Articles tagged with Neptune
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A new study by the University of Zurich suggests that Uranus and Neptune may be more rocky than icy, challenging their classification as ice giants. The researchers developed a unique simulation process to model the planets' interiors, which found that the two planets could have either water-rich or rock-rich compositions.
Researchers analyzed Trans-Neptunian Objects using the James Webb Space Telescope, finding two distinct groups with varying surface ice methanol presence. The discovery sheds light on the formation and evolution of these distant icy worlds, revealing insights into the solar system's origins and potentially habitable exoplanets.
Hubble's OPAL program has observed the four giant outer planets since 2018, providing long-term baseline data on their atmospheric changes. The observations have led to remarkable discoveries, including the measurement of Jupiter's wind speeds and Saturn's ring system colors.
Researchers argue that the planets' unique magnetic fields can be explained by immiscible layers of water and hydrocarbons. Computer simulations show that a combination of water, methane, and ammonia separates into two distinct layers under extreme temperatures and pressures.
The NASA TESS-Keck Survey catalog features 126 exotic planets with detailed measurements allowing for comparisons with our solar system. Several planets stand out as touchstones for deepening astronomers' understanding of planetary formation and evolution.
A team of UCF scientists used the James Webb Space Telescope to analyze the elemental composition of a binary duo in the Kuiper Belt, revealing clues about Neptune's formation. The study provides valuable insights into the dynamical history of Neptune and its neighboring objects.
Astronomers have discovered a small, cold exoplanet with an orbital period of 146 days, providing insight into planetary formation and evolution. The planet, HD88986b, is about twice the size of Earth and orbits a star similar to the Sun.
Researchers used data from Hubble Space Telescope to determine the true colors of Neptune and Uranus, revealing they are a similar shade of greenish blue. The main difference is that Neptune has a slight hint of additional blue due to a thinner haze layer on that planet.
New studies show that giant gas planets in nearby star systems can prevent life on smaller, rocky planet neighbors by kicking them out of orbit and wreaking havoc on their climates. Researchers found that four giant planets in the HD 141399 system are likely to destroy the chances for life on Earth-like planets.
Astronomers have discovered a surprising link between Neptune's cloud abundance and the 11-year solar cycle. The study found that two years after the solar cycle's peak, clouds on Neptune increase in number. The team believes UV radiation from the Sun may be triggering photochemical reactions that produce clouds.
A team of astronomers discovered a population of reddish Neptunian asteroids, which are thought to have formed beyond the transition boundary between neutral-colored and redder objects. The red coloration suggests these asteroids contain more volatile ices, providing insight into the early Solar System's conditions.
Researchers used density functional theory to investigate the mechanical properties of superionic ice XVIII, which is thought to make up a large part of Neptune and Uranus. The study found that dislocations in the crystal lattice produce shear, leading to macroscopic deformations and potentially influencing the planets' magnetic fields.
A team from UNIGE has observed a sample of planets at the edge of the Hot Neptune Desert to understand its creation. They found that most of these planets have an orbit misaligned with the stellar equator, indicating disruptive migration processes.
Researchers found that oxygen makes diamond formation more likely, allowing for a wider range of conditions and planets. This discovery could lead to new methods of fabricating nanodiamonds with various applications.
Researchers at Helmholtz-Zentrum Dresden-Rossendorf have successfully created nanodiamonds out of PET plastic using powerful laser flashes. This breakthrough method opens up new possibilities for producing these minuscule diamonds, which are needed for highly-sensitive quantum sensors and medical contrast agents.
Researchers discovered a Neptune-sized planet around a bright blue star, shedding light on the dearth of Hot Neptunes. The planet's proximity to its star makes it susceptible to stripping of its gas, but it may survive for a billion years.
The Gemini North telescope has helped astronomers understand why Uranus and Neptune have different colors. Excess haze on Uranus builds up in its stagnant atmosphere, making it appear lighter than Neptune's. The team developed a single atmospheric model that matches observations of both planets.
A new study by University of Leicester researchers reveals Neptune's atmospheric temperatures have dropped by roughly 8 degrees Celsius between 2003 and 2018, with unexpected stratospheric warming at the south pole. The cause of these changes is currently unknown, but may be related to seasonal variations in atmospheric chemistry.
Dr Henrik Melin, a researcher at the University of Leicester, has been awarded the third-ever Webb Fellowship to study the atmospheres of giant planets using the James Webb Space Telescope. He aims to understand the mechanisms driving powerful aurorae on these planets and address the 'energy crisis' in their upper atmospheres.
Researchers have created superionic ice phases XVIII and XX by subjecting water to record-breaking pressures and temperatures. The study provides insights into the formation of these conductive forms of ice and their potential role in explaining the mysterious magnetic fields of Uranus and Neptune.
