Wd 1856 b

The object, called WD 1856 b, is roughly the same size as Jupiter, with possibly up to 14 times its mass. About every day and a half, it orbits a white dwarf, a star containing half the Sun’s mass in a space only slightly larger than Earth. TESS hunts for regular dips in starlight caused when planets pass in front of, or transit, their stars.

19 Feb 2021 ... V20 consider ideas other than CE to explain the orbit of. WD 1856 b, and favour planet migration from a larger or- bit by the von Zeipel-Lidov- ...WD 1856 b is thought to have formed at greater sep-arations, and to have migrated inward after the main sequence (MS). Although WD 1856 b is a cool (< 200K) object, its orbit resembles those of the ‘hot Jupiters’ that ac-company ˘1% of MS stars (e.g..Howard et al.2012).WD 1856 b is only considered a "likely" planet because it is in the range between the heaviest planet and the lightest brown dwarf, another type of stellar object. Spitzer analysis strongly points ...Jupiter-size WD 1856 b is nearly seven times larger than the white dwarf it orbits every day and a half. Astronomers discovered it using data from NASA’s Transiting ...WD 1856+534 is a white dwarf located in the constellation of Draco. At a distance of about 25 parsecs (80 ly) from Earth, it is the outer component of a visual triple star system consisting of an inner pair of red dwarf stars.Sep 16, 2020 · The planet, called WD 1856 b, is about seven times larger than the smaller white dwarf star and completes an orbit in just 34 hours. “WD 1856 b is a planet that shouldn’t be there,” said Kaye, an LSR member and regular visitor to HKU, who runs the Raemor Vista Observatory in southern Arizona, USA. A transmission spectrum of the planet candidate WD 1856+534 b and a lower limit to its mass. 2021 ALONSO R., RODRIGUEZ-GIL P., IZQUIERDO P., DEEG H., LODIEU N. et al. Astron. & Astrophys., 649, A131. paper arxiv. Under the Light of a Dead Star: Revealing the Atmospheric Composition of a White Dwarf Planet. 2021 MACDONALD R. et al.Dilansir dari Space, Kamis (17/9/2020), katai putih atau yang kerap disebut WD 1856 b merupakan sistem tiga bintang yang terletak sekitar 80 tahun cahaya dari bumi. Sementara itu ada kandidat exoplanet baru yang seukuran dengan Jupiter yang dinamai WD 1856 b. Ukuran planet extrasurya tersebut sekitar tujuh kali lebih besar WD 1856, …

The white dwarf WD 1856+534 is just 82 light years from Earth Advertisement Astronomers have discovered a planet the size of Jupiter closely orbiting the smouldering remains of a dead star, the first time that an intact exoplanet has been discovered travelling around a white dwarf, according to research published Wednesday.Dilansir dari Space, Kamis (17/9/2020), katai putih atau yang kerap disebut WD 1856 b merupakan sistem tiga bintang yang terletak sekitar 80 tahun cahaya dari bumi. Sementara itu ada kandidat exoplanet baru yang seukuran dengan Jupiter yang dinamai WD 1856 b. Ukuran planet extrasurya tersebut sekitar tujuh kali lebih besar WD 1856, …The satellite spotted WD 1856 b about 80 light-years away in the northern constellation Draco. It orbits a cool, quiet white dwarf that is roughly …In this artist's illustration, the Jupiter-sized planet WD 1856 b orbits the white dwarf every day and a half. ... LHS 475 b is relatively close, 41 light-years away, in the constellation Octans.These mass limits put WD 1856 b firmly within the planet category. Furthermore, our inferred values imply that WD 1856 b was born a typical gas giant. We further estimate the occurrence rate of Kozai-migrated planets around WDs to be O (10-3 - 10-4), suggesting that WD 1856 b is the only one in the TESS sample, but implying O(102) future ...After its initial discovery, the authors knew the rough size of the object (called WD 1856 b) because of how much light it blocked out, but did not know its mass. Jupiter-sized objects can be anything from a giant planet (which has a mass of 1/10th of Jupiter’s mass) to a low-mass star (which can weigh as much as 10 Jupiters).WD 1856 b can probably only have formed by this mechanism if the common-envelope phase began after much of the envelope's mass had already been lost. Given the difficulty in forming WD 1856 b ...

