New 'Tron: Ares' trailer paints the town neon red as an ominous voice declares that 'Military AI is the future!' (video)
On Sept. 1, 1859, amateur astronomer Richard Carrington observed a massive eruption of bright light from the Sun’s surface. It was the first recorded observation of a solar flare. Within only 17.5 hours, a coronal mass ejection (CME) – an expulsion of plasma and magnetic waves that often accompanies flares and prominences – reached Earth,Continue reading "Sept. 2, 1859: The Carrington Event peaks"
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Mercury passes 1.2° north of Regulus at 6 A.M. EDT; the pair is visible in the east just before sunrise, but it might be a challenging observation. You’ll want to get to a location above the surrounding terrain if possible, with an eastern horizon free of tall trees or buildings. Rising around 5:30 A.M. localContinue reading "The Sky Today on Tuesday, September 2: Mercury meets Regulus"
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In this episode, Astronomy magazine Editor Emeritus Dave Eicher invites you to head out during the early morning hours the first week of September. It’s then when you’ll see the brilliant planet Venus pass by the Beehive Cluster, which lies in the constellation Cancer the Crab. Venus will be easy to spot but if twilight has started,Continue reading "This Week in Astronomy with Dave Eicher: Venus and the Beehive"
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Humanity is obsessed with astronomical record keeping. The Babylonians compiled their first listing of the stars in the 12th century b.c.e. Around 1000 b.c.e., they followed it with an expanded catalog that includes familiar constellations and star clusters, as well as motions of the Sun, the Moon, and the planets. The Mayans inscribed into stoneContinue reading "An introduction to common astronomical catalogs"
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Cepheid variables are some of the most well-known variable stars in the sky, responsible for helping astronomers accurately measure cosmic distances and famously clueing Edwin Hubble in to the fact that the Andromeda Galaxy was far beyond the Milky Way. So, tonight let’s begin September by finding the Cepheid variable that started it all: DeltaContinue reading "The Sky Today on Monday, September 1: Observe Delta Cephei"
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On Sept. 1, 1804, German astronomer Karl Ludwig Harding peered through a 5-centimeter refracting telescope at a private observatory near Bremen, and discovered a celestial body he named Juno. Harding was part of the so-called Celestial Police. This group of astronomers had dedicated themselves to the search for the “missing planet” that the Titius-Bode lawContinue reading "Sept. 1, 1804: Karl Harding spots 3 Juno"
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September’s sky is rich with opportunities. Titan’s shadow continues to transit Saturn. The ringed planet reaches opposition along with Neptune, with both worlds in the same region of the sky. Mars is descending toward solar conjunction. Uranus is a fine binocular target, while Jupiter dominates the early morning. Venus starts the month near M44, thenContinue reading "September 2025: What’s in the sky this month? Saturn and Neptune reach opposition, as Jupiter and Venus greet the dawn"
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The evening sky boasts two naked-eye planets. Start your night’s viewing with ruddy Mars, which lies in the west as darkness falls. It treks eastward against the backdrop of Virgo, passing 2° north of the Maiden’s brightest star, 1st-magnitude Spica, on Sept. 12. The Red Planet shines at magnitude 1.6, slightly fainter than the blue-whiteContinue reading "September 2025: What’s in the Southern Hemisphere sky this month?"
