ASTRONOMY
In the Sky this Week, Astronomy News, and TWSftUoTtCBDftSoTiFoOT
IN THE SKY THIS WEEK
ASTROTOURISM IS A THING! And not just for Total Solar Eclipses! Over 80% of Americans live in areas where light pollution is so severe that one can never see the Milky Way; they see only the brightest stars and planets on a good night. Astronomical communities and Dark Sky zones are springing up in places where one can actually see a dark sky. Many U.S. National Parks and Monuments, at least those in favorable locations, have Dark Sky programming and events!
It's Not Too Early to Plan for 2028! I hate to say it, but the tourism opportunities for the 2026 total solar eclipse in Iceland/Spain/Majorca and for the 2027 total solar eclipse in Egypt are filling up quickly. But there is another opportunity in 2028, a total eclipse that slashes across Australia, hitting Sydney dead center, before going on to the South Island of New Zealand, where totality will occur near sunset. Fred “Mr. Eclipse” Espenak has published information on this particular viewing opportunity at: http://astropixels.com/pubs/Guide2028.html.
Nova Watch: No, I’m not promoting the really good PBS series, I’m talking about T Coronae Borealis, a recurring nova. It’s usually about magnitude +10, not exactly a target for most backyard astronomers. However, every 80 years or so, it goes nova, becoming as bright as Alphecca, the brightest star in the Northern Crown (Corona Borealis). The last time it blew was in 1946, and its starting to show the same signs it did back then before it brightened.
I would suggest you become familiar with the look of this particular constellation so you can see the change for yourself when it happens. You can find out more about it at: https://skyandtelescope.org/astronomy-news/observing-news/this-weeks-sky-at-a-glance-june-7-16 . There is a link within to a 2016 Sky & Telescope article by Bob King that shows you how to find T CrB at its normal brightness. There’s even a more recent S&T piece that will help you find the “Blaze Star”: https://skyandtelescope.org/astronomy-news/is-the-blaze-star-about-to-blow-you-may-be-the-first-to-know. We’ll need a little luck, since the maximum brightness of T CrB will only last a few hours.
Here's the Latest on T CrB: https://phys.org/news/2024-09-flares-blaze-star-corona-borealis.html!
A Helpful Tip from Dr. Steve: If you do an Internet search on “Blaze Star,” be sure you don’t channel your inner Ringo and spell it with two “r”s. Just ask Governor Earl Long….
But wait, there’s more! There is a supernova right now in galaxy NGC 3524, in Leo. It’s shining as brightly as the entire galaxy it’s in! Those of you with access to a relatively-good telescope – check it out!
Sun: The Sun has an ~11-year cycle of sunspot activity. The last minimum period was in late 2020; the next maximum will be in mid-2025. NOAA’s 30-Minute Aurora Forecast: https://www.swpc.noaa.gov/products/aurora-30-minute-forecast.
Sun: Nazmus Nasir took some extremely good eclipse pictures last April, part of NASA’s Eclipse Megamovie 2024 Project. Check them out, and his eclipse movie, at: https://science.nasa.gov/get-involved/citizen-science/an-eclipse-megamovie-megastar!
THE PLANETS NEXT WEEK
Moon: The Moon reaches First Quarter at 2:06 AM EDT on Wednesday, September 11
Mercury (-1.0) is now in the early morning sky, just above Regulus in the ENE.
Venus is still quite low in the evening twilight sky this week, shining at -3.8. It will lie close to Virgo’s lucida, Spica, this week.
Mars (+0.6) and Jupiter (-2.3) were very close together in the V-shaped “face” of Taurus last month, but they’ve been separating ever since. Jupiter still lies between the horns of Taurus, but Mars is now near Castor’s feet.
Saturn is presently in Aquarius, to the lower-right of the Great Square, shining at +0.6. It culminates in the south around local midnight.
Uranus lies very close to Mars this week, in western Taurus, shining at +5.7; here’s a sky chart for it.
Neptune (+7.8) is in Pisces, doable but you’ll need a sky chart (e.g.here).
COMETS
Sky & Telescope’s “Best Comets in 2024:” https://skyandtelescope.org/astronomy-news/the-best-comets-in-2024
Comets (presently brighter than +10): There are presently only three, with a fourth a “maybe.”
Comet Watch: Recently-discovered Comet C/2023 A3 (Tsuchinshan-ATLAS) is on a trajectory that will bring it near enough to Earth in October, 2024, for it to be potentially an unaided-eye object. It’s already at +9.8, lying in/near Sextans. It may brighten quickly in the coming weeks. Sky & Telescope has info (5/12) on this newcomer and a sighting map, see: https://skyandtelescope.org/observing/celestial-objects-to-watch/comets/comet-tsuchinshan-atlas-brightens-grows-a-tail! There is some possibility it could be really bright, see: https://phys.org/news/2023-03-astronomers-comet-brighter-stars-year.html and http://www.aerith.net/comet/catalog/2023A3/2023A3.html. Let’s be optimistic (but I remember not seeing Kohoutek…).
