Friday, November 29, 2024

4626 - HUBBLE - discoveries other galaxies?

 

-  4626  -   HUBBLE  -  discoveries other galaxies?  It's been 100 years since we learned the Milky Way is not the only galaxy.   On Sunday November 23, 1924, 100 years ago this month, readers perusing page six of the New York Times would have found an intriguing article, amid several large adverts for fur coats. The headline read: Finds Spiral Nebulae are Stellar Systems: "Dr. Hubbell Confirms View That They Are 'Island Universes'; Similar to Our Own."


------------------------------------------   4626  -   HUBBLE  -  discoveries other galaxies?

-

-   The American astronomer at the center of the article, Dr. Edwin Powell Hubble, was probably bemused by the misspelling of his name. But the story detailed a groundbreaking discovery: Hubble had found that two spiral-shaped nebulae, objects made up of gas and stars, which were previously thought to reside within our Milky Way galaxy, were located outside it.

-

-    These objects were actually the Andromeda and Messier 33 galaxies, the closest large galaxies to our Milky Way. Today, up to several trillion galaxies are estimated to fill the universe, based on observations of tens of millions of galaxies.

-

-    Four years before Hubble's announcement, an event called "the great debate" had taken place in Washington DC between the American astronomers Harlow Shapley and Heber Curtis. Shapley had recently shown the Milky Way to be larger than previously measured. Shapley argued that it could accommodate spiral nebulae within it. Curtis, on the other hand, advocated for the existence of galaxies beyond the Milky Way.

-

-    In hindsight, and ignoring certain details, Curtis won the debate. However, the method Shapley used to measure distances across the Milky Way was critical to Hubble's discovery, and was inherited from the work of a pioneering US astronomer: Henrietta Swan Leavitt.

-

-   In 1893, a young Leavitt was hired as a "computer" to analyze images from telescope observations at Harvard College Observatory, Massachusetts. Leavitt studied photographic plates from telescope observations of another galaxy called the Small Magellanic Cloud carried out by other observatory researchers.

-

-    Leavitt was searching for stars whose brightness changed over time. From over a thousand variable (changing) stars, she identified 25 were of a type known as Cepheids, publishing the results in 1912.

-

-   The brightness of Cepheid stars changes with time, so they appear to pulse. Leavitt found a consistent relationship: Cepheids that pulsed more slowly were intrinsically brighter (more luminous) than those pulsing more quickly. This was named the "period-luminosity relationship."

-

-    Other astronomers realized the significance of Leavitt's work: the relationship could be used to work out distances to stars. While a student at Princeton University, Shapley used the period-luminosity relationship to estimate distances to other Cepheids across the Milky Way. This is how Shapley reached his estimate for our galaxy's size.

-

-       But, in order for astronomers to be sure about distances within our galaxy, they needed a more direct way to measure distances to Cepheids. The stellar parallax method is another way to measure cosmic distances, but it only works for nearby stars. As the Earth orbits the sun, a nearby star appears to move relative to more distant background stars. This apparent motion is known as “stellar parallax”. Through the angle of this parallax, astronomers can work out a star's distance from Earth.

-

-    The Danish researcher Ejnar Hertzsprung used stellar parallax to obtain the distances to a handful of nearby Cepheid stars, helping calibrate Leavitt's work.   Telescope size is generally assessed by the diameter of the primary mirror. With a 100-inch (2.5-meter) diameter mirror for collecting light, the Hooker telescope at Mount Wilson was the largest telescope at the time.

-

-   Large telescopes are not only more sensitive to resolving galaxies, but also create sharper images. Edwin Hubble was therefore well placed to make his discovery. When Hubble compared his photographic plates taken using the 100 inch telescope with those taken on previous nights by other astronomers, he was thrilled to see one bright star appear to change in brightness over time, as expected for a Cepheid.

-

-    Using Leavitt's calculations, Hubble found that the distance to his Cepheid exceeded Shapley's size for the Milky Way. Over subsequent months, Hubble examined other spiral nebulae as he searched for more Cepheids with which to measure distances.

