star cluster. And there were other surprises when I started comparing overall brightnesses of deep-sky objects. For instance, you mightContinue reading "Observe the brightest deep-sky objects"
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SpaceX, the world’s dominant commercial space launch provider, is looking to ramp up the activity of its workhorse rocket. The FAA on Friday released a draft environmental assessment (EA) analyzing the company’s proposal to more than double the number of Falcon 9 launches from Space Launch Complex 40 (SLC-40) at Cape Canaveral Space Force StationContinue reading "SpaceX proposal would more than double Falcon 9 launches at Cape Canaveral"
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In this episode, Astronomy magazine Editor Dave Eicher invites you to head out soon and look at the planets in the evening sky. The highest is Mars, the so-called Red Planet. The giant planet Jupiter is a bit lower but much brighter. Brightest of all is Venus, low in the west. If you want to see thatContinue reading "This Week in Astronomy with Dave Eicher: The Planets Align"
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Astronomers and space scientists are living in a state of fear and anxiety as the Trump administration and Elon Musk-led U.S. DOGE Service target science spending and diversity initiatives with actions that are already damaging research and threaten to set back U.S. scientific leadership for years, scientists tell Astronomy. The assault began during Trump’s firstContinue reading "Space scientists fearful as Trump administration targets science and mulls NASA cuts"
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Author(s): David Lindley
Researchers proposed methods to preserve the integrity of quantum bits—techniques that may become the key to practical quantum computing on a large scale.
[Physics 18, 59] Published Fri Mar 14, 2025
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Philippe Moussette, taken at Cap-Rouge, Quebec, Canada The reddened shadow of Earth falling upon the Moon during the lunar eclipse of March 13/14 — a so-called Blood Moon — is captured in this sequence taken with a Canon mirrorless camera and 600mm lens.
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The public is enamored of images returned to Earth by space probes. Whether they show the moons of Jupiter, the rings of Saturn, or the icy surface of Pluto, these captivating images garner loads of attention. In addition to cameras, robotic probes always carry an array of scientific instruments that get far less attention fromContinue reading "Why so many spacecraft carry magnetometers"
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Sky This Week is brought to you in part by Celestron. Friday, March 14The Moon reaches Full phase early this morning at 2:55 A.M. EDT, with a total lunar eclipse underway. Everyone across the U.S. can watch the event, and no special equipment is needed — just your eyes! Totality begins about half an hourContinue reading "The Sky This Week from March 14 to 21: The start of spring"
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Author(s): Katherine Wright
Researchers have proposed methods to tune the properties of altermagnets, a step toward practical applications for this new form of magnet.
[Physics 18, 58] Published Thu Mar 13, 2025
Author(s): Charles Day
Illuminating a metasurface with a laser can enable the rapid modulation of the polarization of terahertz light transmitted through the metasurface.
[Physics 18, s24] Published Thu Mar 13, 2025
Author(s): Yuval Grossman and Yosef Nir
A symmetry violation has been observed in a particle-decay process that—together with five related decays—could shed light on the matter–antimatter imbalance in the Universe.
[Physics 18, 56] Published Wed Mar 12, 2025
Author(s): Ryan Wilkinson
Time crystals realized in the so-called quasiperiodic regime hold promise for future applications in quantum computing and sensing.
[Physics 18, s28] Published Wed Mar 12, 2025
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Jamie Cooper from Northamptonshire, U.K. Craters dot the Moon’s rugged south pole region in this shot taken March 7 with a 16-inch Dobsonian. The central-peak crater just above and left of center is Moretus, and Clavius is the large crater at lower right (with multiple smaller craters inside).
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We’ve always known Mars as the Red Planet — but it turns out, we may have had the reason why wrong. If so, it could revise much of what we know about the history of our smaller neighbor planet. In a study published Feb. 25 in Nature Communications, researchers tied the nature of Mars’ redContinue reading "Could Mars’ red color have formed under wet conditions?"
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A recent paper suggests that if astrobiologists want to make an educated guess about what life on Venus might look like, they should look to a weird microbe called A. ferrooxidans, found here onEarth. Earthly life-forms are the only examples we have of what life looks like, so astrobiologists often study them for clues aboutContinue reading "Strange microbes on Earth might help us understand life on Venus"
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Author(s): Samuel Jarman
JWST observations reveal two distinct types of flares from the Milky Way’s black hole, suggesting that they originate from two different electron-acceleration mechanisms within the supermassive black hole’s accretion disk.
[Physics 18, 55] Published Tue Mar 11, 2025
Author(s): Marric Stephens
Experiments have shown that heavy-ion irradiation of biomolecules in aqueous environments efficiently triggers DNA-destroying cascades.
[Physics 18, s32] Published Tue Mar 11, 2025
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Comets develop the spectacular long tails that they are known for by approaching the Sun. When they get too close, their icy volatile materials begin to sublimate away, carrying along clouds of dust. But this activity usually only happens relatively close to the Sun, as comets spend most of their time in the outer solarContinue reading "Astronomers have spotted the most distant comet ever discovered"
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During the night of March 13, most of North and South America will be treated to a total lunar eclipse, an event popularly referred to as a Blood Moon. The event is aptly named — the Moon is cast in a dark red, brown, or orange color during totality, giving it an eerie appearance inContinue reading "How to get the most out of the lunar eclipse"
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Author(s): David Lindley
Theorists proposed an idea they called quantum teleportation—a means of transferring the identity of one particle to another over some distance.