In this artist's illustration, the Jupiter-sized planet WD 1856 b orbits the white dwarf every day and a half. ... LHS 475 b is relatively close, 41 light-years away, in the constellation Octans.The discovery of a giant planet candidate orbiting the white dwarf WD 1856+534 with an orbital period of 1.4 d poses the questions of how the planet reached its current position. We here reconstruct the evolutionary history of the system assuming common envelope evolution as the main mechanism that brought the planet to its current position. We find that common envelope evolution can explain ...A Red Giant Branch Common-envelope Evolution Scenario for the Exoplanet WD 1856 b. Ariel Merlov1, Ealeal Bear1, and Noam Soker1,2. Published 2021 July 14 ...Nov 27, 2020 · WD 1856+534 b is a Jupiter-sized, cool giant planet candidate transiting the white dwarf WD 1856+534. Here, we report an optical transmission spectrum of WD 1856+534 b obtained from ten transits ... CAPTION: WD 1856 b, a potential planet the size of Jupiter, orbits its dim white dwarf star every 36 hours and is about seven times larger. Credit: NASA's Goddard Space Flight Center. The violent events leading up to the death of a star would likely drive away any planets. The newly discovered Jupiter-size object may have arrived long after the ...

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T 3 | Popertie WD 1856+534 b Parameter Value V (eccentric f) Orbital period a, P 1.4079405 ± 0.0000011 days 1.4079405 ± 0.0000011 days Time of transit, t t 0.0000034 BJD TDBWD 1856+534 b (or WD 1856 b for short) is the first known transiting planet candidate around a white dwarf star. WD 1856 b is about the size of Jupiter, has a mass less than about 12 Jupiter ...Sep 17, 2020 · The white dwarf WD 1856+534 is just 82 light years from Earth Advertisement Astronomers have discovered a planet the size of Jupiter closely orbiting the smouldering remains of a dead star, the first time that an intact exoplanet has been discovered travelling around a white dwarf, according to research published Wednesday. “WD 1856 b somehow got very close to its white dwarf and managed to stay in one piece,” said Andrew Vanderburg, an assistant professor of astronomy at the University of Wisconsin-Madison. “The white dwarf creation process destroys nearby planets, and anything that later gets too close is usually torn apart by the star’s immense …WD 1856 b در فاصله‌ی ۸۰ سال نوری از ما در صورت فلکی شمالی اژدها (Draco) قرار دارد و به دور یک کوتوله‌ی سفید و سرد می‌چرخد که تقریبا ۱۸۰۰۰ کیلومتر قطر دارد و ممکن است تا ۱۰ میلیارد سال سن داشته باشد.WD 1856+534 b (or WD 1856 b for short) is the first known transiting planet candidate around a white dwarf star. WD 1856 b is about the size of Jupiter, has a mass less than about 12 Jupiter masses, and orbits at a distance of about 2% of an astronomical unit. The formation and migration history of this object is still a mystery. Here, we present …

MOA-2010-BLG-477Lb is a observational confirmation that Jupiter and its system of moons will most probably survive the Sun’s death without migrating inwards too much, contrary to what happened ...Illustration of WD 1856 b and its host star. (NASA’s Goddard Space Flight Center) Astronomers have discovered a planet the size of Jupiter closely orbiting the smouldering remains of a dead star, the first time that an intact exoplanet has been discovered travelling around a white dwarf, according to research published Wednesday.As per the study authors, WD 1856 b is about 80 light-years away in the northern constellation Draco. It orbits a white dwarf around 18,000 kms across which may be up to 10 billion years old and is a distant member of a triple star system.16 Sep 2020 ... In this illustration, WD 1856 b, a potential Jupiter-size planet, orbits its much smaller host star, a dim white dwarf ...Pencarian tanda-tanda kehidupan di zona layak huni bintang WD 1856 itu nantinya akan diamati menggunakan teleskop luar angkasa NASA lainnya, yakni James Webb, yang akan diluncurkan pada Oktober 2021. ”WD 1856 b menunjukkan bahwa planet dapat bertahan dari proses chaos pembentukan bintang katai putih. Dalam kondisi yang …These mass limits put WD 1856 b firmly within the planet category. Furthermore, our inferred values imply that WD 1856 b was born a typical gas giant. We further estimate the occurrence rate of Kozai-migrated planets around WDs to be O (10-3 - 10-4), suggesting that WD 1856 b is the only one in the TESS sample, but implying O(102) future ... WD 1856 actually has a larger mass than WD 1856 b: the NASA overview page gives 0.518 solar masses (543 Jupiter masses) for the white dwarf, while the planet has less than 13.8 Jupiter masses. The white dwarf has a smaller radius than the planet as it is much denser.16 Sep 2020 ... WD 1856 b. In this illustration, WD 1856 b, a potential Jupiter-size planet, orbits its dim white dwarf star every day and a half. (NASA's ...In this artist's illustration, the Jupiter-sized planet WD 1856 b orbits the white dwarf every day and a half. NASA's Goddard Space Flight Ce. This illustration shows a carbon-rich planet with ...

