Astronomers still have yet to directly capture an image of a black hole—they’re working on it—but they know where some of the largest ones are: inside the hearts of galaxies, where they power brilliant and powerful quasars whose light can be seen across the Universe. Some of these supermassive black holes (SMBs) can contain the mass of millions if not billions of Sun-sized stars and, when two galaxies happen to collide (which they often do) their respective resident SMBs can end up locked in an orbital embrace. As their spinning dance grows tighter and tighter they send out gravitational waves, rippling the very fabric of space and time itself (the LIGO experiment announced the first detection of these waves in 2016.) But if the gravitational waves are uneven, say because the two merging SMBs are of vastly different masses and/or individually spinning in different orientations (a possible but not common scenario) then the super-duper-supermassive black hole that results from the merger can end up getting one serious cosmic-scale kick after the event occurs and the waves shut off—perhaps a strong enough kick to send it hurtling out of the galaxy altogether.
That’s what astronomers think we’re witnessing here in this image from the Hubble Space Telescope.
See that big rock there? (It’s easy because there’s a big yellow arrow pointing to it.) That’s a 100-foot/30-meter wide boulder that was imaged sitting on the surface of Comet 67P/Churyumov-Gerasimenko by ESA’s Rosetta on May 2, 2015. Nine months later Rosetta captured another image of the same area in which that huge stone had clearly moved—find out below just how far!
From July 1969 to December 1972, 12 American astronauts landed in six different locations on the lunar surface as part of NASA’s Apollo program, leaving their footprints and taking samples and data that are still being used today to learn about the Moon. The Apollo landing sites remain exactly as they were left over four decades ago—footprints, rover tracks, discarded equipment and all—and with a new generation of space explorers around the world setting their sights on the Moon it’s important that we make sure these six off-world locations are preserved, just as would be done with any historic artifact.
“President Donald Trump on Tuesday, March 21 signed the NASA Transition Authorization Act of 2017, which includes a section [Sec. 831] directing the White House Office of Science and Technology Policy (OSTP) [a position yet to be filled] to assess the issues that relate to “protecting and preserving historically important Apollo program lunar landing sites and Apollo program artifacts residing on the lunar surface, including those pertaining to Apollo 11 and Apollo 17,” the first and last missions to land astronauts on the [M]oon.” (via CollectSpace)
While this is only a plan for an assessment to take place, it’s a(nother) first step in making sure our first footprints on another world aren’t lost to careless or malicious future lunar visitors, whether human or robotic.
Read the full story on CollectSpace: White House to look at how best to ‘protect and preserve’ Apollo moon landing sites
In its long history of space exploration the United States has never had a robotic mission sent to the surface of Venus. Flybys, orbiting spacecraft, and atmospheric probes yes, but to date nothing from NASA has operated on the extreme, hellish surface of the second rock from the Sun. Russia, on the other hand, has successfully landed on Venus ten times, eight with its Venera program and the ninth and tenth in 1984–85 with the Vega 1 and 2 missions. Because of its long-running expertise, the U.S. is looking to partner with Russia on a brand-new Venera mission, Venera-D, which in 2025 would send an orbiter, a lander, and possibly even an inflatable airship to Venus to explore its exotic and overheated environments.
“While Venus is known as our ‘sister planet,’ we have much to learn, including whether it may have once had oceans and harbored life,” said Jim Green, NASA’s director of Planetary Science. “By understanding the processes at work at Venus and Mars, we will have a more complete picture about how terrestrial planets evolve over time and obtain insight into the Earth’s past, present and future.”
Read the full story from NASA here: NASA Studying Shared Venus Science Objectives with Russian Space Research Institute
Supernovas are some of the most powerful and energetic events in the entire Universe. When a dying star explodes you wouldn’t want to be anywhere nearby—fresh elements are nice and all, but the energy and radiation from a supernova would roast any planets within tens if not hundreds of light-years in all directions. Luckily for us we’re not in an unsafe range of any supernovas in the foreseeable future, but there was a time not very long ago (in geological terms) that these stellar explosions occurred nearby (in astronomical terms) and in 2016 scientists found the “smoking gun” evidence at the bottom of the ocean.
What’s more, the arrival of the iron-rich fallout from those stellar explosions seems to coincide with ancient global temperature changes*, the most recent dated near the start of the last major ice age which brought lower sea levels, widespread glaciation…and eventually the rise of the first modern humans.
Read more at Universe Today here: Nearby Supernovas Showered Earth With Iron
*Note: the changes in climate referred to here are not the same as the climate change we are witnessing today. Not only are we now seeing rapid warming of land and sea temperatures globally, but today’s forcings are the result of increasing greenhouse gases like carbon dioxide in the atmosphere—not radioactive iron from exploding stars.
At the north pole of Saturn’s largest moon Titan lie the largest (and only known) bodies of surface liquid in the Solar System outside of Earth. But on Titan, where temperatures are regularly around negative 300ºF, the liquid isn’t water but rather methane and ethane: compounds which are found as gases here on Earth. Titan’s seas and lakes are exotic environments that scientists are only just starting to understand, and even with radar imaging by NASA’s Cassini spacecraft there’s a lot we just don’t know about them. But one thing some researchers have managed to figure out using simulated Titan environments in the lab is that these lakes may sometimes fizz with bubbles of nitrogen—potentially explaining some of the mysteries of Cassini’s observations.
“Thanks to this work on nitrogen’s solubility, we’re now confident that bubbles could indeed form in the seas, and in fact may be more abundant than we’d expected,” said Jason Hofgartner of JPL, who serves as a co-investigator on Cassini’s radar team and was a co-author of the study.
Read the news straight from NASA here: Experiments Show Titan Lakes May Fizz with Nitrogen