-

-    Word of Hubble's observations was spreading among astronomers. At Harvard, Shapley received a letter from Hubble detailing the discovery. He handed it to fellow astronomer Cecilia Payne-Gaposchkin, remarking: "Here is the letter that has destroyed my universe."

-

-    Besides estimating the distance to a galaxy, telescopes can also measure the speed at which a galaxy moves towards or away from Earth. In order to do this, astronomers measure a galaxy's spectrum: the different wavelengths of light coming from it. They also calculate an effect known as the Doppler shift and apply it to that spectrum.

-

-   The Doppler shift occurs for both light and sound waves; it is responsible for the pitch of a siren increasing as an emergency vehicle approaches, then decreasing as it passes you. When a galaxy is moving away from Earth, features of the spectrum known as absorption lines have longer measured wavelengths than they would if they were not moving. This is due to the Doppler shift, and we say that these galaxies have been "redshifted."

-

-    Beginning in 1904, the American astronomer Vesto Slipher used the Doppler technique with a 24-inch telescope at the Lowell Observatory in Flagstaff, Arizona. He found that nebulae, including Andromeda, were all redshifted. Slipher found they were moving away from Earth at speeds as high as a thousand kilometers a second.

-

-   Hubble combined Slipher's measurements with his distance estimates for each galaxy and discovered a relationship: the further a galaxy is from us, the faster it is moving away from us. This can be explained by the expansion of the universe from a common origin, which would become known as the “Big Bang”.

-

-   The announcement 100 years ago cemented Hubble's place in the history of astronomy. His name would later be used for one of the most powerful scientific instruments ever created: the Hubble space telescope. It seems incredible how, over the course of just five years, our understanding of the universe was brought into focus.

-

-

November 29, 2024           HUBBLE  -  discoveries other galaxies?             4626

------------------------------------------------------------------------------------------                                                                                                                       

--------  Comments appreciated and Pass it on to whomever is interested. ---

---   Some reviews are at:  --------------     http://jdetrick.blogspot.com ----- 

--  email feedback, corrections, request for copies or Index of all reviews

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Friday, November 29, 2024  ---------------------------------

 

 

 

 

 

           

 

 

Wednesday, November 27, 2024

4625 - MARS - are there signs of life?

 

-  4625  -  MARS  -  are there signs of life?  -    On Earth, these types of features in rocks are often associated with the fossilized record of microbes living in the subsurface.   NASA's Perseverance rover may have found signs of ancient life in a rock on Mars.



--------------------------------------   4625  -   MARS  -  are there signs of life?

-   See Review 4624 “Mars had water at one time” .  This Review asks, “What about life?” Perseverance Mars rover finds possible signs of ancient Red Planet life

-

-    The rover has come across an intriguing, arrowhead-shaped rock that hosts chemical signatures and structures that could have been formed by microbial life billions of years ago, when Mars was significantly wetter than it is today.

-

-    Inside the rock, which scientists have nicknamed "Cheyava Falls," Perseverance's instruments detected organic compounds, which are precursors to the chemistry of life as we know it. Wisping through the length of the rock are veins of calcium sulfate, which are mineral deposits that suggest water, also essential for life, once ran through the rock.

-

-    The rover also found dozens of millimeter-sized splotches, each surrounded by a black ring and mimicking the appearance of leopard spots. These rings contain iron and phosphate, which are also seen on Earth as a result of microbe-led chemical reactions.

-

-    These spots are a big surprise.   On Earth, these types of features in rocks are often associated with the fossilized record of microbes living in the subsurface.    Cheyava Falls sits at the edge of an ancient, 400-meter-wide river valley named Neretva Vallis. Scientists suspect this ancient channel was carved out long ago due to water gushing into Jezero Crater; Neretva Vallis runs along the inner wall of this region.

-

-    In one possible scenario, mud that already possessed organic compounds got dumped into the valley and later cemented into the Cheyava Falls rock, which Perseverance sampled on July 21, 2024. A second episode of water oozing into the formed rock would have created the object's calcium sulfate veins and black-ringed spots the team sees today.

