Chinese Companies are Planning to Offer Space Tourism Flights by 2025

The first Long March 5 rocket being rolled out for launch at Wenchang in late October 2016. Credit: Su Dong/China Daily

One of the more famous features of Space Age 2.0 is the rise of the commercial space industry, also known as “NewSpace.” While the space agencies of the world plan to send astronauts back to the Moon (this time, to stay), crewed missions to Mars, and robotic missions to every corner of the Solar System, NewSpace companies are offering cost-effective launch services, sending commercial astronauts to space, and commercializing Low Earth Orbit (LEO). There’s also the prospect of space tourism, with companies like Virgin Galactic, Blue Origin, and SpaceX offering suborbital flights, trips to LEO, and beyond!

China, one of the fastest-growing nations in space, is looking to offer commercial flights to suborbital space. According to senior rocket scientists Yang Yiqiang, who spoke to the state-run China Global Television Network (CGTN), China will send its first group of commercial passengers on a spaceflight, with ticket prices ranging between $287,200 to $430,800 (2 to 3 million yuan). While China is a relative newcomer to the commercial space scene, this announcement signals its intent to catch up to companies based in the U.S. and other space competitors.

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Webb Scans a Nearby Brown Dwarf and Finds it has Clouds Made of Sand

An artist's conception of a brown dwarf. A new study identifies CK Vulpeculae as the remnant of a collison between a brown dwarf and a white dwarf. Image: By NASA/JPL-Caltech (http://planetquest.jpl.nasa.gov/image/114) [Public domain], via Wikimedia Commons
An artist's conception of a brown dwarf. Brown dwarfs are more massive than Jupiter but less massive than the smallest main sequence stars. Image: By NASA/JPL-Caltech (http://planetquest.jpl.nasa.gov/image/114) [Public domain], via Wikimedia Commons

In its first few months of operation, the James Webb Space Telescope (JWST) is already proving that it was well worth the wait! To date, it has provided astronomers with the most detailed and precise images of the cosmos, conducted observations of iconic galaxies and nebulae, peered to the very edge of the Universe, and obtained spectra from distant exoplanets. These resulting images, made public through the JWST Early Release Science (ERS) program, have provided a good cross-section of what this next-generation observatory can do.

Among its many objectives, the JWST will provide valuable insights into the formation and evolution of exoplanet systems through direct imaging. Using data from the ERS, an international team of astronomers and astrophysicists conducted a direct imaging study of a brown dwarf companion (VHS 1256-1257 b) orbiting within a triple brown dwarf system approximately 69.0 light-years away. The spectra they obtained from this body provided a detailed composition of its atmosphere, which included an unexpected find – clouds made of silicate minerals (aka. sand)!

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The World’s Ground Stations are Getting Ready to Watch a Spacecraft Crash Into an Asteroid Next Week!

NASA's DART spacecraft is due to collide with the smaller body of the Didymos binary asteroid system on Sept. 26th, 2022. Credit: ESA

On September 26th, NASA’s Double-Asteroid Redirect Test (DART) will rendezvous with the Near-Earth Asteroid (NEA) Didymos. By 01:14 UTC (07:14 PM EDT; 04:14 PM PDT), this spacecraft will collide with the small moonlet orbiting the asteroid (Dimorphos) to test the “kinetic impactor” method of planetary defense. This method involves a spacecraft striking an asteroid to alter its orbit and divert it from a trajectory that would cause it to collide with Earth. The event will be broadcast live worldwide and feature data streams from the DART during its final 12 hours before it strikes its target.

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Webb Turns its Infrared Gaze on Mars

Graphic of Webb’s 2 NIRCam instrument images of Mars, taken on Sept. 5, 2022. Credit: NASA, ESA, CSA, STScI, Mars JWST/GTO team

The James Webb Space Telescope (JWST) is the most complex and sophisticated observatory ever deployed. Using its advanced suite of infrared instruments, coronographs, and spectrometers – contributed by NASA, the European Space Agency (ESA), and the Canadian Space Agency (CSA) – this observatory will spend the next ten to twenty years building on the achievements of its predecessor, the venerable Hubble. This includes exoplanet characterization, star and planet formation, and the formation and evolution of the earliest galaxies in the Universe.