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On Aug. 31, 1913, Alfred Charles Bernard Lovell was born in England. When he was 15, a school trip to hear a lecture on electricity prompted a keen interest in science and math, and Lovell would go on to study physics at Bristol University. He graduated with honors in 1934 and finished his Ph.D. onlyContinue reading "Aug. 31, 1913: Birth of Bernard Lovell"
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Bright Venus hangs near the lovely Beehive Cluster (M44) in Cancer this morning. Both rise more than two hours before the Sun and reach nearly 20° high in the east an hour before sunrise. Venus shines at magnitude –3.9, a blazing beacon just 1.4° southwest (to the upper right) of the Beehive. At magnitude 3.1,Continue reading "The Sky Today on Sunday, August 31: Venus hangs with the Beehive"
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The third member of NASA’s space shuttle program, Discovery had a fraught journey to its launch. First, a test in June of 1984 found a flaw in the thermal shield; then a launch scheduled for later the same month was delayed due to a computer failure. Attempt No. 2 was halted only four seconds beforeContinue reading "Aug. 30, 1984: Space Shuttle Discovery launches"
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Saturn’s moon Iapetus reaches greatest western elongation today, now located 9.5’ west of the ringed planet. Iapetus has two vastly different hemispheres, one light and one dark. As the moon orbits Saturn, it slowly rotates so that one and then the other side faces us, with its brightness varying vastly depending on which region isContinue reading "The Sky Today on Saturday, August 30: Iapetus reaches western elongation"
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On Saturday, September 20, an ambitious project will be announced and celebrated in Animas, New Mexico, which lies near the Arizona border. And you’re invited. Dubbed “Lunar Base Alpha,” it will replicate the lunar landscape and feature rovers conducting science experiments and habitats that you’ll be able to stay in. The initial project will coverContinue reading "Experience the Moon on Earth"
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The first light from the explosion that was the death of a massive star in the nearby Large Magellanic Cloud reached Earth on Feb. 23, 1987. Supernova 1987A’s proximity gave astronomers unprecedented access into the final stages of stellar life, and in 1990, the Hubble Space Telescope began taking high-res images of the former star.Continue reading "Aug. 29, 1990: Hubble sees Supernova 1987A clearly"
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Rodney Pommier, taken from Portland, Oregon Roughly 40 million years ago near the core of the spiral galaxy NGC 7331, a white dwarf star ended its life in a thermonuclear explosion. The light from that explosion was detected July 14 by the Gravitational-wave Optical Transient Observer project. This astroimager acquired the shot on the leftContinue reading "Spot the supernova"
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This evening Titan stands east of Saturn and Iapetus is far to the west, the latter approaching its greatest western elongation tomorrow. You can find the ringed planet already 15° high in the east at 10 P.M. local daylight time, continuing to rise until around 2:30 A.M., when it reaches the highest point in itsContinue reading "The Sky Today on Friday, August 29: Saturn’s moons line up"
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Sky This Week is brought to you in part by Celestron. Friday, August 29The waxing Moon lies in southern Libra tonight. Our satellite is quickly approaching Scorpius, where it will meet the Scorpion’s brightest star in just a few days. High in the southeast in the few hours after sunset is the small constellation SagittaContinue reading "The Sky This Week from August 29 to September 5: Saturn’s time to shine"
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Patrick A. Cosgrove from Honeoye Falls, New York Sharpless 2–124 is a faint emission nebula located around 15,000 light-years away in Cygnus. This image reveals intricate filaments of dust crossing the bright central region, reminiscent of the Trifid Nebula (M20). The imager took 14.2 hours of SHO and LRGB data with a 2.8-inch f/5.6 astrograph.
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iAFS2 automatic focuser iOptronWoburn, MA The iAFS2 automatic focuser is designed to stay focused even after it is adjusted. It allows the user to control its movement three ways: by connecting to a computer, with affixed adjuster buttons, or with a manual focus wheel. The focuser also features a built-in temperature sensor and two USBContinue reading "Make summer last with these new astronomy products"
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A team of scientists claims a computational tool for studying black hole collisions could be our best bet for answering mysterious questions about the universe’s origins. In a new paper in Living Reviews in Relativity, they argue for applying a technique called numerical relativity to peer into the moment before the Big Bang. At itsContinue reading "Scientists seek to discover what came before the Big Bang"