New research reveals that a layer of 'hot', electrically conductive ice could be responsible for generating the magnetic fields of ice giant planets. The study found two forms of superionic ice, one of which may exist in the interiors of Uranus and Neptune.
Researchers propose that giant hailstones called mushballs carry ammonia deep into the atmospheres of ice giants Uranus and Neptune, hiding it from detection. This process could explain the unexpected lack of ammonia in their atmospheres compared to other planets.
A new paper discusses how smoking may affect risk for COVID-19 and proposes areas of research needed to better understand the link. Studies have shown that current smokers with COVID-19 have twice the risk of dying in the hospital as nonsmokers, highlighting the need for rigorous study design to clarify this relationship.
The team discovered a planetoid dubbed 'Farfarout,' located 132 astronomical units (au) from the Sun, making it the most distant object ever observed. It has a highly elongated orbit that takes approximately 1,000 years to complete, crossing Neptune's orbit every time.
Researchers found high levels of plastic debris trapped in seagrass litter and fibers, suggesting that seagrass meadows can facilitate marine plastic removal from the sea. The study estimates that Mediterranean seagrass meadows may trap up to 867 million plastic items each year.
Astronomers observing a dark vortex on Neptune noticed it change direction by August 2020, doubling back to the north. A smaller dark spot, possibly a fragment of the giant vortex, was also spotted near its larger cousin in January this year.
Researchers measured the spectrum of a rare hot Neptune exoplanet, revealing evidence of molecular absorption in its atmosphere. This detection provides clues on the origin of the planet and how it managed to hold onto its atmosphere.
Researchers from the University of Kansas have characterized the atmospheric makeup of LTT 9779b, a highly unusual hot Neptune discovered by NASA's TESS mission. The study reveals the planet's temperature and composition, shedding light on the formation of exoplanet atmospheres.
Astronomers at the University of Warwick have discovered a Neptune-sized gas giant with an exposed core, allowing for the first time to peer inside a planet. The core is believed to be 'failed' or stripped of its gaseous atmosphere, offering insights into planet formation and composition.
A study by Brazilian researchers suggests the Solar System took shape in its current form between 10-60 million years after its formation. The model, supported by São Paulo Research Foundation - FAPESP, reveals a chaotic phase that placed objects in their current orbits within the first 100 million years.
Astronomers have discovered a rare opportunity to study the evolution of a planetary system, with the DS Tuc binary system providing insights into how planets form without being heavily impacted by external forces. The findings suggest that the planet DS Tuc Ab formed through relatively calm processes.
Astronomers discover unique infrared signature on Triton, suggesting a mix of carbon monoxide and nitrogen ices. This finding sheds light on conditions on other distant, icy worlds and could provide insights into the origins of life.
Scientists will study Uranus and Neptune's poorly understood regions with greater accuracy using a new, improved net flux radiometer. The instrument, developed for NASA's Planetary Concepts for the Advancement of Solar System Observations program, features thermopile sensors and seven infrared channels to measure heat.
Scientists from HZDR drove shock waves through plastics to simulate planetary conditions and observed crystalline structures at extreme pressures. The discovery may require revised models of Uranus and Neptune's interiors, suggesting less free hydrogen than previously thought.
A team of planetary scientists used Hubble images to track the growth of a new Great Dark Spot on Neptune, finding that dark spots originate deeper in the planet's atmosphere than previously thought. The study also revealed that these storms occur with a frequency of every four to six years and last up to six years.
Astronomers found a tiny moon, Hippocamp, around Neptune that shouldn't exist due to gravitational clearance by Proteus. The moon is thought to be a chipped-off piece from Proteus resulting from a comet collision, measuring 20 miles across.
The Hubble Space Telescope has uncovered new insights into the weather patterns of Uranus and Neptune, revealing dynamic atmospheres with mysterious dark storms. The observations suggest that these storms form in a similar way to Jupiter's Great Red Spot and are driven by seasonal changes.
Researchers discovered two warm Neptunes at the edge of the 'hot Neptune desert' losing their atmospheres at a rapid pace. This supports the idea that hot Neptunes transform into super-Earths, which are more numerous than previously thought. The study used NASA's Hubble Space Telescope to observe the evaporation of these planets.
Astronomers use Hubble to detect a second 'very warm' Neptune losing its atmosphere at an unprecedented rate, shedding light on the mysterious hot-Neptune deficit. The planet's evaporation may be linked to its star's intense radiation and age.
Researchers have recreated superionic water, a state where oxygen remains fixed while protons flow freely, exhibiting properties of both solid and liquid. This discovery could lead to new materials with unique practical applications and provide insights into the physical properties of planets in our solar system.