WD 1856 b, and favour planet migration from a larger or-bit by the von Zeipel-Lidov-Kozai (ZLK) effect (von Zeipel 1910;Lidov1962;Kozai1962)intandemwithtidalfriction (Wu&Murray2003;Fabrycky&Tremaine2007).Theycon-cludethatWD1856b’sM-dwarfcompanionsG229-20A/B

Gaia DR2 2146576589564898688 b. Description. Whereas some white dwarfs show evidence for rocky material floating in their atmospheres, WD 1856+534 b is the first giant planet candidate transiting a white dwarf. During a star's red giant phase, any close-orbiting planets will be engulfed by the star, but more distant planets can survive this ...WD 1856 b has a low mass and long orbital period compared to other post common envelope binaries (Vanderburg et al. 2020) which makes it challenging to explain its formation by this mechanism, but ...WD 1856 b is a gas giant planet that most likely survived being engulfed by it’s star during it’s red giant phase. The idea is based on two studies done by F. Lagos et. al. 2020 and L. Chamandy et.al. 2020. In both studies, the scientists found that massive gas giant planets are more robust than previously thought.satellites: individual: WD 1856+534 b 1. INTRODUCTION Vanderburg et al.(2020) report the detection of a planet orbiting a white dwarf (WD 1856+534; TIC 267574918) with a period of P orb = 1:4 days andThe discovery of a giant planet candidate orbiting the white dwarf WD 1856+534 with an orbital period of 1.4 d poses the questions of how the planet reached its current position.Last year, a team found an intact Jupiter-like planet called WD 1856 b orbiting a white dwarf, reports Becky Ferreira for the New York Times. Unlike the planet described in the recent Nature study ...WD 1856+534 b is a gas giant exoplanet that orbits a K-type star. Its mass is 13.8 Jupiters, it takes 1.4 days to complete one orbit of its star, and is 0.0204 AU from its star. Its discovery was announced in 2020.satellites: individual: WD 1856+534 b 1. INTRODUCTION Vanderburg et al.(2020) report the detection of a planet orbiting a white dwarf (WD 1856+534; TIC 267574918) with a period of P orb = 1:4 days and

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"The satellite spotted WD 1856 b about 80 light-years away in the northern constellation Draco. It orbits a cool, quiet white dwarf that is roughly 11,000 miles (18,000 kilometres) across, maybe up to 10 billion years old, and is a distant member of a triple star system," Nasa's statement further read.The Jovian-sized object WD 1856 b transits a white dwarf (WD) in a compact 1.4 day orbit. Unlikely to have endured stellar evolution in its current orbit, WD 1856 b is thought to have migrated from much wider separations. Because the WD is old, and a member of a well-characterized hierarchical multiple, the well-known Kozai mechanism provides an effective migration channel for WD 1856 b. The ... In this artist's illustration, the Jupiter-sized planet WD 1856 b orbits the white dwarf every day and a half. NASA's Goddard Space Flight Ce This illustration shows a carbon-rich planet with ...Vacant land located at 856 Burdsal Pkwy, Indianapolis, IN 46208. View sales history, tax history, home value estimates, and overhead views. APN 49-06-26-150-039.000-101.WD 1856+534 b is a Jupiter-sized, cool giant planet candidate transiting the white dwarf WD 1856+534. Here, we report an optical transmission spectrum of WD 1856+534 b obtained from ten transits using the Gemini Multi-Object Spectrograph. This system is challenging to observe due to the faintness of the host star and the short transit duration.Canada. Deviant for 9 years. Bari Marcus Anthony. He / Him. Follow me on. Badges. My Bio. A writer and screenwriter under James Montana Films and Canadian Northwest Publishing Company. Raised in the Okanagan Valley, British Columbia, Canada, I continue writing and applying my art skills with Okanagan College in Kelowna, BC , …exoplanets.eu: WD 1856+534 b Search the TESS EB Catalog · TESS Web Visibility Tool TOIs 1 CTOIs 0 Planet Params 2 Stellar Params 2 Stellar Companions 0 Magnitudes 10 Imaging 0 Spectroscopy 0 Time Series 1 Files 3 Observing Notes 1Art Gallery. Here’s another exoplanet I created with my imagination of a real exoplanet known as the Giant Purple Jupiter, (WD 1856 b) by