SAD (?) UPDATE on C/2023 A3: The comet is not brightening as much as expected (hoped) as it approaches the Sun. There is some evidence that the comet is starting to break up due to the Sun’s gravity. If it does fragment, the show will be pretty much over before it starts. For a summary of this pessimistic outlook, see: https://phys.org/news/2024-07-comet-tsuchinshan-prior-sun.html; for a preprint of the scientific paper, see: https://arxiv.org/pdf/2407.06166.
The aerith website has not been updated recently as to the brightness of C/2023 A3. It will become visible again in the northern hemisphere in October.
Comet 12P/Pons-Brooks, discovered in 1812, has also arrived in its 70-year period. It’s fading quickly (now about our +10 threshold) but it is no longer visible in the northern hemisphere (it’s now near Crux). For more information, see here and here. This particular comet has been in a number of Science-phobic social media posts because of an unfortunate asymmetric release of a pulse of gas and dust, briefly forming a twin tail that some have taken to be the (actual) Devil’s horns or that the comet is a giant version of the Millenium Falcon. Comets always seem to get a bad rap! The orientation of its orbit causes it to appear to have two tails, one following and one ahead of it, much like Comet Arend-Roland back in 1057! Here’s some more real information about it: https://phys.org/news/2024-03-12ppons-brooks-devil-comet.html.
Comet 13P/Olbers has returned to perihelion, on its 68-year orbit. Not paradoxically, it has started to fade, presently shining at +8, but it’s too close to the Sun in the sky to be seen, being near Arcturus. Sky & Telescope has a detailed chart of Olber’s position; see here.
No other comets are anywhere near +10.
For info on comets currently visible, see: http://www.aerith.net/comet/weekly/current.html.
SATELLITES NEXT WEEK
International Space Station
There are 12 overpasses of the ISS this week for those of you in the DC area; two are good, one is fair, and nine are unfavorable.
On Tuesday, September 10, the ISS will appear at 8:47 PM EDT, 10° above the SW horizon, near Antares and the Moon, then rise to an altitude of 66°, near Delphinus, then descend to 50° above the E horizon, where it will disappear abruptly into the Earth’s shadow.
On Thursday, September 12, the ISS will appear at 8:50 PM EDT, 10° above the WSW horizon, then rise closely past Arcturus to an altitude of 40°, near Kochab, then descend to 18° above the NNE horizon, near Perseus, where it will disappear.
On Friday, September 13, the ISS will appear at 10:03 PM EDT, 10° above the WSW horizon, rise to an altitude of 67°, near the head of Draco, then descend through Cepheus and Cassiopeia to 10° above the NE horizon, where it will disappear.
There are 12 overpasses of the ISS this week for those of you in the Colorado Springs area. One is very good, one is quite good, one is eh-good, and nine are unsatisfactory.
On Tuesday, September 10, the ISS will appear 10° above the SSW horizon at 10:20 PM MDT, near the Moon and Antares, rise to an altitude of 41°, then descend to 26° above the E horizon, in the Great Square, where it will disappear abruptly into the Earth’s shadow.
On Thursday, September 12, the ISS will appear 10° above the WSW horizon at 8:22 PM MDT, then rise through Corona Borealis to an altitude of 59°, in Draco, then descend to 13° above the NE horizon, where it will disappear.
On Friday, September 13, the ISS will appear 10° above the SW horizon at 7:35 PM MDT, then rise to an altitude of 80°, near Vega, then descend through Cygnus to 10° above the NE horizon, where it will disappear.
Hubble Space Telescope
There are no overpasses of the HST this week for those of you in the DC area.
There are no overpasses of the HST this week for those of you in the Colorado Springs areas.
To find out about satellite overpasses in your area, see https://heavens-above.com (set your own location in the upper-right corner).
ASTRONOMY NEWS
THE AMAZING GAIA!
ESA’s Gaia spacecraft has been making extremely detailed measurements of the movements of stars, asteroids, and other objects both near and far. The analysis of Gaia data has led to a better understanding of the formation and present shape of our Milky Way galaxy, profoundly affected by a collision with another galaxy, Gaia-Enceladus, billions of years ago. Further, Gaia data has been used recently to determine odd features of the Milky Way’s central super-massive black hole. The best model for it shows that the present version of the black hole arose from the collision of three black holes that merged into one larger black hole. Gaia has exceeded all expectations of its scientists and engineers, and is still going strong despite some infirmities of age. For more information on this amazing discoveries, see: https://scitechdaily.com/the-merger-that-led-to-the-formation-of-the-milky-way and https://phys.org/news/2024-09-massive-merger-reveals-evidence-supermassive.html.