Scientists at Helmholtz-Zentrum Dresden-Rossendorf simulated the conditions inside Neptune and found diamonds forming in real time using an ultra-strong X-ray laser. The study provides insights into the planet's chemical makeup and has potential applications for electronic instruments, medical procedures, and industrial production.
Researchers at the University of Edinburgh used computer simulations to predict chemical compounds in Neptune's mantle, finding ammonia hemihydrate as a likely component. The discovery sheds light on the extreme conditions and chemistry of ice giants, influencing future studies.
Researchers discovered a massive storm system near Neptune's equator, about 1/3 the size of Neptune's radius, with bright clouds forming at low latitudes. This unexpected feature was observed during twilight and is thought to be linked to high-pressure dark vortex systems.
Researchers have successfully removed the neutralizer in plasma propulsion systems, enabling charge-neutral beams to be generated. This breakthrough is a significant improvement over traditional electric propulsion concepts.
A team of international researchers has uncovered the primitive atmosphere surrounding a distant exoplanet called HAT-P-26b, also known as Warm Neptune. The study found that the planet's atmosphere is composed almost entirely of hydrogen and helium with no clouds present.
A new study reveals that HAT-P-26b, a Neptune-sized planet, has a hydrogen and helium-dominated atmosphere with a strong water signature. The discovery challenges the long-held assumption that planets like Neptune formed in a region of icy debris, instead suggesting alternative formation mechanisms.
A NASA study using Hubble and Spitzer space telescopes reveals a primitive atmosphere around HAT-P-26b, composed mainly of hydrogen and helium. The planet's water signature suggests it formed closer to its star or later in the planetary system than similar planets.
A study published in Nature Astronomy found that blue binaries in the Kuiper Belt formed closer to the Sun and were shaped by Neptune's gravitational nudges. The research suggests a smooth and calm migration of Neptune from 20 AU to its current location at 30 AU, allowing fragile binaries to be pushed out to their current orbits.
Research from the University of Warwick suggests that Planet Nine's existence could lead to the elimination of a giant planet and its ejection into interstellar space. The hypothetical planet's presence could cause a 'pinball' effect, hurling planets out of the solar system as the sun dies in around seven billion years.
New calculations suggest the six extreme trans-Neptunian objects, initially used to propose Planet Nine, would have unstable orbits if it exists. The orbits of these objects could escape the Solar System in less than 1.5 billion years.
Researchers propose that gravitational forces alter ETNO orbits, indicating the presence of unseen planets. Calculations reveal a possible second planet with characteristics diverging from current theories on solar system formation.
The newly discovered moon, S/2004 N 1, is estimated to be 12 miles across and is the smallest known moon orbiting Neptune. It was found using archival images taken by Hubble from 2004 to 2009 and noticed a white dot between the orbits of Neptunian moons Larissa and Proteus.
Astronomers found two planets smaller than Neptune orbiting Sun-like stars in the dense star cluster NGC 6811. The discovery shows that planets can form and survive even in crowded clusters.
A team of scientists has determined that the atmospheric layer on Uranus and Neptune extends only about 1000 km in depth, a significant finding that challenges current understanding of these planets' weather systems. This discovery was made possible by analyzing gravitational field data using novel methods.
Researchers identified a new molecular pathway involved in the growth of tiny air sacs called alveoli crucial for breathing. HGF treatment showed a 17% improvement in air sac size and lung structure, suggesting a potential approach to regrow destroyed air sacs in people with emphysema.
Researchers at Johns Hopkins University discovered that losartan, a blood pressure medication, reduces lung disease caused by cigarette smoke exposure. The study suggests other TGF-beta targeted therapeutics might be viable candidates for COPD treatment.
Voyager 1 has sailed to the edge of the solar system and is expected to punch its way into interstellar space in the coming months or years. The spacecraft was launched in 1977 and completed the Grand Tour of the Solar System, making numerous groundbreaking discoveries about the outer planets and their moons.
The Hubble Space Telescope has taken anniversary pictures of Neptune, revealing high-altitude clouds in the northern and southern hemispheres composed of methane ice crystals. The images also show that cloud activity is shifting to the northern hemisphere, with seasons lasting about 40 years.
A University of Arizona planetary scientist has determined Neptune's rotation with high accuracy by tracking atmospheric features in its atmosphere. The discovery improves upon previous measurements and provides a better understanding of the planet's fundamental properties.
Researchers found binary systems in the Kuiper Belt would be destroyed by Neptune's interaction, contradicting previous assumptions. The study suggests the region formed near its present location and remained undisturbed over the age of the solar system.