However, one of the main objectives of the JWST is to study the planets, moons, asteroids, comets, and other celestial bodies here in the Solar System. This includes Mars, the first Solar planet to get the James Webb treatment! The images Webb took (recently released by the ESA) provide a unique perspective on Mars, showing what the planet looks like in infrared wavelengths. The data yielded by these images could provide new insight into Mars’ atmosphere and environment, complimenting decades of observations by orbiters, landers, rovers, and other telescopes.

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Astronomers Find a Sun-like Star Orbiting a Nearby Black Hole

Gaia BH1 is a Sun-like star co-orbiting with a black hole estimated at 10 times the Sun's mass. Credit: ESO/L. Calcada

In 1916, Karl Schwarzchild theorized the existence of black holes as a resolution to Einstein’s field equations for his Theory of General Relativity. By the mid-20th century, astronomers began detecting black holes for the first time using indirect methods, which consisted of observing their effects on surrounding objects and space. Since the 1980s, scientists have studied supermassive black holes (SMBHs), which reside at the center of most massive galaxies in the Universe. And by April 2019, the Event Horizon Telescope (EHT) collaboration released the first image ever taken of an SMBH.

These observations are an opportunity to test the laws of physics under the most extreme conditions and offer insights into the forces that shaped the Universe. According to a recent study, an international research team relied on data from the ESA’s Gaia Observatory to observe a Sun-like star with strange orbital characteristics. Due to the nature of its orbit, the team concluded that it must be part of a black hole binary system. This makes it the nearest black hole to our Solar System and implies the existence of a sizable population of dormant black holes in our galaxy.

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Mars Might Have Been Covered in Lakes in the Ancient Past

Artist's impression of Mars during the Noachian Era. Credit: Ittiz/Wikipedia Commons

Ever since robotic explorers began visiting the Red Planet during the 1960s and 70s, scientists have puzzled over Mars’ surface features. These included flow channels, valleys, lakebeds, and deltas that appear to have formed in the presence of water. Since then, dozens of missions have been sent to Mars to explore its atmosphere, surface, and climate to learn more about its warmer, wetter past. In particular, scientists want to know how long water flowed on the surface of Mars and whether it was persistent or periodic in nature.

The ultimate purpose here is to determine whether rivers, streams, and standing bodies of water existed long enough for life to emerge. So far, missions like Curiosity and Perseverance have gathered volumes of evidence that show how hundreds of large lakebeds once dotted the Martian landscape. But according to a new study by an international team of researchers, our current estimates of Mars’ surface water may be a dramatic understatement. Based on a meta-analysis of years’ worth of satellite data, the team argues that ancient lakes may have once been a very common feature on Mars.

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Hubble Sees a Spiral Galaxy With a Supermassive Black Hole Feasting at its Center

The galaxy NGC 1961 unfurls its gorgeous spiral arms in this newly released image from NASA’s Hubble Space Telescope. Credit: NASA/ESA/J. Dalcanton/R. Foley/G. Kober

Even after thirty years, and with next-generation telescopes (like the James Webb) hogging all the attention, the Hubble Space Telescope still manages to inspire. Recently, Hubble acquired a breathtaking image of NGC 1961, an intermediate spiral galaxy measuring 220,000 light years in diameter and located about 180 million light-years away in the constellation Camelopardalis. Intermediate spiral galaxies are so-named because they are between “barred” and “unbarred” spiral galaxies, which means they don’t have a well-defined bar of stars at their centers.

The data used to create this image came from two sources, the first being a study of previously-unobserved objects belonging to the Atlas of Peculiar Galaxies (or “Arp galaxies,” named after astronomer Halton Arp). The second source consisted of observations made of the progenitors and explosions of a variety of supernovae. Between 1998 and 2021, four supernovae were observed in NGC 1961 (SN 1998eb, SN 2001is, SN 2013cc, and SN 2021vaz), making it a high-value target for study.