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The Northern Hemisphere’s summer is — by far — the best time to view our galaxy’s rich star fields. And it’s during summer that the spectacular Wild Duck Cluster flies through the Milky Way. German astronomer Gottfried Kirch discovered the Wild Duck Cluster in 1681. Messier made it his 11th catalog entry May 30, 1764,Continue reading "Michael’s Miscellany: Observe the Wild Duck Cluster"
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Engineers at NASA successfully tested key hardware for the Nancy Grace Roman Space Telescope in a crucial two-day sequence on Aug. 7 and 8, according to an Aug. 26 press release from the agency. In simulated space-like conditions, the team confirmed that the telescope’s four solar panels and a unique, visor-like sunshade will unfold asContinue reading "Watch as the Roman Space Telescope unfurls its solar panels and visor in successful test"
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The space probe Galileo was launched in 1989 with the goal of studying Jupiter and its moons. On its way to the gas giant, it became the first spacecraft to do a flyby of an asteroid as it zoomed past 951 Gaspra on Oct. 29, 1991. Then, on Aug. 28, 1993, Galileo made its secondContinue reading "Aug. 28, 1993: An asteroid harbors a surprise"
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Comet C/2024 E1 (Wierzchoś) is passing less than 0.5° from magnitude 5.4 Lambda (λ) Coronae Borealis in the western sky this evening. The comet is quite faint at 15th magnitude, so you’ll want a dark observing site and a large scope to net it. Fortunately, you have the luxury of waiting until the sky isContinue reading "The Sky Today on Thursday, August 28: Comet Wierzchoś passes Lambda Coronae Borealis"
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In the late 20th century, when we still captured celestial images on film, the few days around New Moon were the only times we could image deep-sky objects. The grainy, low-sensitivity films we used back then demanded the darkest skies possible for quality portraits. When First Quarter arrived, it was time to say goodbye toContinue reading "Tips for imaging during a Full Moon"
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SpaceX’s more than 400-foot-tall Starship rocket returned to form Tuesday, deploying its first payload and completing critical heat shield tests following a string of in-flight and preflight failures. The spacecraft experienced different issues on each of its previous three test flights, with explosions in January and March disrupting air travel. In June, a Starship exploded on the test stand asContinue reading "SpaceX Starship Flight 10 viewed as roaring success"
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New research suggests a giant impact may not have been responsible for the formation of Jupiter’s core. Most planetary scientists thought that a colossal collision with an early planet containing half of Jupiter’s core material could have mixed up the central region of the gas giant enough to explain its interior today. But a newContinue reading "A new theory explains how Jupiter’s core formed"
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When the Sun, Earth, and Mars all align so that from an earthly perspective, Mars is opposite the Sun, Mars is said to be at opposition. Mars oppositions happen about every other year, and at opposition – or rather, within a few days of it – Mars is also at its closest approach to EarthContinue reading "Aug. 27, 2003: Mars zooms in"
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José J. Chambó, taken from Farm Hakos, Namibia Comet C/2025 K1 (ATLAS) glides by the star 9 Herculis in this Aug. 21 image, glowing with a greenish coma about 2′ wide and a 20″ tail. Captured at roughly magnitude 12.5, this icy visitor was 0.33 astronomical units (the average Earth-Sun distance) from the Sun. TheContinue reading "A comet in Hercules"
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The Moon moves 1.2° south of Spica during the daylight hours, sitting due south of Virgo’s luminary at 11 A.M. EDT. By this evening, a new line has formed in the sky, with Spica now between Mars and the Moon, which sits to the star’s left. An hour after sunset, Spica is still some 7°Continue reading "The Sky Today on Wednesday, August 27: The Moon moves past Spica"
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دادههای تلسکوپ فضایی جیمز وب اطلاعات ارزشمندی دربارهی فرآیند ستارهزایی درون کهکشانها به دانشمندان میدهد. توان تفکیک بالای این تلسکوپ، همراه با پوشش گستردهی طولموجی ( از ۰/۵ تا ۳/۵ میکرومتر)، امکان مطالعهی کهکشانها را در انتقالبهسرخهای بالاتر و با درخشندگیهای سطحی پایینتر برای منجمان فراهم میسازد. یکی از موضوعات کلیدی در مطالعهی ستارهزایی کهکشانها، بررسی تودههای۱ چگال و ستارهزا است. این تودهها که در طولموج فرابنفش۲ و تابش هیدروژن-آلفا۳ بهوضوح قابل مشاهدهاند، بخش قابلتوجهی از نرخ تشکیل ستاره در کهکشان را به خود اختصاص میدهند. در انتقالبهسرخهای پایین (کمتر از ۰/۱۵)، پژوهشهای گستردهای دربارهی ارتباط میان نرخ ستارهزایی و فلزیت۴ در تودهها انجام شده است. در مطالعهی ساختار کهکشانها، «فلزیت» به میزان حضور عناصر سنگینتر از هیدروژن — که حاصل فرایندهای هستهای در ستارگان هستند — در محیط گازی یا درون خود ستارگان گفته میشود. این نتایج نشان میدهند که ورود گازهای با فلزیت پایین به درون کهکشان میتواند با افزایش منابع سوخت ستارهزایی، موجب تشدید نرخ تشکیل ستاره شود. در عین حال، ورود این گازها موجب تغییر در ترکیب شیمیایی گازهای درون کهکشان شده و با رقیق کردن آن، میزان فلزیت درون تودههای ستارهزا را کاهش میدهد.
