Using the Hubble Space Telescope (HST), astronomers from the University of California Santa Cruz (UCSC) and elsewhere have observed an ultra-diffuse galaxy known as FCC 224. Results of the observational campaign, published Jan. 18 on the arXiv pre-print server, provide important insights into the properties of this galaxy and its globular cluster system.

Globular clusters (GCs) are collections of tightly bound stars orbiting galaxies. Astronomers perceive them as natural laboratories enabling studies on the evolution of stars and galaxies. In particular, GCs could help researchers to better understand the formation history and evolution of early-type galaxies, as the origin of GCs seems to be closely linked to periods of intense star formation.

Located some 65 million light years away in the Fornax galaxy cluster, FCC 224 is a quiescent ultra-diffuse galaxy about 10 billion years old. It has a major axis effective radius of approximately 6,160 light years and its mass is estimated to be at a level of 200 million solar masses.

Southwest Research Institute partnered with the Carnegie Institution for Science to perform laboratory experiments to better understand how Saturn’s moon Titan can maintain its unique nitrogen-rich atmosphere. Titan is the second largest moon in our solar system and the only one that has a significant atmosphere.

“While just 40% the diameter of the Earth, Titan has an atmosphere 1.5 times as dense as the Earth’s, even with a lower gravity,” said SwRI’s Dr. Kelly Miller, lead author of a paper about these findings published in the journal Geochimica et Cosmochimica Acta. “Walking on the surface of Titan would feel a bit like scuba diving.”

The origin, age, and evolution of this atmosphere, which is roughly 95% nitrogen and 5% methane, has puzzled scientists since it was discovered in 1944.

“Part of the atmosphere of this planet is moving towards us at a high velocity while another part is moving away from us at the same speed,” said Dr. Lisa Nortmann.

Do weather patterns on exoplanets mimic those on Earth? This is what a recent study published in Astronomy & Astrophysics hopes to address as an international team of researchers explored unique weather patterns on WASP-127b, which is a hot Jupiter exoplanet located approximately 520 light-years from Earth. This study has the potential to help scientists better understand the formation and evolution of weather patterns on exoplanets throughout the cosmos and how these patterns compare to Earth’s.

For the study, the researchers used the CRyogenic high-resolution InfraRed Echelle Spectrograph (CRIRES+) instrument installed on the European Southern Observatory’s (ESO) Very Large Telescope (VLT) to observe the atmospheric characteristics during one transit of WASP-127b passing in front of its parent star, with one orbit being completed in approximately 4.2 days.

In the end, the researchers identified signals of water (H2O) and carbon monoxide (CO) within WASP-127b’s atmosphere, along with identifying supersonic jet winds occurring at the exoplanet’s equator estimated to be traveling at approximately 7.7 kilometers per second (4.8 miles per second) or 27,720 kilometers per hour (17,280 miles per hour). These winds were identified to only exist at the equator and not at the poles. For context, the fastest winds recorded at the Earth’s equator is only a few kilometers (miles) per hour. They also found significant temperatures differences between the dayside and night side of WASP-127b, which mimics planetary atmosphere behavior of Earth and other planets in our solar system.