“Recent” Milky Way Collision: Astronomers have long believed that collisions between galaxies are fairly common, and that our own Milky Way has not been exempt. The Magellanic Clouds and perhaps even globular clusters are remnants of our collisional past, some 8-11 billion years ago. Recent observations and computer modeling, however, suggests that a collision has occurred more recently, on the order of three billion years ago. A team from RPI used data from ESA’s Gaia satellite, which is mapping a billion stars across the Milky Way, noting their motion, luminosity, and composition. Those data were used in creating computer modeling of how those stars may have acquired that motion.
As you might imagine, an inter-galactic collision and their combined and shifting gravity, would affect the movement of individual stars significantly, creating a wavy structure not unlike ripples in a pond. Such rhythmic stellar motions would tend to dampen with time, giving at least a crude estimation of the time since the original disturbance. When the Gaia data are put in the model, there is more wavy structure than would be expected if the disturbing collision was as old as thought, the collision had to have been more recent. For an announcement and summary of this research, see: https://news.rpi.edu/2024/06/06/rensselaer-researchers-upend-theory-about-formation-milky-way-galaxy.
Gaia Woes: ESA’s Gaia spacecraft has been occupying the Earth-Sun L2 point for over a decade, making high-precision observations of the locations and motions of over a billion stars in our Milky Way. However, it has faced two threats to its operation in recent months: high-speed micrometeors and the strongest solar storm in twenty years. Gaia was designed to withstand small impacts, and it has done so, but last April it was hit by one in a sensitive spot. The damage allows a tiny amount of light to enter the spacecraft from time to time, which interferes with the operation of its “billion-pixel” camera. Engineers understand the problem and have come up with ways to avoid (or put up with) it. One of its CCD cameras, vital for validating observations, has failed, and now Gaia is returning a LOT of false positives. The timing of the failure coincides with the big aurora-producing solar storm last May. Gaia normally returns 25 gigabytes of data daily; false positives were increasing that amount to the point that the receiving systems were overloaded. But there has been a silver lining to the cloud of data overload. Engineers have tweaked the threshold detection limit for stars, reducing the false positives to a manageable level. Even better, the short hiatus caused by the overload gave engineers a chance to refocus Gaia’s twin telescopes, and the venerable spacecraft is “now producing some of the best quality data it ever has.” For more on this happy story, see: https://phys.org/news/2024-07-gaia-micrometeoroid-solar-storm.html.
Gaia’s Joys: In spite of its woes, Gaia provided some joy recently, especially to asteroid fans. Gaia has always been an amazing asteroid finder, and it has determined the orbits of over 150,000 asteroids. A new study published in Astronomy & Astrophysics reports the finding of 352 new binary asteroids (asteroids with “moons”), almost as many as have been discovered prior. Astronomers expect binary asteroids be commonplace, based on studies of examples to date and computer modeling. However, asteroids are so numerous, and Gaia’s capabilities are so great, that many more binary asteroid systems are out there, awaiting discovery. For more on the topic, see: https://phys.org/news/2024-08-gaia-moons-hundreds-asteroids.html.
OTHER ASTRONOMY NEWS
Giant Magellan Telescope News: The Richard F. Caris Mirror Lab at the University of Arizona began the four-year manufacturing process for the seventh and final main mirror for the GMT last September. The other six mirrors have already been completed. The telescope will be sited at Las Campanas Observatory in Chile. The site preparation is pretty much complete, work on the telescope structure is underway, and the building that will enclose the telescope just passed its final design review. When completed, the 65-meter tall, 5,000 metric ton enclosure will be one of the largest mechanized buildings ever constructed. It will be capable of a full rotation in only four minutes. The GMT is being built by a consortium of 14 universities and research institutions, one of which is the Harvard-Smithsonian Center for Astrophysics. Design, construction, and testing work is generating hundreds of jobs in 36 different States. However …
There is a problem with funding the GMT. The National Science Board is a panel of scientists that oversees the National Science Foundation and its funding for large-scale science projects. They met on February 22, and among other things, decided to cap NSF’s support for its Extremely Large Telescope Program at $1.6B (not to be confused with the European Southern Observatory’s Extremely Large Telescope now building on Chile’s Cerro Amazones). The cap will prevent NSF from fully-funding both the Giant Magellan Telescope in Chile and the Thirty Meter Telescope in Hawaii as originally planned, and the NSB is requiring NSF to make a tough decision on the matter by May.
Both affected telescopes are presently under construction and have already received considerable funding. They joined forces in 2018, offering NSF an opportunity for American astronomers to have access to coverage of the entire sky in exchange for public support. The National Academy of Science’s 2020 Decadal Survey in Astrophysics prioritized the pair the highest among other ground-based astronomy projects, and the NSF approved preliminary design reviews early last year. Six of the seven main mirrors for the GMT have been finished, and the observatory site for them has been prepared. The TMT is less far along, in part due to opposition by native Hawaiians to another, larger, dome atop Mauna Kea. The TMT has one advantage, and that its location will provide coverage of the entire sky, if data are shared with ESO’s Extremely Large Telescope. That’s an Extremely Large “if.”
