The morning sky will be putting on a show worth waking up for.
On Saturday (April 30) and Sunday, Venus and Jupiter will be in conjunction – where they’ll look as if they’re nearly touching each other. The two will come within 0.2 degrees of each other, though they’re actually 690 million kilometres apart in space.
Stargazers will have to wake up around near dawn, or just before 5 a.m. on Saturday to see the planetary show. As a reward, they’ll be treated not only to the conjunction of Venus and Jupiter — Mars, and Saturn will be visible as well.
The planets are best viewed through a pair of binoculars or a telescope if you have one handy. Just make sure to be careful using them as the sun comes up to avoid any damage to your eyes.
After the big conjunction on Saturday, Venus and Jupiter will begin to separate again and stargazers can watch them slowly drift apart over the following days.
All this planetary action coincides with a new moon and a partial solar eclipse. This means that it’ll be easier to view the planets in the morning sky due to the lack of light from the moon. Unfortunately, the eclipse won’t be visible from the Northern Hemisphere. But in the Southern Hemisphere, nearly 64 per cent of the sun’s disc will be hidden behind the moon.
But don’t be too dimmed by the lack of eclipse action. On the night between May 4 and 5, the Halley’s Comet will bring the Eta Aquarids meteor shower. The best viewing will be from 3 a.m. to 5 a.m. and skywatchers will see between 10 to 30 meteors per hour at the shower’s peak. Just don’t try to catch too many winks of sleep or you may miss the speedy comets as they streak across the sky.
So, if you wake up early this week you can treat yourself to something out of this world.
Blood moon, big city: Skywatcher captures total lunar eclipse over New York – Galaxy Reporters
The moon during eclipse burns red high above the yellow lights of New York City in beautiful photos caught by novice astronomer Alexander Krivenyshev.
Alexander Krivenyshev is the president of WorldTimeZone.com, who snapped images of the total lunar eclipse on Sunday night (May 15) from Guttenberg, New Jersey, outside the Hudson River from the Big Apple.
Krivenyshev told Space.com through the email that he maintained through cloudy conditions to get shots of the blood-red moon glowing like a beacon in a light-polluted sky.
The eclipse started at 9:32 p.m EDT on Sunday (0132 GMT on May 16) when the moon nosed into the dark part of Earth’s shadow, recognized as the penumbra, and stopped five hours later. The total eclipse phase, in which Earth’s huger umbral shadow blackened the moon, survived 85 minutes longer than any lunar eclipse in 33 years.
Earth’s closest neighbor temporarily turns coppery red during entire lunar eclipses. This “blood moon” impact is caused by Earth’s atmosphere, which bends some red light throughout the lunar surface while scattering away shorter-wavelength light.
— SPACE.com (@SPACEdotcom) May 18, 2022
Last weekend’s sky show was nicely observed from America and fractions of Western Europe and West Africa. It was the first total lunar eclipse of the year; however, it won’t be the last. One more eclipse will occur on Nov. 8. The Nov. 8 lunar eclipse will be observed from Australia, eastern Asia, and the western United States.
Searching for the Milky Way's Black Hole – Skywatching – Castanet.net
When we look into the southern sky close to the horizon on summer evenings, we are looking towards the centre of our galaxy, the Milky Way.
It is lurking around 30,000 light years behind the stars making up the constellation of Sagittarius, “The Archer”. However, thanks to our location in the disc of our galaxy, our view is blocked by huge clouds of stars, gas and dust.
Our first images of the centre of the Milky Way were obtained by means of radio telescopes, which show us what the universe would look like if we could see radio waves rather than light. They revealed a strange, bright and unusually small radio source.
Measurements of the speeds stars orbit the centre of our galaxy indicate that at the same position as the bright radio source lies something very massive, very small and active. The best candidate to explain this is a black hole.
Radio waves have power to penetrate clouds and dust, which is why radar is so useful for navigation, detecting threats and avoiding hazards at night or in bad weather. However, radio waves have this greater penetration power because they are much longer than light waves. This means that to see detail when observing at radio wavelengths we need to use huge antennas.
To have the same ability to discern detail as the human eye, a radio telescope tuned to the wavelength of emissions from cosmic hydrogen (21cm) the antenna would need to be about a kilometre in diameter. Moreover, black holes are small by cosmic standards and at great distances, so to discern any details the radio telescope would need an antenna the size of the Earth.
This sounds impossible, but there is a solution, a technique called “Very Long Baseline Interferometry”.
In the 1960s, Canada was the first country to succeed in combining radio telescopes thousands of kilometres apart so that they would have the detail discerning ability of a radio telescope thousands of kilometres in diameter.
This procedure has made possible a powerful, new astronomical instrument, the Event Horizon Telescope (EHT).
Several radio telescopes, thousands of kilometres apart operate in collaboration to observe the centre of the Milky Way at the same time. One of them is the Atacama Large Millimetre Array, located in Chile, in which Canada is a partner. In addition, scientists at several Canadian universities are involved.