نویسندگان این مقاله با بهرهگیری از دادههای تصویری و طیفی تلسکوپ فضایی جیمز وب، به مطالعهی کهکشانهایی میپردازند که تودههای ستارهزایی در آنها دیده شدهاند. هدف اصلی این مطالعه، بررسی فلزیت و میزان تغییرات آن در این نوع از کهکشانها در انتقال به سرخ بین ۰/۶ تا ۱/۳۵ است. این بازهی انتقالبهسرخ بهگونهای انتخاب شده است که خطوط نشری هیدروژن-آلفا (Hα) و گوگرد ۳ (SIII) در طیف این کهکشانها قابل مشاهده باشند. خط هیدروژن-آلفا نشاندهندهی تابش ناشی از بازترکیب هیدروژن یونیزه است. در نواحی ستارهزا، مناطقی از گاز هیدروژن یونیزه وجود دارد که پیرامون ستارگان جوان و پرجرم تشکیل میشوند. این ستارگان با تابش فوتونهای پرانرژی، اتمهای هیدروژن اطراف را یونیزه کرده و باعث جدا شدن الکترونهای آنها میشود. زمانی که این الکترونها دوباره با هستههای هیدروژن ترکیب میشوند، در طولموجهای مشخصی تابش میکنند، که شامل خطوط بازترکیب هیدروژن مانند هیدروژن-آلفا (از سری خطوط بالمر هیدروژن با طول موج ۶۵۶۳ آنگستروم) میشود. میزان تابش این خط مستقیماً با میزان فعالیت ستارگان جوان و در نتیجه نرخ ستارهزایی اخیر در کهکشان مرتبط است. گوگرد ۳ نیز یکی از مهمترین خطوط طیفی برای مطالعهی فلزیت است، زیرا نسبت شدت آن به خطوط دیگر، بهویژه خطوط دیگر گوگرد و اکسیژن، به دما و ترکیب شیمیایی گاز حساس است و میتواند برآورد دقیقی از فراوانی عناصر سنگینتر (فلزیت) در محیط ارائه دهد.
تصویر شماره ۱ چندین نمونه از کهکشانهای مطالعه شده در این مقاله را نشان میدهد. یکی از مزایای دادههای طیفی و تصویری جیمز وب، وضوح بالای آنها از نظر توان تفکیک طیفی۵ و مکانی۶ است. این ویژگی امکان مطالعهی کهکشانها را در مقیاسهای کوچکتر و با جزئیات بیشتر فراهم میکند. در هر ردیف نمایش داده شده در تصویر شماره ۱، تصویر رنگی از کهکشان، نقشههای تفکیکی۷ از تودههای ستارهزا، میزان ستارهزایی و فلزیت به ترتیب از چپ به راست نمایش داده شده است. با توجه به این تصاویر، بهوضوح میتوان مشاهده کرد که فلزیت این تودههای ستارهزا نسبت به سایر نواحی نشانداده شده از کهکشان کمتر است .
شکل ۱. نقشههای تفکیک شده از سه کهکشان نمونه . هر ردیف شامل تصویر رنگی کهکشان، نقشهی تفکیک شدهی تودههای ستارهزا، نقشهی لگاریتمی نرخ ستارهزایی و همچنین نقشهی لگاریتمی فلزیت محاسبه شده در نواحی مختلف کهکشان (از چپ به راست) است.
نویسندگان در ادامه برای مقایسهی فلزیت تودههای ستارهزا با فلزیت نواحی اطراف آن، ابتدا فلزیت داخل تودهها و سپس دیسک خارج از آنها را اندازهگیری میکنند. در نمودار سمت چپ تصویر شمارهی ۲، فلزیت مربوط به تودهها و دیسک اطراف آنها نمایش داده شده است. برازشهای خطی نشان میدهند که تودههای ستارهزا عموماً فلزیتی کمتر از دیسک پیرامونشان دارند، که بیانگر رقیقشدن گاز در این تودهها است. نمودار سمت راست، میانهی فلزیت اندازهگیریشده برای همهی تودههای ستارهزای هر کهکشان نشان میدهد. شواهدی از وجود دو جمعیت احتمالی در این کهکشانها دیده میشود: کهکشانهایی که فلزیت تودههای آنها مشابه فلزیت دیسک پیرامونشان است، که با رنگ قرمز نشان داده شدهاند و نزدیک به خط برابری قرار دارند و کهکشانهایی که تودههایشان اختلاف فلزیت بیشتری دارند، که با رنگ آبی نمایش داده شدهاند.
شکل ۲. نمودار سمت چپ: فلزیت هر تودهی ستارهزا و دیسک پیرامونش به همراه خط برازش خطی و همچنین خطچین ۱:۱ (برابری فلزیت). نمودار سمت راست: مقدار میانهی به دست آمده برای فلزیت تودهها در هر کهکشان. نقاط قرمز کهکشانهایی با اختلاف فلزیت کم و نزدیک به خط برابری و نقاط آبی کهکشانهایی با اختلاف بیشتر را مشخص میکنند.