Telescopes of the size now under construction cost more than the NSF is used to. The GMT has a $2.54B price tag, of which only $850M has been pledged by other project sponsors. The TMT is even more expensive, $3.6B, of which about $2B has been pledged by its partners. Funding both as much as NSF can afford risks loss/delays in both, and would consume more than three-quarters of the NSF telescope funding program, which has many other responsibilities. Funding only one wastes money already spent on the other. For more on this dilemma, see: https://www.science.org/content/article/nsf-board-approves-funding-just-one-two-proposed-giant-telescopes.
The telescopes in question are really huge, on the order of the size of a tennis court. If you want to see a good comparison of their sizes relative to other telescopes (and familiar objects to scale), and find out more about astronomy in Chile, see: https://www.airandspacethisweek.com/assets/pdfs/20240122%20Astronomy%20in%20Chile.pdf.
UPDATE: I came across a March 7 analysis of the NSF telescope funding situation on the “Big Think” website a while back. The authors demonstrate that while the need to make the reduction is arguably due to the lack of Congressional support is understandable, many of the reasons put forth to justify the funding reduction are not accurate. The National Board’s assessment of the need for both telescopes is still sound. As the BT authors point out, “Once you stop investing in something important to your nation, that field almost never recovers in that country,” and cite the diminished role for the U.S. in high-energy particle physics research due to the abandonment of the Superconducting Super Collider a few decades ago. It’s a thought-provoking piece; see it for yourself at: https://bigthink.com/starts-with-a-bang/future-astronomy-dimmed-by-half.
The Presidential Budget Request for FY 2025 provides for the completion of only one of the two extremely-large telescopes presently under construction.
The NSF was supposed to deliver its funding plan for the U.S. Extremely Large Telescope Program by May, 2024. That did not happen. It is now September. The most recent item I could find on this issue was dated May 24, 2024; see: https://www.science.org/content/article/nsf-wrestles-dilemma-over-dueling-giant-telescopes.
ASTRONOMY IN CHILE
But Some Good News, Too, from Chile: Phys.org recently posted a piece about the Vera Rubin Observatory and how it will help astronomers find “weird and wonderful things happening in the Solar System.” There’s a lot of info about the VRO, its Simonyi Telescope, and giant camera, and the piece is built around a recent preprint paper in The Astronomical Journal. The summary makes for interesting reading; see here: https://phys.org/news/2024-01-vera-rubin-weird-solar.html and the AJ paper is accessible here: https://arxiv.org/abs/2401.08763.
More: Another Phys.org item points out the value of the VRO’s ability to image the entire available night-time sky every few days, allowing a search for all sorts of transient objects, either those changing rapidly in brightness, or those changing in location. The latter could include “InterStellar Objects” (ISOs), such as the surprise visits by Oumuamua and Borisov, and many more Near Earth Objects. Some researchers predict as many as 70 new ISOs could be discovered annually when VRO comes on line. This article gives a lot of food for thought, and will likely appeal to the general public. See it at: https://phys.org/news/2024-02-vera-rubin-keen-eye-solar.html.
Still More: Score one for the ALMA radio telescope complex in Chile! Cerro Tololo, the VRO, et. al. are not the only observatories making news in the Andes. Quasars are compact yet extremely energetic objects, where a super-massive black hole in a galactic center generates enormous amounts of energy. They are extremely distant and formed very early after the Big Bang. Astronomical models of quasars predict that they would eject large quantities of molecular gases, the “fuel” for star formation. If the ejection rate is too high, the galaxies containing the quasar have fewer new stars forming that would be the case if all of the ejected gases were incorporated into star formation. ALMA data provide observational evidence for gas outflow; additional work is being done to determine how effective star formation is in utilizing it. For a summary of this research, see here; for the paper in The Astrophysical Journal, see here.
More ALMA: Recent observations of galaxy NGC 253 with the ALMA radio telescope array has revealed the presence of over 100 different molecule species. NGC 253, in Sculptor, is ~10,000 light-years distant, and has more vigorous star formation than is present in our Milky Way. The 100 different molecules detected there is more than double the number of molecular species have been seen in any other galaxy. For more info, see: https://phys.org/news/2024-03-alma-molecular-signposts-starburst-galaxy.html.
Follow up to the Astronomy in Chile Item of the Week: The June, 2024, issue of Sky & Telescope magazine has two major articles about astronomy in Chile. One is about Walter Baade, who is the namesake for one of the Twin Magellan Telescopes at Las Campanas Observatory. The other is about the Vera Rubin Observatory and its Simonyi Telescope atop Cerro Pachón. Baade earned the prestigious Bruce Medal in 1955 for his work on supernovae and how they could produce cosmic rays and neutron stars; the article in S&T is on pages 28-33. The Simonyi Telescope is not the largest in Chile by any means, but it will be paired with the Legacy Survey of Space and Time (LSST) camera, whose 25-inch diameter focal plane is covered by 189 CCDs of 16 million pixels each! It’s by far the largest digital camera ever built, and will image of the entire sky visible to it, at high resolution, every week. The data will be made available to anyone who wants to use it, enabling a remarkable transformation in how astronomy will be done in the future. For more about it, see pages 34-40.
