Tag Archive for 'Star'

An artist’s conception of the HR 858 planetary system. Image credit: Sci-News.com.

Two Planets in HD 3167 System are on Perpendicular Orbits, Astronomers Say

Nov 2, 2021 by Natali Anderson

The super-Earth HD 3167b is close to orbiting within the stellar equatorial plane, while the mini-Neptune HD 3167c orbits above the poles of the host star,...

An artist’s impression of the sub-Neptune TOI-2285b and its parent star. Image credit: Sci-News.com.

Temperate Sub-Neptune Found Orbiting Nearby Red Dwarf

Nov 1, 2021 by Natali Anderson

Using data from NASA’s Transiting Exoplanet Survey Satellite (TESS) and several ground-based telescopes, astronomers have discovered and confirmed a...

An artist’s impression of the hot-Jupiter exoplanet HAT-P-68b and its parent star HAT-P-68 (also known as GSC 1925-01046 and 2MASS 07535598+2356176), a K5-type dwarf star with a mass of 0.68 solar masses and a radius of 0.67 solar radii. Image credit: Sci-News.com.

Astronomers Measure Amount of Carbon and Oxygen in Hot Jupiter’s Atmosphere

Oct 29, 2021 by News Staff

Using the Immersion GRating INfrared Spectrometer (IGRINS) at the Gemini South Observatory on Cerro Pachon, Chile, astronomers have measured carbon-to-hydrogen...

This Hubble image shows the carbon star CW Leonis. The image incorporates observations from 2011 and 2016 by Hubble’s Wide Field Camera 3 (WFC3). The star is brightest in the red filters, R and I, and therefore the simmering orange color pervading the center of the image well represents the real color of the star. Image credit: NASA / ESA / Hubble / T. Ueta / H. Kim.

Hubble Observes Red Giant Star CW Leonis

Oct 29, 2021 by News Staff

CW Leonis, which is located 400 light-years away in the constellation of Leo, is a carbon star — a luminous type of red giant star with a carbon-rich...

An artist’s impression of the binary system MAXI J1820+070. Image credit: John Paice.

Warped Accretion Disk Spotted around Stellar-Mass Black Hole

Oct 28, 2021 by News Staff

Variations in the brightness of light seen from around a stellar-mass black hole in the binary system MAXI J1820+070 were caused by a huge warp in its...

This image from NASA’s Spitzer Space Telescope shows a Godzilla-like nebula in the constellation of Sagittarius. Four colors (blue, cyan, green, and red) represent different wavelengths of infrared light: blue and cyan represent wavelengths primarily emitted by stars; dust and organic molecules called hydrocarbons appear green; and warm dust that’s been heated by stars or supernovae appears red. Image credit: NASA/ Spitzer / JPL-Caltech.

Spitzer Spots ‘Godzilla-Like Nebula’

Oct 27, 2021 by News Staff

NASA has released an incredibly beautiful image of a nebula, a cloud of gas and dust captured by the agency’s Spitzer Space Telescope. This image from...

An artist’s impression of the Proxima Centauri system. Image credit: Lorenzo Santinelli.

Signal of Interest from Proxima Centauri Was Not Alien Technosignature, Astronomers Say

Oct 26, 2021 by Natali Anderson

In 2019, astronomers with the Breakthrough Listen project observed Proxima Centauri using CSIRO’s Parkes ‘Murriyang’ radio telescope. They detected...

False-color image of SN 2020fqv in its host galaxy system NGC 4567 and NGC 4568; the location of the supernova is shown in the inset. The image is composed of a pre-explosion single-band HST/WFPC2 image in the F606W filter with the color information from ground-based images obtained using the Nickel Telescope at Lick Observatory. The image of SN 2020fqv and the area outside of HST field of view is also from Nickel. Image credit: Joseph Depasquale / STScI.

Astronomers Observe ‘Rosetta Stone of Supernovae’

Oct 25, 2021 by News Staff

A Type II core-collapse supernova called SN 2020fqv exploded in NGC 4568, a member of a pair of colliding unbarred spiral galaxies; the other member of...

Super-Jupiter Found Circling Very Young, Very Low Mass Star

Oct 25, 2021 by Enrico de Lazaro

The discovery of a super-Jupiter exoplanet around the M-type dwarf star 2MASS J04372171+2651014 challenges models of planet formation by either core accretion...

An artist’s impression of a white dwarf -- in this case a white dwarf in the MV Lyrae system -- accreting as it draws in material from a companion star. Image credit: Helena Uthas.

TESS Finds Pulsating White Dwarf in TW Pictoris System

Oct 19, 2021 by News Staff

The white dwarf observed by NASA’s Transiting Exoplanet Survey Satellite (TESS) is a member of the binary system TW Pictoris and is known to be accreting...

This WISE multicolor image shows NGC 1605, a binary open cluster located 8,480 light-years away in the constellation of Perseus. It was first discovered on December 11, 1786 by the German-born British astronomer William Herschel. Image credit: NASA / WISE / Camargo, arXiv: 2109.14664.

Astronomer Discovers Ancient Binary Open Cluster in Milky Way

Oct 18, 2021 by Sergio Prostak

An open cluster called NGC 1605 is in fact two merging open clusters with evidence of tidal streams, according to new research by Professor Denilso Camargo...