آنچه احتمالاً در اینجا مشاهده میکنیم این است که کهکشانهایی با اختلاف فلزیت کمتر بین تودههای ستارهزا و دیسک پیرامونشان (رنگ قرمز در نمودار سمت راست شکل ۲) ممکن است عمدتاً تودههای ستارهزای خود را از طریق ناپایداریهای دیسکی تشکیل داده باشند و بنابراین این تودهها از گازی که پیشتر در خود کهکشان وجود داشته شکل گرفته باشند و منجر به اختلاف فلزیت کم بین آنها و محیط پیرامونشان شده باشد. در مقابل، کهکشانهایی با اختلاف فلزیت بیشتر تودههای ستارهزا و دیسک پیرامونشان (رنگ آبی در نمودار سمت راست شکل ۲) احتمالاً تودههایشان را از گازهای ورودی به کهکشان تشکیل دادهاند. این گاز که فلزیت کمی دارد، میتواند باعث افزایش میزان ستارهزایی در این تودهها شود، و همزمان با رقیق کردن محیط باعث کاهش فلزیت تودهها شود.
شکل ۳. توزیع فلزیت و تابش هیدوژن-آلفا در یک کهکشان نمونه. تودههای ستارهزا به صورت نواحی بنفش کوچک بر روی پسزمینهی نارنجی کهکشان دیده میشوند. پنلهای سمت راست: نقشههای تفکیکی از کهکشان برای نرخ ستارهزایی به دست آمده از شار هیدوژن-آلفا، نرخ ستارهزایی ویژه، و فلزیت را نشان میدهند. پنل پایین، تغییرات هیدوژن-آلفا (نقاط سبز) و فلزیت (خطوط سفید) را در طول نواری که روی کهکشان مشخص شده، نمایش میدهد.
نویسندگان این مقاله پس از بررسی تغییرات فلزیت در نواحی مختلف کهکشان، به دنبال یافتن ارتباط میان نرخ ستارهزایی و فلزیت هستند. نقشههای نرخستارهزایی و فلزیت (تصویر شماره ۱) نشان میدهد که کاهش فلزیت در تودههای ستارهزا با افزایش نرخ ستارهزایی ارتباط دارد. برای بررسی بیشتر این ارتباط، آنها یک کهکشان خاص را که درتصویر شماره ۳ نشان داده شده است، بررسی کردهاند. برای ارزیابی رابطهی میان نرخ ستارهزایی و فلزیت، شار هیدوژن-آلفا را بر روی نوار نشان داده شده در تصویر جمع زده و فلزیت را در طول این نوار اندازهگیری کردهاند. این نوار شامل سه تودهیستارهزا و بخشی از برآمدگی مرکزی کهکشان است. نمودار پایین تصویر کهکشان، فلزیت (خطوط سفید) را بهطور مستقیم با شار هیدوژن-آلفا (نقاط سبز) مقایسه میکند. این نمودار با تصویر رنگی همتراز شده است تا محل دقیق اندازهگیری شار هیدوژن-آلفا و فلزیت به درستی مشخص شود.
هر توده نهتنها نرخ ستارهزایی بالاتر و فلزیت کمتری دارد، بلکه ناحیهای که بیشترین چگالی نرخ ستارهزایی را نشان میدهد، کمترین فلزیت را نیز دارد. برآمدگی بخش مرکزی کهکشان در مجاورت یک تودهی ستارهزا قرار گرفته است. توزیع شار هیدوژن-آلفا نشان میدهد که بخش مرکزی مقدار زیادی شار هیدوژن-آلفا منتشر میکند و شار اندازهگیریشده از تودهی مجاور را تحتتاثیر قرار میدهد. با این حال، فلزیت در جایی که شار هیدوژن-آلفا در مرکز مقدار بیشینه را دارد، به کمینهی محلی نمیرسد، بلکه کمینهی محلی فلزیت با مکان تودهی ستارهزا ارتباط دارد. این موضوع نشان میدهد که اگرچه میان نرخ ستارهزایی و فلزیت یک ارتباط معکوس وجود دارد، اما سازوکار محرک ستارهزایی در برآمدگی مرکز کهکشان با سازوکار موجود در تودههای ستارهزا متفاوت است. همچنین مطالعهی جمعیتی از تودههای ستارهزا در کهکشانهایی با جهتگیری عمود به خط دید، روندی را نشان میدهد که در آن تودههای پرجرمتر، بیشتر به مرکز کهکشان نزدیک هستند؛ رفتاری که برای تودههایی که درون کهکشان تشکیل شده و به سمت برآمدگی مرکز کهکشان مهاجرت میکنند، انتظار میرود.
یافتههای این مقاله نشان میدهد که تودههای ستارهزا در این کهکشانها فلزیتی کمتر از نواحی پیرامون خود دارند. این امر میتواند بیانگر ورود گاز کمفلزیت به درون کهکشان باشد. ورود این گاز با فلزیت پایین میتواند نرخ ستارهزایی را افزایش دهد و همزمان ترکیبات شیمیایی محیط را رقیق کند. این پژوهش بر اهمیت درک پیچیدگی رابطهی بین ستارهزایی و غنیسازی شیمیایی در ظهرکیهانی اشاره میکند و قدمی است رو به جلو برای بررسی دیدگاههای تازه در مورد سازوکارهایی که شکلگیری کهکشانها را در انتقال به سرخهای بالاتر (عالم جوانتر) کنترل میکنند.