OTHER ASTRONOMY NEWS
We Are Star Stuff: Prevailing thought about post-Big Bang neucleosynthesis holds that elements heavier than helium were created by fusion process within stars, at least up to iron. Fusion reactions involving iron and above are endothermic, requiring a lot of energy to produce. The only logical energy source for those reactions comes when that particular star goes super-nova. OK, but why do we see evidence of a higher quantity of heavier-than-iron elements than we would expect from supernovae?
In the last decade, we have learned more about another mechanism that may be capable of creating heavy elements, via the detection of gamma-ray bursts. Two types of GRBs have been observed, “long” and “short.” Long GRBs are likely caused by the death of massive, fast-rotating stars, where the rotation ejects material into narrow, fast-moving jets of gamma rays. Short GRBs are thought to be the flash formed by the collision of two neutron stars. Such a collision is capable of not only spewing gamma rays, the resulting explosion can actually send detectable gravitational waves in our direction. The energy from a GRB could conceivably be capable of fusing heavier elements. One such event has been observed, in August, 2017. Earth-bound gravity detectors detected the signal of an impending collision of neutron stars, and a few seconds later, a significant GRB was detected from the same spot in the sky. The spot was monitored by a number of instruments, and within a few weeks revealed that a “kilonova” explosion, big but smaller than a full-blown supernova. A large amount of heavy elements was observed, too.
There is a problem with both hypotheses. Neutron star-neutron star collisions are very rare, and even if each produced heavy elements, there aren’t enough such collisions to produce the quantities of heavy elements we observe.
What about long GRBs? On October 9, 2022, the biggest long GRB ever seen occurred. Detailed observations of the site of the GRB’s origin showed no concentration of heavy elements, so long GRBs cannot be the energy source for the creation of heavy elements, either.
Back to the Hypothesis Drawing Board!
For more on this issue, see: https://phys.org/news/2024-05-universe-biggest-explosions-elements-mystery.html.
Hunting for the “First Stars” Immediately after the Big Bang, there were large amounts of hydrogen and helium suffusing Space. The first stars, so-called “Population III,” began forming almost immediately, really big ones. Intense fusion processes deep within them formed many of the heavier-than-helium atoms around us. The initial and final chemistry of these behemoths would reveal much about the earliest days of the Universe. But finding them is difficult. Along with the Population III stars, a large number of black holes formed, too. Astronomers hypothesize that when a Pop III star gets close to a black hole, it suffers a “tidal disruption event,” meaning it is torn apart by the black hole’s intense gravity, which produces an incredibly-bright flare. Since the distance to the disruption site is huge, the light from it is strongly red-shifted into the IR, and the spectral lines seen give clues as to the composition the disrupted star. For a summary of this work, see here; for the paper in The Astrophysical Journal Letters, see here.
Fingerprints of Iron: The Japanese XRISM satellite observatory has acquired X-ray spectral data from the area around active-center galaxy NGC 4151, 43 million light-years away. The galaxy has a giant black hole at its center, 20 million times more massive than the Sun. Gas and dust falling into the black hole releases huge amounts of energy, much of it at X-ray wavelengths, which XRISM was designed for. The X-rays cause the inrushing material to fluoresce, and the wavelengths of the resulting spectral lines reveal the chemistry of the gas. One such wavelength indicates the presence of iron. XRISM website: https://www.xrism.jaxa.jp/en; summary of study: https://www.sciencedaily.com/releases/2024/05/240508113126.htm; NASA: https://science.nasa.gov/missions/xrism/nasa-jaxa-xrism-spots-iron-fingerprints-in-nearby-active-galaxy.
Hungry White Dwarfs are Sloppy Eaters: The vast majority of stars in our galaxy either are white dwarfs, or will end up as one near the end of their “lives.” Spectral analysis of the light from many of them shows the presence of elements heavier than should be on their surfaces. Such “pollution” is most likely to come from the accretion of planetesimals rich in “metals” (any element heavier than helium to astronomers). Detailed computer simulations of material in orbit around a forming white dwarf show that such accretion will likely continue for an extended period. For a summary of this work, see https://phys.org/news/2024-05-hungry-white-dwarfs-puzzle-stellar.html.
Big Bad Black Holes Blow Bigly: Data from the JWST lead to a hypothesis that the formation of super-massive black holes in the earliest giant galaxies shut off the formation of new stars within them. The data show that the galactic version of “solar wind” is made up mostly of neutral gas, not detectable before the JWST. The neutral gas was the fuel for new star creation; when much of it was blown out of the galaxy, star formation slowed/stopped. For a summary of this work, see here; for the abstract of the paper in Nature, see here.