An artist’s impression of the early Venus. Image credit: Manchu.

Venus Never Had Oceans, New Study Suggests

Oct 18, 2021 by News Staff

New research led by the Observatoire astronomique de l’Université de Genève suggests that water never condensed and that, consequently, oceans never...

An artist’s rendition of the MOA-2010-BLG-477Lb exoplanet and its white-dwarf host. Image credit: W.M. Keck Observatory / Adam Makarenko.

Jupiter-Mass Exoplanet Found Orbiting White Dwarf

Oct 15, 2021 by News Staff

Using a technique called gravitational microlensing, which occurs when a star close to Earth momentarily aligns with a more distant star, astronomers have...

Red dwarfs flare actively and expel particles that can alter and evaporate the atmospheres of planets in their orbit. Image credit: Leibniz Institute for Astrophysics Potsdam / J. Fohlmeister.

LOFAR Detects Coherent Radio Emission from 19 Red Dwarfs

Oct 13, 2021 by News Staff

Astronomers using the Low Frequency Array (LOFAR), a large radio telescope network located mainly in the Netherlands, have detected coherent low-frequency...

Palmerini et al. analyzed the isotopic composition of heavy neutron capture elements measured in SiC stardust grains extracted from pristine meteorites, interpreting them as the outcome of s-process nucleosynthesis occurring in the AGB stages of stars with masses between two and three solar masses and solar metallicities. Image credit: Nan Liu / Andrew Davis / NASA.

Researchers Measure Isotopic Ratios in Presolar Stardust Grains

Oct 12, 2021 by News Staff

An international team of scientists has analyzed a diverse set of presolar grains with the goal of realizing their true stellar origins. Palmerini et al....

Pluto’s haze layer shows its blue color in this picture taken by the New Horizons Ralph/Multispectral Visible Imaging Camera (MVIC). The high-altitude haze is thought to be similar in nature to that seen at Saturn’s moon Titan. The source of both hazes likely involves sunlight-initiated chemical reactions of nitrogen and methane, leading to relatively small, soot-like particles -- called tholins -- that grow as they settle toward the surface. This image was generated by software that combines information from blue, red and near-infrared images to replicate the color a human eye would perceive as closely as possible. Image credit: NASA / Johns Hopkins University Applied Physics Laboratory / Southwest Research Institute.

Pluto’s Nitrogen Atmosphere is Condensing as Dwarf Planet Moves Away from Sun

Oct 5, 2021 by News Staff

The surface pressure on the dwarf planet Pluto is decreasing and that its nitrogen atmosphere is condensing, forming ice on the dwarf planet’s surface,...

This ALMA image shows the shadow of the innermost ring on the rest of the circumtriple protoplanetary disk around GW Orionis. Image credit: ALMA / ESO / NAOJ / NRAO / University of Exeter / Kraus et al.

Massive Planets May Be Orbiting Young Triple Star GW Orionis

Oct 4, 2021 by Natali Anderson

Astronomers have found strong evidence of a massive planet (or planets) — the first planet(s) in a circumtriple orbit — in a hierarchical triple...

An artist’s rendition of the ultrahot Jupiter TOI-1518b and its parent star. Image credit: Sci-News.com.

New Ultrahot Jupiter Contains Iron in Its Atmosphere

Sep 28, 2021 by Natali Anderson

Astronomers have discovered a highly-irradiated gas giant exoplanet in close-in, highly misaligned orbit around a bright star called TOI-1518. An artist’s...

(a) WISE false color image of the Pa 30 nebula where blue and green stand for 11 μm emission, and red for 22 μm; (b) in this false color image, where green stands for WISE 11 μm (as in the left panel) and red for WISE 22 μm (adjusted to show extended emission), the emission from the central star is highlighted in blue from the GALEX near-UV data, while the XMM-Newton contors show that the majority of the X-ray emission originates from the core of the nebula; a background point source is seen westward of the CS in the XMM-Newton contour map; (c) the 2.1 m KPNO image; the green cross in the center of the image marks the location of the CS; panels (a)-(c) are reproduced at the same angular scale and orientation; at the Gaia distance of Pa 30 of 2,300 parsecs, an angular scale of 45'' translates to about 100,000 AU. Image credit: Ritter et al., doi: 10.3847/2041-8213/ac2253.

Astronomers Identify Remnant of Historical Supernova SN 1181

Sep 20, 2021 by News Staff

New research led by University of Hong Kong astronomers shows that a fast expanding nebula called Pa 30 surrounding the hot Wolf-Rayet star IRAS 00500+6713...

This Hubble image shows the globular cluster Palomar 6. The color image is a composite of separate exposures acquired by Hubble’s Wide Field Camera 3 (WFC 3) and Advanced Camera for Surveys (ACS). Image credit: NASA / ESA / Hubble / R. Cohen.

Hubble Captures Stunning New Image of Palomar 6

Sep 20, 2021 by Enrico de Lazaro

Astronomers using the NASA/ESA Hubble Space Telescope have captured the brilliance of a globular cluster called Palomar 6. This Hubble image shows the...

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