۱. Clump
۲. Ultraviolet
۳. (Hα) H-alpha
۴. Metallicity
۵. Spectral resolution
۶. Spatial resolution
۷. Resolved map
شکل بالای صفحه: کهکشان بیضوی NGC 5291 در مرکز تصویر.
منبع: Image credit: ESO
عنوان اصلی مقاله: Metal-Poor Star-Forming Clumps in Cosmic Noon Galaxies: Evidence for Gas Inflow and Chemical Dilution Using JWST NIRISS
نویسندگان: .Vicente Estrada-Carpenter et al
لینک اصلی مقاله: https://arxiv.org/pdf/2508.00985
گردآوری: فائزه اخلاقیمنش
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Author(s): Mark Buchanan
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Author(s): Nikhil Karthik
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Last Quarter Moon occurs at 1:12 A.M. EDT as sunset sweeps across the lunar nearside following the Full phase last week. Visible in the early-morning sky, the Moon lies just under 4° west of the Pleiades in Taurus some two hours before sunrise, rising in the east. (The Moon will continue to creep closer toContinue reading "The Sky Today on Saturday, August 16: The Moon reaches Last Quarter"
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President Donald Trump on Wednesday directed federal agencies to relax requirements for commercial launch and reentry licenses in a bid to jump-start competition in the U.S. space sector. The White House issued an executive order that calls for the elimination of environmental reviews and portions of Part 450 — a set of launch safety-related measures that tookContinue reading "Commercial spaceflight receives boost with Trump order"
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The basic unit of astronomical time measurement is the day, one rotation of Earth on its axis. But there is more than one way to define day. We can define it based on the Sun. One solar day is the time for the Sun to leave and return to your local meridian, the imaginary line that joins theContinue reading "Michael’s Miscellany: Sidereal Time"
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On Aug. 15, 1977, a narrowband radio signal was detected by the Big Ear Radio Telescope at Ohio State. The signal was powerful, lasted for 72 seconds, and was picked up on only 1 of 50 possible channels. It also showed a distinct pattern – starting low, growing, and then decreasing again — suggesting itContinue reading "Aug. 15, 1977: The Wow! Signal arrives"
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Dwarf planet 1 Ceres is stationary at 9 P.M. EDT, though to spot it you’ll have to get up early, as it’s only visible in the morning sky. Around 4 A.M. local daylight time, Ceres is just over 40° high in the southern sky. The main belt’s largest body is currently making its way throughContinue reading "The Sky Today on Friday, August 15: Ceres stands stationary"
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Sky This Week is brought to you in part by Celestron. Friday, August 15Dwarf planet 1 Ceres reaches its stationary point in Cetus the Whale at 9 P.M. EDT. Previously it was moving eastward relative to the background stars. Now it will begin to move westward, or retrograde. Ceres is only visible in the morningContinue reading "The Sky This Week from August 15 to 22: The Moon hangs with the morning planets"
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Author(s): David Ehrenstein
Experiments show that one of the standard electrode types for semiconductor-based quantum processors isn’t needed.
[Physics 18, s110] Published Thu Aug 14, 2025
If you missed my first 10 cool things about the Sun, you can read them here. Now you’re ready for 10 more. 11. Astronomers call the Sun’s visible surface the photosphere. Its thickness ranges from tens of miles to a few hundred miles. 12. The chromosphere is a layer about 1,200 miles thick that lies aboveContinue reading "Michael’s Miscellany: 10 More Cool Things About the Sun"
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NASA’s Explorer 6 satellite was launched Aug. 7, 1959, from Cape Canaveral, Florida. The spacecraft’s mission was to study Earth’s magnetic fields and radiation, as well as cosmic rays, geomagnetism, and micrometeorites. It also carried a photocell scanner, an instrument intended to photograph Earth’s cloud cover. A complication with one of its solar cells leftContinue reading "Aug. 14, 1959: Explorer 6 images Earth"
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Massimo Tamajo from Syracuse, Sicily, Italy A Perseid meteor streaks above Mount Etna in Italy in this Aug. 10 shot, taken just days before the peak of this year’s shower. The photographer used a Nikon mirrorless camera and 16mm lens at f/2.5 to take a 5-second exposure at ISO 640. Editor’s note: This credit andContinue reading "Perseid peak"
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The Moon reaches perigee at 1:59 P.M. EDT. Perigee is the point in the Moon’s orbit when it is closest to Earth; this afternoon, our satellite will sit 229,456 miles (369,274 km) away. Mercury is just starting to emerge from the Sun’s glare, presenting a challenging but reachable target. Now shining at magnitude 1, theContinue reading "The Sky Today on Thursday, August 14: Mercury reappears"
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Author(s): Paul Tschisgale
As large language models improve, the real challenge is not how to shield education from AI, but how to embrace AI as a cornerstone of future physics learning and teaching.