Funding woes for the Chandra X-ray Observatory: “NASA's budget for 2025 and projections forward foresee a steep reduction in funding for Chandra. This change would also slash support for research projects in X-ray astronomy, especially in the U.S.” While it is true that Chandra’s instruments are showing their age a bit, the satellite has a lot more operational life left; if the present budget cuts hold then Chandra will begin a three-year slowdown/shutdown. For more, see: https://skyandtelescope.org/astronomy-news/an-early-end-for-the-chandra-x-ray-observatory.
[The JWST and M-1: The Crab Nebula in Taurus is a favorite of backyard astronomers. It was one of the first supernova remnants discovered and identified as such. The Anasazi at Chaco Canyon were so impressed by the 1054 CE supernova that made it that they recorded the event in a petroglyph (still extant but very highly protected!). The HST, not long after its deployment, returned a beautiful visible-light photo of it in 2015. Now it’s JWST’s turn, and it sent back an infrared image of the Crab that is allowing astronomers to identify different supernova-related elements and learn more about the supernova that created it. For more info, see: https://www.jpl.nasa.gov/news/the-crab-nebula-seen-in-new-light-by-nasas-webb.
UPDATE: There is an image of M-1 in the Chandra budget item above that combines visible-light data from the HST, IR data from Spitzer, and X-ray data from Chandra; it’s quite spectacular! See for yourself at: https://skyandtelescope.org/astronomy-news/an-early-end-for-the-chandra-x-ray-observatory.]
Is the Sun’s 11-year Activity Peak Coming Early? The Sun’s 11-year cycle of activity is well-known, with the next maximum expected in mid-2025. But there are some indications that the peak may come earlier than usual this time around. Since solar activity can play hob with satellites, power transmission systems, and other technological infrastructure, having a good handle on its timing and severity ahead of time is crucial. For more on this issue, see: https://phys.org/news/2023-10-sun-peak-earlyknowing-secrets-star.html.
Without Infrastructure, Little is Possible: A truism in many contexts, including astronomy. For example, images from the James Webb Space Telescope dazzle professional astronomers and the public alike. The really-complex-yet-extremely-successful satellite is a marvel of engineering design and construction (as only NASA can!). But JWST would be of no value without the supporting infrastructure here on Earth that receives the information from its instruments.
Downlinks of data are always of paramount importance, but communicating with satellites in LEO or Geosynchronous orbit is simple compared with receiving data from JWST, which orbits the Sun-Earth L2 point, a million miles away. NASA’s Deep Space Network, originally built 60 years ago to ensure continuous radio contact with early manned spacecraft, is still up to the task! Although I’d bet that the electronics of their receivers and transmitters may have had an upgrade or two over the decades!
The DSN is an engineering marvel. For a summary, see here; for the DSN website, see here; and if you want to see whose signal the DSN is receiving, see here.
TWSftUoTtCBDftSoTiFoOT
The World Society for the Understanding of Things that Can Be Understood from the Study of Things in Front of Other Things says: An astonishing amount of Science can be conducted via the Study of Things in Front of Other Things! Examples range from the confirmation of Relativity by observations made during a total solar eclipse to asteroid shapes to rings around Uranus to planets of other Suns. Since many exoplanets have been discovered when they were “in front of other things,” all exoplanet and SETI news and info will be covered in the section below.
A Primer in Transits: NASA posted an introductory piece to the TWSFTUOTTCBDFTSOTIFOOT favorite of planetary transits here. Detecting the small drop in light from a star when its exoplanet transits across its face is one of the primary means of detecting exoplanets, enabled by ground-based observation and satellites like Kepler and TESS. While the transit method has produced many exoplanet findings, but other methods are useful, too (see immediately below).
Confirmed Exoplanets: Now 5,502! Over 31 years ago, the first two confirmations of planets orbiting another star were made. It was a strange system, since they were both orbiting a pulsar! Now, the announcement of six new confirmations has pushed the total of definite exoplanets to 5,502. For of the new finds were made by the transit method, one by the radial velocity method, and one was made by direct observation.
Dangerous Red Dwarfs: The transit method of exoplanet discovery has a very strong detection bias toward larger planets very close to their suns; it would be essentially impossible to discover a stellar system like our own with Kepler or TESS. The bias is why most known exoplanets tend to be large and very close to smaller stars, such as red dwarfs. However, we have found some exoplanets in that close zone that are also in the temperature “Goldilocks Zone,” where water could persist as a liquid for at least part of its orbit. Some red dwarfs are known to produce high-UV stellar flares that could damage life on any exoplanet, but the percentage of those red dwarfs that are dangerous to life was thought to be fairly low, giving better chances for extraterrestrial life.
The mission of the decommissioned GALEX Space Telescope was to observe the entire sky at near- and far-UV wavelengths; it was operational from 2003 to 2013. New computational capabilities and techniques allowed a team of researchers to search for stellar UV flares from “thousands and thousands” of relatively close red dwarfs. Alas, such flares were more common and more powerful than previously thought. For a summary of this report, see here; for the paper in the Monthly Notices of the Royal Astronomical Society, see here.