-

-    The rock's visible features aren’t irrefutable evidence of ancient microbial life on Mars. It is possible that the observed calcium sulfate entered the rock at uninhabitably high temperatures, perhaps during a nearby volcanic event. However, whether such non-biological chemical reactions could have resulted in the observed black-ringed spots is an open question.

-

-    This trip through the Neretva Vallis riverbed paid off as we found something we've never seen before, which will give our scientists so much to study.   We have zapped that rock with lasers and X-rays and imaged it literally day and night from just about every angle imaginable.

-

-    To fully grasp what really unfolded in the ancient river valley billions of years ago, scientists are keen to get the Cheyava Falls sample to Earth, where it can be scrutinized with powerful instruments that Perseverance’s limited suite doesn't have.

-

-   The complex “Mars Sample Return” effort, however, has run into many snags in recent months after its costs spiked to $11 billion. In its current form, the program requires multiple launches to Mars to place a vehicle on the Red Planet, after which either Perseverance will travel to the vehicle and drop off its collected samples, or pop those samples over to a retrieval helicopter that can complete the handoff. Then, an ascender would launch the samples into orbit, where a spacecraft would collect them and return them to Earth.

-

-

November 26, 2024          MARS  -  are there signs of life?                  4625

------------------------------------------------------------------------------------------                                                                                                                       

--------  Comments appreciated and Pass it on to whomever is interested. ---

---   Some reviews are at:  --------------     http://jdetrick.blogspot.com ----- 

--  email feedback, corrections, request for copies or Index of all reviews

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Wednesday, November 27, 2024  ---------------------------------

 

 

 

 

 

           

 

 

4624 - MARS - had water at one time?

 

-  4624 -  MARS  -  had water at one time?     A  4.45 billion-year-old crystal from Mars reveals the planet had water from the beginning.   Water is ubiquitous on Earth, about 70% of Earth's surface is covered by water. Water is in the air, on the surface and inside rocks. Geologic evidence suggests water has been stable on Earth since about 4.3 billion years ago.


-------------------------------------   4624  -    MARS  -  had water at one time?

-

-    The history of water on early Mars is less certain. Determining when water first appeared, where and for how long, are all burning questions that drive Mars exploration. If Mars was once habitable, some amount of water was required.

-

-   We studied the mineral zircon in a meteorite from Mars and found evidence that water was present when the zircon crystal formed 4.45 billion years ago.   This may represent the oldest evidence for water on Mars.

-

-    Water has long been recognized to have played an important role in early Martian history. Like Earth, Mars formed about 4.5 billion years ago. The history of Mars has four geological periods. These are the Amazonian (from today back to 3 billion years), the Hesperian (3 billion to 3.7 billion years ago), the “Noachian” (3.7 billion to 4.1 billion years ago) and the Pre-Noachian (4.1 billion to about 4.5 billion years ago).

-

-    Evidence for water on Mars was first reported in the 1970s when NASA's Mariner 9 spacecraft captured images of river valleys on the Martian surface. Later orbital missions, including Mars Global Surveyor and Mars Express, detected the widespread presence of hydrated clay minerals on the surface. These would have needed water.

-

-   The Martian river valleys and clay minerals are mainly found in “Noachian terrains”, which cover about 45% of Mars. In addition, orbiters also found large flood channels, outflow channels, in Hesperian terrains. These suggest the short-lived presence of water on the surface, perhaps from groundwater release.

-

-   Most reports of water on Mars are in materials or terrains older than 3 billion years. More recently than that, there isn't much evidence for stable liquid water on Mars.   But what about during the Pre-Noachian? When did water first show up on Mars?

-

-   There are three ways to hunt for water on Mars. The first is using observations of the surface made by orbiting spacecraft. The second is using ground-based observations such as those taken by Mars rovers.   The third way is to study Martian meteorites that have landed on Earth.

