Category Astronomy/Space

Mysterious Planet Nine May Be a Captured ‘Rogue’ World

Mysterious Planet Nine May Be a Captured 'Rogue' World

Artist’s illustration of Planet Nine, a world about 10 times more massive than Earth that may lie undiscovered in the far outer solar system. Credit: Caltech/R. Hurt (IPAC)

Space researchers James Vesper and Paul Mason with New Mexico State University have given a presentation at this year’s American Astronomical Science meeting outlining the results of simulations they have been running to learn more about Planet Nine—a planet that many in the space science community believe exists far beyond Pluto. They presented evidence suggesting that if Planet Nine is out there, it is likely a rogue.

Planet Nine was first predicted to exist just 2 years ago, when a team of investigators noticed what appeared to be an unknown gravitational influence in the outer solar system...

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Our Galaxy’s Black Hole is Spewing out planet-size ‘Spitballs’

This artist's conception portrays a collection of planet-mass objects that have been flung out of the galactic center at speeds of 20 million miles per hour (10,000 km/s). These cosmic "spitballs" formed from fragments of a star that was shredded by the galaxy's supermassive black hole. Credit: Mark A. Garlick / CfA

This artist’s conception portrays a collection of planet-mass objects that have been flung out of the galactic center at speeds of 20 million miles per hour (10,000 km/s). These cosmic “spitballs” formed from fragments of a star that was shredded by the galaxy’s supermassive black hole. Credit: Mark A. Garlick / CfA

Every few thousand years, an unlucky star wanders too close to the black hole at the center of the Milky Way. The black hole’s powerful gravity rips the star apart, sending a long streamer of gas whipping outward. New research shows that not only can the gas gather itself into planet-size objects, but those objects then are flung throughout the galaxy in a game of cosmic “spitball.”

“A single shredded star can form hundreds of these planet-mass objects...

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Astronomers discover Molecular and Atomic Clouds associated with a Superbubble in LMC

Astronomers discover molecular and atomic clouds associated with a superbubble in LMC

RGB image of the superbubble 30 Doradus C observed by Chandra (Bamba et al. 2004). The red, green, and blue colors represent the energy bands, 0.5–1.2, 1.2–2.0, and 2.0–7.0 keV, respectively. Credit: Sano et al., 2017.

An international team has uncovered molecular and atomic gas clouds associated with the superbubble 30 Doradus C, located in the Large Magellanic Cloud (LMC). Called superbubble or supershell, 30 Doradus C is a bright X-ray cavity in the LMC with a diameter of approximately 300 light years. Although it was well studied at different wavelengths that revealed its shell-like morphology and 6 stellar clusters, the interstellar gas associated with this superbubble has not been thoroughly investigated yet.

Due to its proximity and face-on inclination to Earth, LMC serves as ...

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Gravitational Biology: Real Time Imaging and Transcriptome Analysis of Fish aboard Space Station

a-d) Whole-body imaging of the osterix-DsRed transgenic line. The left-side images show the same ground control at day 1; and the right-side images, the same flight medaka at day 1. Arrows point to the head and fin region. All images show ventral views. Montage images were made from 6 captured optical images, divided by dotted lines (a,b). The white region shows an osterix-DsRed fluorescent signal. Embedded views show the enlarged head region (c,d). (e) The fluorescent intensity from day 1 to 7 of observation day constantly increased in the flight group. (f-h) The representative visualizing data for osterix-DsRed/TRAP-GFP in the flight group. All images show ventral views in the head region. (i-l) The merged images were captured by 3D views for osterix-DsRed and TRAP-GFP in the pharyngeal bone region of the double transgenic line. The pharyngeal bone region in the ground control (i) or the flight (k) group at day 4. The image for TRAP-GFP in the pharyngeal bone region of "i" (j) or "k" (l). lp, lower pharyngeal bone; c, cleithrum. GFP signals identify osteoclasts (OC). Credit: Tokyo Institute of Technology

a-d) Whole-body imaging of the osterix-DsRed transgenic line. The left-side images show the same ground control at day 1; and the right-side images, the same flight medaka at day 1. Arrows point to the head and fin region. All images show ventral views. Montage images were made from 6 captured optical images, divided by dotted lines (a,b). The white region shows an osterix-DsRed fluorescent signal. Embedded views show the enlarged head region (c,d). (e) The fluorescent intensity from day 1 to 7 of observation day constantly increased in the flight group. (f-h) The representative visualizing data for osterix-DsRed/TRAP-GFP in the flight group. All images show ventral views in the head region...

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