[Physics 18, 147] Published Wed Aug 13, 2025
Author(s): Rachel Berkowitz
Edge currents are observed in a magnetic topological insulator even when conventional theory says that they should not.
[Physics 18, s99] Published Wed Aug 13, 2025
After years of certification snags, the U.S. Space Force finally has its latest National Security Space Launch (NSSL) rocket. The newest branch of the U.S. armed forces on Tuesday launched United Launch Alliance’s (ULA) Vulcan Centaur to geosynchronous Earth orbit (GEO), marking the two-stage, heavy-lift launch vehicle’s debut national security mission. The NSSL program isContinue reading "ULA Vulcan makes successful Space Force debut"
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Using an AI algorithm, astronomers have discovered a new type of supernova likely resulting from the merger of a dying star and its black hole companion. In July 2023, the Zwicky Transient Facility discovered supernova SN 2023zkd, located 730 million light-years from Earth. Six months later, in January 2024, an artificial intelligence algorithm known asContinue reading "How AI helped uncover a new type of supernova"
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If you own a telescope with an aperture (the size of the lens or mirror) of 4 inches or more, there’s a wonderful object now high in the sky as darkness falls. It’s called the Ring Nebula, also known as M57 — the 57th object on French comet hunter Charles Messier’s famous list. He discovered the RingContinue reading "Michael’s Miscellany: Observe the Ring Nebula"
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Likely the best-known meteor shower of the year, the Perseids occur from late July through late August annually, typically peaking around Aug. 12-13. Meteor showers occur when the Earth passes through the debris field left behind as a comet orbits the Sun. In the case of the Perseids, that comet is Comet 109P/Swift-Tuttle, discovered inContinue reading "Aug. 13, 2011: Perseids from space"
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Chirag Upreti from New York City Venus and Jupiter met in a conjunction on the early morning of Tuesday, Aug. 12, captured in this shot above Croton Reservoir in New York State at nautical twilight. The photographer used a Sony mirrorless camera and lens at 24mm and f/5.6, taking a 1.5-second exposure at ISO 200.
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The Wild Duck Cluster, also cataloged as M11, flies high in Scutum this evening about two hours after sunset. Around 10 P.M. local daylight time, you can find it some 40° high in the south, some 3° west-southwest of the tail feathers of Aquila the Eagle. As an open cluster, M11’s stars are young, estimatedContinue reading "The Sky Today on Wednesday, August 13: The Wild Duck Cluster flies overhead"
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Author(s): Charles Day
New evidence supports the idea that solid oxygen switches under pressure to an exotic entangled state.
[Physics 18, s101] Published Tue Aug 12, 2025
Author(s): Gunnar Jeschke
A radio-frequency field can be resonant with nuclear spins in a sample even if its frequency does not match a spectroscopic transition—a result that could enable new forms of NMR spectroscopy.
[Physics 18, 145] Published Mon Aug 11, 2025
Using the Hubble Space Telescope, a team of astronomers has imaged an interstellar comet. This icy body was discovered by NASA’s Asteroid Terrestrial-impact Last Alert System (ATLAS) on July 1, 2025, when it was 420 million miles (676 million kilometers) from the Sun. ATLAS is an asteroid impact early warning system developed by the University of Hawai’i. AfterContinue reading "Hubble estimates the size of a comet from deep space"
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The latest astronaut crew conducting research on the International Space Station (ISS) returned to Earth on Saturday, marking the successful completion of NASA’s 10th Commercial Crew mission to the orbital laboratory. The crew of NASA and SpaceX’s Crew-10 mission splashed down off the coast of California on Friday morning, ending its nearly five-month mission. DuringContinue reading "NASA, SpaceX Crew-10 astronauts splash down"
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The Smithsonian Institution began collecting aeronautical artifacts in 1876, when it acquired 20 Chinese Imperial kites. By the end of World War I, a Section of Aeronatics had been established within the Division of Engineering, and Smithsonian Secretary Charles Walcott had mandated that the institution collect aircraft of historical significance. In particular, Charles Lindbergh’s SpiritContinue reading "Aug. 12, 1946: President Truman establishes the National Air Museum"
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Katelyn Beecroft from London, Ontario, Canada The dark nebula LDN 673 in Aquila is a dusty complex that blots out the light of background stars behind it — to this imager, visually resembling a Rorschach test. The image represents 18.8 hours of LRGB exposure with a 2.8-inch f/5.6 refractor.