NASA. The planet is about seven times larger than the white dwarf star you see, that’s orbiting every 34 hours. Incredibly, according to NASA, it’s actually purple. You can also join.Jupiter-size WD 1856 b is nearly seven times larger than the white dwarf it orbits every day and a half. Astronomers discovered it using data from NASA’s Transiting ...WD-40 News: This is the News-site for the company WD-40 on Markets Insider Indices Commodities Currencies StocksMay 2, 2023 · In this artist's illustration, the Jupiter-sized planet WD 1856 b orbits the white dwarf every day and a half. NASA's Goddard Space Flight Ce This illustration shows a carbon-rich planet with ... The discovery of a giant planet candidate orbiting the white dwarf WD 1856+534 with an orbital period of 1.4 d poses the questions of how the planet reached its current position. ….

Draft version July 1, 2021 Typeset using LATEX twocolumn style in AASTeX63 A red giant branch common envelope evolution scenario for the exoplanet WD 1856 b Ariel Merlov, 1Ealeal Bear, andNoam Soker1,2 1Department of Physics, Technion { Israel Institute of Technology, Haifa 3200003, Israel; [email protected]; [email protected] 1856 b، سیاره ای در حد مشتری به دور ستاره میزبان که کوتوله سفید است گردش می‌کند. نکته جالب تر آنکه سطح سیاره WD 1856 b بسیار خنک اعلام شده و به قول Xu «جزو خنک ترین سیاراتی است که تاکنون کشف شده است.»Washington: Scientists have, for the first time, discovered a Jupiter-sized planet orbiting a white dwarf or a dead star located about 80 light years away. The finding, published in the journal Nature, shows the likely presence of the planet, named WD 1856 b, orbiting the smaller star remnant every 34 hours. "This planet is roughly the size of …A transmission spectrum of the planet candidate WD 1856+534 b and a lower limit to its mass. 2021 ALONSO R., RODRIGUEZ-GIL P., IZQUIERDO P., DEEG H., LODIEU N. et al. Astron. & Astrophys., 649, A131. paper arxiv. Under the Light of a Dead Star: Revealing the Atmospheric Composition of a White Dwarf Planet. 2021 MACDONALD R. et al.The planet, WD 1856 b, is around the size of Jupiter, making it seven times the size of the white dwarf WD 1856+534, which it orbits around. A white dwarf is the remnant left behind after a star ...WD 1856 b در فاصله‌ی ۸۰ سال نوری از ما در صورت فلکی شمالی اژدها (Draco) قرار دارد و به دور یک کوتوله‌ی سفید و سرد می‌چرخد که تقریبا ۱۸۰۰۰ کیلومتر قطر دارد و ممکن است تا ۱۰ میلیارد سال سن داشته باشد.The Jupiter-sized object, called WD 1856 b, is about seven times larger than the white dwarf. It circles this stellar cinder every 34 hours, over 60 times faster than Mercury orbits our sun. It orbits a cool, quiet white dwarf called WD 1856+534, about 80 light-years away in the northern constellation Draco. The host star is roughly 11,300 ..."WD 1856 b somehow got very close to its white dwarf and managed to stay in one piece," said Andrew Vanderburg, an assistant professor of astronomy at the University of Wisconsin-Madison. "The white dwarf creation process destroys nearby planets, and anything that later gets too close is usually torn apart by the star's immense gravity.The Jovian-sized object WD 1856 b transits a white dwarf (WD) in a compact 1.4 day orbit. Unlikely to have endured stellar evolution in its current orbit, WD 1856 b is thought to have migrated from much wider separations. Because the WD is old, and a member of a well-characterized hierarchical multiple, the well-known Kozai mechanism provides ...WD 1856 b to have been ∼2.5au, and its mass to be ;0.7–3M J. These mass limits put WD 1856 b firmly within the planet category. Furthermore, our inferred values imply that WD 1856 b was born a typical gas giant. We further estimate the occurrence rate of Kozai-migrated planets around WDs to be ()10 10--34- , suggesting that Wd 1856 b, WD 1856+534 b is a Jupiter-sized, cool giant planet candidate transiting the white dwarf WD 1856+534 . Here, we report an optical transmission spectrum of WD 1856+534 b obtained from ten transits ..., When you’re planning a road trip, there are several options for mapping out your route. One option is free Rand McNally directions available online. Rand McNally is a familiar name in the map world with history dating back to 1856., The Jovian-sized