Nearby Exoplanet with Oceans? Astronomers first detected exoplanet LHS 1140 b in 2017. It’s a “mere” 48 light-years from Earth, but it is particular interest because it lies in the “Goldilocks Zone” around its star, where temperatures are such that water could be liquid at least part of its “year.” LHS 1140 b was originally thought to be one of the “mini-Neptune” class of exoplanets. However, recent JWST data show it to be a “super-Earth,” 1.7x Earth’s size and 5.6x its mass. But wait, there’s more. JWST transit observations show no hydrogen or helium in its atmosphere, consistent with the “super-Earth” designation, but those data also show that LHS 1140 b has a LOT of water, perhaps as much as 10-20% of its total mass! Additional JWST observations will be required to assess the state of water on this interesting exoplanet. For more information, see: https://phys.org/news/2024-07-nearby-exoplanet-ocean-world-webb.html. For the draft version of the paper for publication in The Astrophysical Journal Letters, see: https://arxiv.org/pdf/2406.15136.
I’ll Keep My Atmosphere, Thank You Very Much: Most exoplanets found very close to their stars have had the atmospheres stripped away by intense radiation from their star. But not all. Astronomers recently found an exoplanet with an atmosphere in spite of orbiting close to its red giant star. They nicknamed it “Phoenix,” a nod to its ability to “survive the fire.”
“Because of Phoenix's age and scorching temperatures, coupled with its unexpectedly low density, the process of stripping its atmosphere must have occurred at a slower pace than scientists thought possible, the scientists concluded. They also estimated that the planet is 60 times less dense than the densest "hot Neptune" discovered to date, and that it won't survive more than 100 million years before it begins dying by spiraling into its giant star.” For more on the quote and additional info on this weird “hot Neptune,” see here.
Gliese 12 b, An Exo-Venus: Japanese astronomers have found an exoplanet only 40 light-years from Earth that is similar in size and stellar heating as Venus. Its sun, Gliese 12, is a red dwarf, and the newly-discovered exoplanet orbits it every 12.8 Earth days. Gliese 12 is about a quarter of the size of the Sun, and has a much cooler surface temperature, which would indicate that Gliese 12 b would have a surface temperature in the “Goldilocks Zone.” The discovery made the news last month, and the results, summarized here, were published in The Astrophysical Journal Letters (here) and the Monthly Notices of the Royal Astronomical Society.
SPECULOOsions About a Nearby Planet and Its Ultra-cool Star: No, this is not yet another example of a Spell-Check error, rather it is about a news item from the Search for Planets EClipsing ULtra-cOOl stars Project. Jupiter needs just a bit more mass before its internal gravity is enough to initiate fusion. An Ultra-Cool star is one that has just a bit more mass than the absolute minimum to initiate fusion, making them the least-massive class of stars. One of them, located 55 light-years from Earth, has been found to have an Earth-sized exoplanet so close to its star that its year is only 17 hours long. The exoplanet gets about 16x the heating the Earth receives, in spite of its star’s dimness. This is only the second planetary system found to date around an ultra-cool star, but such stars “represent a significant fraction of the planetary population in the Milky Way,” so learning more about them is important. For a summary of this discovery, see: https://www.sciencedaily.com/releases/2024/05/240515122831.htm.
Search for Brown Dwarfs, Our “Cool Neighbors”: Ultra-cool stars (above) are the least-massive stars, just barely large enough to initiate hydrogen fusion in their cores. Brown dwarfs are bodies that were almost, but not quite, large enough to initiate fusion. The give off some radiation, mostly in the IR, due to internal heat left over from their formation, but so little that it makes them hard to find, even though they should be commonplace. Knowing more about them would inform models of star formation. Examination of the brown dwarfs discovered to date so them to contain water and methane, suggesting a kinship with exoplanets. Detailed examination of as many brown dwarfs as possible could give more insight into the formation of exoplanets and the spectrum of astronomical objects from stars to independent planets (those that don’t orbit stars).
YOU can help astronomers search for brown dwarfs from the comfort of your own home. Find out more about it in the Citizen Science section below!
Volcanic Exoplanet: HD 104067 is a star system 66 light-years from Earth. The first-known planet in the system is a “super-Earth,” and recent analysis of TESS and other data have revealed two additional exoplanets there. The geometry of the Super-Earth’s orbit is distorted by the gravity of the other two, and the ellipticity so induced causes the Super-Earth to flex, generating considerable heat (the same is true for Jupiter’s moon, Io). Calculations suggest that the heating would cause widespread volcanic activity and a surface temperature above 2000 K. For more on this Klingon pleasure planet, see: https://www.sciencedaily.com/releases/2024/05/240509155528.htm.