The resulting image captures the dusty spiral arms, bright, hot star-forming regions of NGC 1961 and the galaxy’s glowing center that manages to outshine all the stars in its disk. This is an example of an active galactic nucleus (AGN), where the central region emits tremendous amounts of energy because it contains a supermassive black hole (SMBH) that feeds on the surrounding dust, gas, and stars in the core region.

Many AGNs have been observed emitting bright jets of hot dust and gas that are accelerated to relativistic speeds (a fraction of the speed of light). These jets can be seen millions of light-years away and play an important role in a galaxy’s evolution. NGC 1961 is a fairly common type of AGN that shines brightly but emits low-energy-charged particles. It just goes to show that the old workhorses never lose their mojo! They just keep on delivering well into their later years!

Further Reading: NASA

A Galaxy With Ten Times the Mass of the Milky Way is Preparing to Become a Quasar

The massive, hyper-luminous galaxy W0410-0913 and its surroundings, seen 12 billion years back in time. Credit: M. Ginolfi & G. Jones / VLT / ESO.

One of the fundamental questions in astronomy is how galaxies formed over 13 billion years ago and have evolved ever since. A common feature that astronomers have noted is that most galaxies appear to have supermassive black holes (SMBHs) at their center – like Sagittarius A*, the ~4 million solar mass SMBH at the center of the Milky Way. These monster black holes occasionally swallow up nearby gas, dust, and stars and emit excess energy as powerful relativistic jets. This phenomenon, where the center of a galaxy outshines the stars in the disk, is known as an Active Galactic Nucleus (AGN) or quasar.

In a recent study, an international team of astronomers led by the European Southern Observatory (ESO) discovered a galaxy in the early Universe that could reveal more about this evolution. Using the Very Large Telescope (VLT) and the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile, they observed a swarm of galaxies orbiting a very bright and vigorously star-forming galaxy in the early Universe. These observations provide fresh insight into how exceptionally bright galaxies grow and evolve into quasars and emit powerful jets of light across the observable Universe.

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There Could be as Many Water Worlds as Earths in the Milky Way

Artist’s impression of the strange landscape of a water world. Credit: Pilar Montañés

On July 12th, 2022, NASA released the first images acquired by the James Webb Space Telescope, which were taken during its first six months of operation. Among its many scientific objectives, Webb will search for smaller, rocky planets that orbit closer to their suns – especially dimmer M-type (red dwarf) stars, the most common in the Universe. This will help astronomers complete the census of exoplanets and gain a better understanding of the types of worlds that exist out there. In particular, astronomers are curious about how many terrestrial planets in our galaxy are actually “water worlds.”

These are rocky planets that are larger than Earth but have a lower density, which suggests that volatiles like water make up a significant amount (up to half) of their mass-fraction. According to a recent study by researchers from the University of Chicago and the Instituto de Astrofísica de Canarias (IAC), water worlds may be just as common as “Earth-like” rocky planets. These findings bolster the case for exoplanets that are similar to icy moons in the Solar System (like Europa) and could have significant implications for future exoplanet studies and the search for life in our Universe.

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Mars did Have Moving Glaciers, but They Behaved Differently in the Planet's Lower Gravity

Glacial landscapes on Axel Heiberg Island (Canadian Arctic Archipelago) showing typical (glaciers) and atypical (subglacial channels, bottom right) glacial landscapes. Credit: A. Grau Galofre

On Earth, shifts in our climate have caused glaciers to advance and recede throughout our geological history (known as glacial and inter-glacial periods). The movement of these glaciers has carved features on the surface, including U-shaped valleys, hanging valleys, and fjords. These features are missing on Mars, leading scientists to conclude that any glaciers on its surface in the distant past were stationary. However, new research by a team of U.S. and French planetary scientists suggests that Martian glaciers did move more slowly than those on Earth.

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