[Physics 18, 52] Published Mon Mar 10, 2025
Author(s): Davide Donadio and Giulia Galli
Computational spectroscopy reveals a possible signature of strongly hydrogen-bonded wires in water and ice.
[Physics 18, 54] Published Mon Mar 10, 2025
Author(s): Philip Ball
Tech giant Microsoft claimed in a recent press release to have made the first topological qubit–an important milestone in the development of quantum computers. But some experts say the firm’s claim has not been backed up by peer-reviewed research.
[Physics 18, 57] Published Mon Mar 10, 2025
Simon Todd, taken from Haywards Heath, U.K. The Christmas Tree Cluster lies at the center of this image, filled with young, newborn stars and surrounding nebulosity cataloged as NGC 2264. That includes the Cone Nebula, just left of center. The Fox Fur Nebula lies directly below the bright blue star (S Monoceros) at center. ThisContinue reading "Stellar nativity scene"
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If you weigh a certain amount on Earth, how much less or more would you weigh on the Moon? MakaylaArkansas The short answer is that you would weigh roughly one-sixth your Earth weight on the Moon. So if your bathroom scale reads 180 pounds (81.6 kilograms) on Earth, it would read 30 pounds (13.6 kg)Continue reading "How much less would you weigh on the Moon than on Earth?"
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Saturn’s largest moon, Titan, is particularly captivating for scientists. This is thanks in large part to its status as the only other planetary body in the solar system known to host an atmosphere about 1.5 times denser than Earth’s and bodies of liquid on its surface. (Unlike Earth, however, where most surface liquid is water,Continue reading "Cryovolcanism on Titan may replenish its thick atmosphere"
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In this episode, Astronomy magazine Editor Dave Eicher invites you to head out on the evening of March 13. That’s when one of the year’s best celestial events — a total eclipse of the Moon — will begin. It will continue into the early morning hours of the 14th, so if you want to see it all, get ready for aContinue reading "This Week in Astronomy with Dave Eicher: A Total Eclipse of the Moon"
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One of the most competitive segments in the amateur telescope marketplace these days spans 3- to 5-inch apochromatic refractors. Once considered telescopes for the well-to-do, these instruments are now affordable to many backyard stargazers. And one of the newest companies to enter this market segment is Starfield Optics from Caledon, Ontario, a suburb of Toronto.Continue reading "We test Starfield Optics’ 115mm Géar Triplet APO"
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Rob Lyons, taken from Vancouver, Canada This wide-field vista spans the constellations Cepheus and Cassiopeia and includes an host of deep-sky objects. From left to right: NGC 7822 (the Question Mark Nebula), LBN 576 (the Garlic Bulb Nebula), NGC 7635 (the Bubble Nebula), Sharpless 2–157 (the Lobster Claw Nebula), and Sharpless 2–155 (the Cave Nebula).Continue reading "Group photo"
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Intuitive Machines’ IM-2 mission has ended after its lunar lander, Athena, apparently toppled over as it touched down and came to rest on its side yesterday in a shadowed crater, the company announced. In a statement released this morning, the company said its batteries had run out and they did not expect it to reawaken.Continue reading "Intuitive Machines’ IM-2 Moon lander is lying dead in a crater"
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Author(s): Charles Day
A neutron-scattering experiment has confirmed the existence of an unusual phase of ice that forms at high temperature and high pressure.
[Physics 18, 47] Published Fri Mar 07, 2025
Author(s): Elizabeth Fernandez
The discovery of a mini aurora above a light-emitting polymer material reveals an electron-ejection process that might be useful in field-emission displays and material fabrication.
[Physics 18, 51] Published Fri Mar 07, 2025
Author(s): Dan Garisto
In 1964, Bell showed that quantum physics predicts correlations that violate certain inequalities. The work implied that quantum mechanics is not compatible with locality, even if there were “hidden variables” not accounted for in quantum theory.
[Physics 18, 53] Published Fri Mar 07, 2025
Millions of viewers who tuned into Thursday’s broadcast of SpaceX Starship’s eighth test flight experienced a collective déjà vu as the mammoth rocket exploded and rained down flaming hunks of metal in eerily similar fashion to Flight 7. So too did pilots flying over the Caribbean ocean, many of whom were forced to change course to avoid theContinue reading "SpaceX Starship explodes, disrupts air travel a second time"
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All lunar eclipses — whether penumbral, partial, or total — offer us thought-provoking views of Earth’s shadow. Frequently, lunar eclipses offer up peculiar color effects, with the shadowed Moon appearing reddish due to the state of Earth’s atmosphere. But the March 14, 2025, total lunar eclipse all but guarantees additional optical phenomena of a differentContinue reading "Look for these effects during the next lunar eclipse"
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