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This morning is a busy one: Venus passes 0.9° south of Jupiter at 4 A.M. EDT, the two planets officially meeting in a conjunction as the Perseid meteor shower peaks. Step outside at 4 A.M. local time to catch the show. At that time, Venus and Jupiter are some 7° high in the east, locatedContinue reading "The Sky Today on Tuesday, August 12: Venus and Jupiter meet, the Perseid meter shower peaks"
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Mission highlight: USSF-106’s historic flight scheduled for Tuesday In last week’s edition, we mistakenly reported that the USSF-106 mission was scheduled for August 10. On August 5, United Launch Alliance announced the official launch date. The historic flight is now set to lift off on Tuesday, August 12, at 7:59 p.m. EDT from Cape Canaveral’sContinue reading "Historic ULA Vulcan launch slated for Tuesday, August 12"
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By reanalyzing archival data from the Atacama Large Millimeter/submillimeter Array (ALMA), scientists have discovered a giant, expanding bubble that is pushing against and distorting the protoplanetary disk surrounding a young star, WSB 52. You can see an animation of this event here: Stars and their planets form when large molecular clouds collapse in on themselves.Continue reading "Stellar jet pressures planet-forming disk"
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On June 28, the Yerkes Future Foundation (YFF), the nonprofit that has operated Yerkes Observatory since 2020, finalized the legal transfer of the site’s massive astronomical glass plate collection from the University of Chicago, according to an Aug. 7 press release. The foundation is now the official owner and steward of all 180,000 plates. BeforeContinue reading "Yerkes Observatory acquires historic glass plate collection"
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Will the Voyager 1 and Voyager 2 spacecraft be damaged when they finally pass through the Oort Cloud? Terry WilsonNorth Prince George, Virginia The Voyager 1 and Voyager 2 spacecraft were launched in 1977. Both passed Jupiter in 1979 and went on to Saturn a few years later, after which Voyager 2 also continued onContinue reading "Will Voyager 1 and Voyager 2 be damaged when they pass through the Oort Cloud?"
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In this episode, Astronomy magazine Editor Dave Eicher invites you to head out on the evenings of August 12th and 13th to watch for rapid streaks of light crossing the sky. Those streaks occur when Earth passes through a stream of particles left behind by a comet. Because they all appear to originate from the constellation Perseus,Continue reading "This Week in Astronomy with Dave Eicher: The Perseid meteor shower"
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After spending the 1850s at Harvard Observatory calculating orbits, Asaph Hall became an assistant at the U.S. Naval Observatory at Washington, D.C., in 1862. He was quickly promoted, and by 1873 had not only held several scientific discussions with Abraham Lincoln during the president’s visits to the observatory, but had also been put in chargeContinue reading "Aug. 11, 1877: Asaph Hall discovers Deimos"
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Ron Brecher The Bear Claw Nebula — also catalogued as Hartl-Dengl-Weinberger 2 and Sharpless 2–200 — is a planetary nebula in Cassiopeia filled with thin, dense filaments. The imager took 55⅔ hours of Hα/OIII/RGB data with a 14-inch f/11 scope.
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Asteroid 89 Julia reaches opposition at 5 A.M. EDT. Shining at magnitude 8.5, it’s easily reachable with binoculars or any telescope. This evening Julia rises around sunset and is visible all night, reaching its highest point around 1 A.M. local daylight time. A few hours earlier, though, around 11 P.M. local daylight time, Julia isContinue reading "The Sky Today on Monday, August 11: Asteroid Julia reaches opposition"
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On Aug. 10, 1990, the Magellan orbiter arrived at Venus and was inserted into orbit. Its goal was to map the surface of the planet, using radar to peer beneath the cloudy atmosphere. Launched aboard the space shuttle Atlantis in May 1989, Magellan was the first deep space probe launched from a shuttle. Budget constraintsContinue reading "Aug. 10, 1990: Magellan enters venusian orbit"
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Saturn’s two-toned moon Iapetus stands 1.5′ north of the ringed planet early this morning, shining around 11th magnitude. Spending much of its time far from Saturn, Iapetus rotates in lockstep with its orbit, so that its magnitude changes throughout its orbit as its brighter or darker hemisphere faces us. When it is north or southContinue reading "The Sky Today on Sunday, August 10: Iapetus stands north of Saturn"
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