object WD 1856 b transits a white dwarf (WD) in a compact 1.4 day orbit. Unlikely to have endured stellar evolution in its current orbit, WD 1856 b is thought to have migrated from much wider separations. Because the WD is old, and a member of a well-characterized hierarchical multiple, the well-known Kozai mechanism provides an effective migration channel for WD 1856 b. The ... , NASA, WD 1856+534 is a white dwarf located in the constellation of Draco. At a distance of about 25 parsecs (80 ly) from Earth, it is the outer component of a visual triple star system consisting of an inner pair of red dwarf stars. , NASA , WD 1856+534 This reference contains discussion regarding the stellar multiplicity of this system. (Vanderburg et al. 2020) WD 1856+534 Stellar age value/uncertainties estimated from range 5.85-10 Gyr. (Vanderburg et al. 2020) WD 1856+534 b Planet parameters drawn from Table 3, circular model in ref. (Vanderburg et al. 2020), Pages in category "1856 in Washington, D.C." The following 2 pages are in this category, out of 2 total. This list may not reflect recent changes. C. Caning of Charles Sumner; S. 1856 State of the Union Address This page was last edited on 23 November 2022, at 08:20 (UTC). Text is available under the Creative ..., arxiv Enhanced Lidov-Kozai migration and the formation of the transiting giant planet WD1856+534b 2021 O'CONNOR Ch., LIU B. & LAI D. MNRAS, 501, 507 paper arxiv WD 1856 b: a close giant planet around a white dwarf that could have survived a common-envelope phase 2021 LAGOS F., SCHREIBER M., ZOROTOVIC M., GÄNSICKE B., RONCO M. & HAMERS A., Sep 17, 2020 · “WD 1856 b somehow got very close to its white dwarf and managed to stay in one piece,” said Andrew Vanderburg, an assistant professor of astronomy at the University of Wisconsin-Madison. “The white dwarf creation process destroys nearby planets, and anything that later gets too close is usually torn apart by the star’s immense gravity. , WD 1856 b is the remnant of a planet that is orbiting a stellar corpse known as a white dwarf—what was once a sun-like star but now a relic not much larger than the size of Earth. Before the host star collapsed and became a white dwarf, its outer gaseous layer expanded and engulfed WD 1856 b but did not destroy it., Sep 16, 2020 · The Jupiter-size object, called WD 1856 b, is about seven times as large as the white dwarf named WD 1856+534. It circles this stellar cinder every 34 hours, more than 60 times as fast as Mercury orbits our sun. “WD 1856 b somehow got very close to its white dwarf and managed to stay in one piece,” said Vanderburg, who was a NASA Sagan ... , The discovery of a giant planet candidate orbiting the white dwarf WD 1856+534 with an orbital period of 1.4 d poses the questions of how the planet reached its current position. We here reconstruct the evolutionary history of the system assuming common envelope evolution as the main mechanism that brought the planet to its current position. We find that common envelope evolution can explain ..., If WD 1856 b were on such an orbit, the orbital energy would have rapidly dissipated, owing to tides raised on the planet by the white dwarf 26,27. The final state of minimum energy would be a ..., The object, called WD 1856 b, is about seven times larger than the white dwarf. Based on the object’s size, astronomers think it’s a giant gaseous planet, which future observations and research may confirm. They also estimate it’s no more than 14 times Jupiter’s mass., If WD 1856 b was a brown dwarf or low-mass star, it would emit its own infrared glow. This means Spitzer would record a brighter transit than it would if the object were a planet, which would block rather than emit light. When the researchers compared the Spitzer data to visible light transit observations taken with the Gran Telescopio Canarias ..., WD 1856 b. Gas giant WD 1856 b is a bit of a mystery, as it orbits the leftovers of a star that is seven times smaller than the exoplanet itself., Given the temperature of WD 1856+534 (K, Vanderburg et al. 2020), we use the 5000 K WD HZ terrestrial planet model from Kozakis et al. for our analysis. We note that WD hosts display largely featureless spectra 7 (Saumon et al. 2014), similar to blackbodies, below 