Hell-Planet Atmosphere: 55 Cancri is a small star 41 light-years from Earth. One of its planets, 55 Cancri e, orbits only 1.4 million miles from its star, making its surface temperature extremely hot. It’s classed as a “Super Earth,” and there is a debate over whether or not it has an atmosphere, and if so, its composition. Some data from the Spitzer Space Telescope indicated a lot of volatiles in its atmosphere, but at the high temperature likely there the only gas would be vaporized rocks. However, recent results from the JWST indicate the surface temperature of 55 Cancri e is hot, but not as hot a previously thought, and it appears that some heat is taken to the night side of the exoplanet, suggesting a volatile-rich atmosphere. Also likely is that the exoplanet is covered by a “bubbling magma ocean.” For more info, see here, and DO NOT fall for the scam that it’s a nice place for a vacation home!
Could Evidence of Life Elsewhere Be Detected by the Europa Clipper? We know that several of the bodies in the outer Solar system have extensive, even global, liquid oceans under their icy crust. The surfaces of two, Jupiter’s Europa and Saturn’s Enceladus, have surfaces that in part resemble fractured pack ice on Earth. Some of Enceladus’ surface cracks are spewing a geyser of liquid, mostly water, from below, the droplets of water quickly freeing. The Cassini spacecraft, near the end of its operational life, was directed to fly through on such plume. Its instruments showed the water had a chemistry similar to that on Earth around a deep-water hot spring; all known such springs on Earth harbor a number of environment-specific life forms.
A recent study of how effective the Europa Clipper’s imaging system would be if it targeted a geyser plume in detecting biological chemistry in its component ice crystals. Experiments show a bio signature could be detected if even only 0.1% of the crystals imaged contained the bio material. For a summary of this interesting possibility, see: https://www.sciencedaily.com/releases/2024/03/240322145406.htm, and for the paper itself in Science Advances, see: https://www.science.org/doi/10.1126/sciadv.adl0849.
SEARCH FOR HABITABLE EXOPLANETS
Habitable Worlds Observatory: Yes, Virginia, there will be such a thing in the future. The 2020 Astronomy Decadal Survey strongly recommended that NASA “develop a 6-meter Space telescope capable of high-contrast observations in optical, infra-red, and ultraviolet wavelengths.” Its primary mission will be to examine 25 different exoplanets in detail, all in their star’s “Goldilocks Zone,” searching for biosignatures. Knowing which stars to choose is obviously of great importance. That work is presently underway; NASA’s Exoplanet Exploration Program has developed a list of 164 candidates to date, based on five selection criteria: stellar composition, photometric values, flare rate, variability, and potentially-sterilizing X-ray emissions. For more information on this project, see: https://phys.org/news/2024-01-astronomers-habitable-worlds-observatory.html and https://science.nasa.gov/astrophysics/programs/habitable-worlds-observatory.
SEARCH FOR INTELLIGENT LIFE ELSEWHERE
Part 1: UCLA’s Jean-Luc Margot is the founder of UCLA SETI’s “Are We Alone in the Universe?” project. Their mission is to detect “technosignatures by searching individual systems. Dr. Margot teaches a graduate course in SETI, and he had his students use TESS data for the closer known exoplanets to narrow the search for such emissions in great detail. No provable technosignatures were seen. Even though the smally sample observed didn’t show emissions, the skills developed by the students (e.g. signal processing, telecommunications, and statistics and other data analysis tools) will no doubt improve their academic success.
Part 2: Traditional SETI tactics, like Dr. Margot’s project, is one way to search. The Breakthrough Listen program (which uses citizen scientists) takes a different approach. Rather than look at relatively-close systems, they are using the Green Bank (West Virginia) and Parkes Murriyang radio telescopes to look for very high powered technosignatures, an entire galaxy at a time. For more on this program and strategy, see: https://phys.org/news/2023-12-breakthrough-scans-entire-galaxies-extremely.html.
Part 3: NASA has produced a six-part on-line series on how it is searching for life in the cosmos. If you are interested in the real science behind this topic, then check out these episodes! Part 1: Beginnings: Life on Our World and Others; Part 2: Life on Other Planets: What is Life and What Does It Need?; Part 3: The Hunt for Life on Mars – and Elsewhere in the Solar System; Part 4: “Life” in the Lab; Part 5: Searching for Signs of Intelligent Life: Technosignatures (see also this week’s Gravity Assist entry in the Solar System section); and Part 6: Finding Life Beyond Earth: What Comes Next?
What Happens After We Discover Life Elsewhere? Mary Voytek, Director of NASA’s Astrobiology Program, has some interesting thoughts on the subject. Check them out at: https://exoplanets.nasa.gov/news/1766/finding-life-beyond-earth-what-comes-next!
Exoplanet Travel Bureau is NASA’s source for whimsical travel posters showcasing various exoplanets as tourist destinations and other exoplanet information. See: https://exoplanets.nasa.gov/alien-worlds/exoplanet-travel-bureau!