-

-     The only Pre-Noachian material we have available to study directly is found in meteorites from Mars. A small number of all meteorites that have landed on Earth have come from our neighboring planet.   An even smaller subset of those meteorites, believed to have been ejected from Mars during a single asteroid impact, contain Pre-Noachian material.

-

-    “Black Beauty” is a famous Martian meteorite made up of broken-up surface material, or regolith. In addition to rock fragments, it contains zircons that formed from 4.48 billion to 4.43 billion years ago. These are the oldest pieces of Mars known.

-

-   While studying trace elements in one of these ancient zircons we found evidence of hydrothermal processes, meaning they were exposed to hot water when they formed in the distant past.

-

-    The zircon being studied is 4.45 billion years old. Within it, iron, aluminum and sodium are preserved in abundance patterns like concentric layers, similar to an onion.   This pattern, called oscillatory zoning, indicates that incorporation of these elements into the zircon occurred during its igneous history, in magma.

-

-   The problem is that iron, aluminum and sodium aren't normally found in crystalline igneous zircon.  How did these elements end up in the Martian zircon?   The answer is hot water.

-

-   In Earth rocks, finding zircon with growth zoning patterns for elements like iron, aluminum and sodium is rare. One of the only places where it has been described is from “Olympic Dam” in South Australia, a giant copper, uranium and gold deposit.

-

-    The metals in places like Olympic Dam were concentrated by hydrothermal (hot water) systems moving through rocks during magmatism.   Hydrothermal systems form anywhere that hot water, heated by volcanic plumbing systems, moves through rocks. Spectacular geysers at places like Yellowstone National Park in the United States form when hydrothermal water erupts at Earth's surface.

-

-   Finding a hydrothermal Martian zircon raises the possibility of ore deposits forming on early Mars.   Previous studies have proposed a wet Pre-Noachian Mars. Unusual oxygen isotope ratios in a 4.43 billion-year-old Martian zircon were previously interpreted as evidence for an early hydrosphere.  Mars may have had an early global ocean 4.45 billion years ago.

-

-     Magmatic hydrothermal systems were active during the early formation of Mars' crust 4.45 billion years ago.   It's not clear whether this means surface water was stable at this time. What is clear is that the crust of Mars, like Earth, had water shortly after it formed,  a necessary ingredient for habitability.

-

November 27, 2024         MARS  -  had water at one time?                4624

------------------------------------------------------------------------------------------                                                                                                                       

--------  Comments appreciated and Pass it on to whomever is interested. ---

---   Some reviews are at:  --------------     http://jdetrick.blogspot.com ----- 

--  email feedback, corrections, request for copies or Index of all reviews

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Wednesday, November 27, 2024  ---------------------------------

 

 

 

 

 

           

 

 

Monday, November 25, 2024

4623 - HISTORY OF THE MIKY WAY – discoveries by Hubble.

 

-  4623 -   HISTORY  OF  THE  MIKY  WAY – discoveries by Hubble,  -    It's been 100 years since we learned the Milky Way is not the only galaxy.  On Sunday November 23, 1924, 100 years ago this month, readers perusing page six of the New York Times would have found an intriguing article, amid several large adverts for fur coats.

-


------------   4623  -    HISTORY  OF  THE  MIKY  WAY – discoveries by Hubble.

-

-    The headline read: “Finds Spiral Nebulae are Stellar Systems”.   Confirms View That They Are 'Island Universes'; Similar to Our Own.   The story detailed a groundbreaking discovery: James Hubble had found that two spiral-shaped nebulae, objects made up of gas and stars, which were previously thought to reside within our Milky Way galaxy, were located outside it.

-

-   These objects were actually the Andromeda and Messier 33 galaxies, the closest large galaxies to our Milky Way. Today, up to several trillion galaxies are estimated to fill the universe, based on observations of tens of millions of galaxies.

-

-   Four years before Hubble's announcement, an event called "the great debate" had taken place in Washington DC between the American astronomers Harlow Shapley and Heber Curtis. Shapley had recently shown the Milky Way to be larger than previously measured. Shapley argued that it could accommodate spiral nebulae within it. Curtis, on the other hand, advocated for the existence of galaxies beyond the Milky Way.