5000 K (Kepler et al. 2016)., The white dwarf in question, called WD 1856, is part of a three-star system that lies about 80 light-years from Earth. The newly detected, Jupiter-size exoplanet candidate, WD 1856 b, is..., Sep 28, 2020 · Planet WD 1856+534 b was first spotted by the NASA’s Transiting Exoplanet Survey Satellite (TESS) and confirmed with a series of observations from ground-based telescopes. The results showed the light from a white dwarf being periodically dimmed by a staggering 56% for brief 8 minutes. For comparison, one of the easiest exoplanet types to ... , The discovery of the first transiting giant planet orbiting a WD, WD 1856+534, showed that planetary-mass objects can survive close-in orbits around WDs. The large radius …, WD 1856+534 b (or WD 1856 b for short) is the first known transiting planet candidate around a white dwarf star. WD 1856 b is about the size of Jupiter, has a mass less than about 12 Jupiter masses, and orbits at a distance of about 2 per cent of an astronomical unit. The formation and migration history of this object is still a mystery., Sep 11, 2019 · As a result, one of WASP-121 b's hemispheres always faces the star, heating it to temperatures of up to 3000 degrees Celsius. ... In this artist's illustration, the Jupiter-sized planet WD 1856 b ... , Sep 16, 2020 · Given the temperature of WD 1856+534 (K, Vanderburg et al. 2020), we use the 5000 K WD HZ terrestrial planet model from Kozakis et al. for our analysis. We note that WD hosts display largely featureless spectra 7 (Saumon et al. 2014), similar to blackbodies, below 5000 K (Kepler et al. 2016). , As a result, one of WASP-121 b's hemispheres always faces the star, heating it to temperatures of up to 3000 degrees Celsius. ... In this artist's illustration, the Jupiter-sized planet WD 1856 b ..., Sep 17, 2020 · The white dwarf WD 1856+534 is just 82 light years from Earth Advertisement Astronomers have discovered a planet the size of Jupiter closely orbiting the smouldering remains of a dead star, the first time that an intact exoplanet has been discovered travelling around a white dwarf, according to research published Wednesday. , WD 1856 b is thought to have formed at greater sep-arations, and to have migrated inward after the main sequence (MS). Although WD 1856 b is a cool (< 200K) object, its orbit resembles those of the ‘hot Jupiters’ that ac-company ˘1% of MS stars (e.g..Howard et …, The Jovian-sized object WD~1856~b transits a white dwarf (WD) in a compact $1.4$-day orbit. Unlikely to have endured stellar evolution in its current orbit, WD~1856~b is thought to have migrated from much wider separations. Because the WD is old, and a member of a well-characterized hierarchical multiple, the well-known Kozai mechanism provides an effective migration channel for WD~1856~b ..., When you’re planning a road trip, there are several options for mapping out your route. One option is free Rand McNally directions available online. Rand McNally is a familiar name in the map world with history dating back to 1856., WD 1856+534 b is a Jupiter-sized, cool giant planet candidate transiting the white dwarf WD 1856+534. Here, we report an optical transmission spectrum of WD 1856+534 b obtained from ten transits using the Gemini Multi-Object Spectrograph. This system is challenging to observe due to the faintness of the host star and the short transit duration., The Jovian-sized object WD 1856 b transits a white dwarf (WD) in a compact 1.4 day orbit. Unlikely to have endured stellar evolution in its current orbit, WD 1856 b is thought to have migrated from much wider separations. Because the WD is old, and a member of a well-characterized hierarchical multiple, the well-known Kozai mechanism …, Car window paint, sometimes referred to as window chalk, can be removed by using soap, water and, if necessary, WD-40 or acetone. People use window chalk to write messages on and otherwise decorate their car windows; writing “Just Married” ..., 最新探测到的木星尺寸地外行星，行星WD1856 b，大约比白矮星大七倍，每34小时快速公转一周。. The white dwarf in question, called WD 1856, is part of a three-star system that lies about 80 light-years from Earth. The newly detected, Jupiter-size exoplanet candidate, WD 1856 b, is about seven times larger than the ...