The collaboration is named after the boundary that forms around black holes, called the event horizon. This is a one-way boundary in space-time—stuff can fall in but nothing, not even light, gets out. This is why they are called black holes.
However, even if we cannot see the black holes directly, we can certainly see the disc of material swirling around the black holes as it gets sucked in. This stuff gets very hot, and has intense magnetic fields trapped in it, so the black hole announces itself with radio emissions and X-rays from that disc.
The first target for the Event Horizon Telescope was the galaxy M87, located some 55 million light years away. It had long been suspected that a very energetic black hole lies at its centre, a big one, around 5 billion times the mass of the Sun. The EHT gave us our first image of that black hole.
Then the EHT radio telescopes were turned on the centre of our galaxy, and got our first image of our black hole. Luckily for us, it is much less massive and active than the one at the centre of M87. At four million times the mass of the Sun, it is relatively tiny.
We believe most spiral galaxies have big black holes in their cores. It is not clear whether galaxies get them when they form or they appear later. However, learning about their roles in galaxies should tell us more about how galaxies form and evolve to the point where they develop stars and planets, and because we live in one, it would be nice to know.
• Venus, Jupiter, Mars and Saturn are still lined up in the dawn glow, in order of decreasing brightness.
• The Moon will be new on May 30.
This article is written by or on behalf of an outsourced columnist and does not necessarily reflect the views of Castanet.
Boeing's Starliner approaching ISS in high-stakes test mission – Phys.org
Boeing’s Starliner capsule was preparing to dock with the International Space Station Friday, in a high-stakes uncrewed test flight key to reviving the US aerospace giant’s reputation after a series of failures.
The spaceship blasted off from the Kennedy Space Center in Florida on Thursday evening, and is now set to rendezvous with the ISS at 7:10 pm Eastern Time (2310 GMT), as part of a mission to prove it is capable of providing safe rides for NASA astronauts.
Starliner encountered some propulsion problems early in its journey, with two thrusters responsible for placing it in a stable orbit failing for unclear reasons—though officials insisted everything remained on track.
“Overall, the spacecraft is doing really well,” Steve Sitch, program manager for NASA’s Commercial Crew Program told reporters at a post-launch press conference, in which he nonetheless flagged anomalies that engineers are working to understand.
One of 12 orbital maneuvering and attitude control (OMAC) thrusters located on Starliner’s aft side failed after one second, at which point a second thruster kicked in and took over, but also cut out after 25 seconds.
The ship’s software then engaged a third thruster that completed the necessary burn.
The OMAC thrusters are set to be used to bring Starliner closer to the ISS, and to help de-orbit the spacecraft near the end of the mission.
“We’ll go look at the data and try to understand what happened. And then from a redundancy perspective, can we recover those thrusters?” said Sitch.
Starliner’s success is key to repairing Boeing’s frayed reputation after its first launch, back in 2019, failed to dock with the ISS due to software bugs—one that led to it burning too much fuel to reach its destination, and another that could have destroyed the vehicle during re-entry.
A second try was scheduled in August 2021, but the capsule was rolled back from the launchpad to address sticky valves that weren’t opening as they should, and the vessel was eventually sent back to the factory for fixes.
NASA is looking to certify Starliner as a second “taxi” service for its astronauts to the space station—a role that Elon Musk’s SpaceX has provided since succeeding in a test mission for its Dragon capsule in 2020.
Both companies were awarded fixed-price contracts—$4.2 billion to Boeing, and $2.6 billion to SpaceX—in 2014, shortly after the end of the Space Shuttle program, during a time when the United States was left reliant on Russian Soyuz rockets for rides to the orbital outpost.
Boeing, with its hundred-year history, was considered by many as the sure shot, while then-upstart SpaceX was less proven.
In reality, it was SpaceX that rocketed ahead, and recently sent its fourth routine crew to the research platform—while Boeing’s development delays have cost the company hundreds of millions of dollars.
Starliner should dock with the ISS about 24 hours after launch, and deliver more than 800 pounds of cargo.
Its sole passenger is a mannequin named Rosie the Rocketeer—a play on the World War II campaign icon Rosie the Riveter—whose job is to collect flight data with her sensors in order to learn what human astronauts would experience.
“We are a little jealous of Rosie,” NASA astronaut Mike Fincke, who is expected to be among the first crew selected for a manned demonstration mission should OFT-2 succeed, said at a press conference this week.
The gumdrop-shaped capsule will spend about five days in space, then undock and return to Earth on May 25, using giant parachutes to land in the desert of the western United States.
NASA sees a second provider to low Earth orbit as a vital backup, should SpaceX encounter problems.
© 2022 AFP
Boeing’s Starliner approaching ISS in high-stakes test mission (2022, May 20)
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