-

-    In hindsight, and ignoring certain details, Curtis won the debate. However, the method Shapley used to measure distances across the Milky Way was critical to Hubble's discovery, and was inherited from the work of a pioneering US astronomer: Henrietta Swan Leavitt.

-

-   In 1893, a young Leavitt was hired as a "computer" to analyze images from telescope observations at Harvard College Observatory, Massachusetts. Leavitt studied photographic plates from telescope observations of another galaxy called the Small Magellanic Cloud.

-

-   Leavitt was searching for stars whose brightness changed over time. From over a thousand variable (changing) stars, she identified 25 were of a type known as “Cepheids”, publishing the results in 1912.

-

-    The brightness of Cepheid stars changes with time, so they appear to pulse. Leavitt found a consistent relationship: Cepheids that pulsed more slowly were intrinsically brighter (more luminous) than those pulsing more quickly. This was called the "period-luminosity relationship."

-

-   Other astronomers realized the significance of Leavitt's work: the relationship could be used to work out distances to stars. While a student at Princeton University, Shapley used the period-luminosity relationship to estimate distances to other Cepheids across the Milky Way. This is how Shapley reached his estimate for our galaxy's size.

-

-     But, in order for astronomers to be sure about distances within our galaxy, they needed a more direct way to measure distances to Cepheids. The stellar parallax method is another way to measure cosmic distances, but it only works for nearby stars. As the Earth orbits the sun, a nearby star appears to move relative to more distant background stars. This apparent motion is known as “stellar parallax”. Through the angle of this parallax, astronomers can work out a star's distance from Earth.

-

-   The Danish researcher Ejnar Hertzsprung used stellar parallax to obtain the distances to a handful of nearby Cepheid stars, helping calibrate Leavitt's work.  The New York Times article emphasized the "great" telescopes at the Mount Wilson Observatory near Los Angeles, where Hubble was working. Telescope size is generally assessed by the diameter of the primary mirror. With a 100-inch (2.5-meter) diameter mirror for collecting light, the Hooker telescope at Mount Wilson was the largest telescope at the time.

-

-    Large telescopes are not only more sensitive to resolving galaxies, but also create sharper images. Edwin Hubble was therefore well placed to make his discovery. When Hubble compared his photographic plates taken using the 100 inch telescope with those taken on previous nights by other astronomers, he was thrilled to see one bright star appear to change in brightness over time, as expected for a Cepheid.

-

-    Using Leavitt's calculations, Hubble found that the distance to his Cepheid exceeded Shapley's size for the Milky Way. Over subsequent months, Hubble examined other spiral nebulae as he searched for more Cepheids with which to measure distances.

-

-    Word of Hubble's observations was spreading among astronomers. At Harvard, Shapley received a letter from Hubble detailing the discovery. He handed it to fellow astronomer Cecilia Payne-Gaposchkin, remarking: "Here is the letter that has destroyed my universe."

-

-    Besides estimating the distance to a galaxy, telescopes can also measure the speed at which a galaxy moves towards or away from Earth. In order to do this, astronomers measure a galaxy's spectrum: the different wavelengths of light coming from it. They also calculate an effect known as the “Doppler shift” and apply it to that spectrum.

-

-   The Doppler shift occurs for both light and sound waves; it is responsible for the pitch of a siren increasing as an emergency vehicle approaches, then decreasing as it passes you. When a galaxy is moving away from Earth, features of the spectrum known as absorption lines have longer measured wavelengths than they would if they were not moving. This is due to the Doppler shift, and we say that these galaxies have been "redshifted."

-

-    Beginning in 1904, the American astronomer Vesto Slipher used the Doppler technique with a 24-inch telescope at the Lowell Observatory in Flagstaff, Arizona. He found that nebulae, including Andromeda, were all redshifted. Slipher found they were moving away from Earth at speeds as high as a thousand kilometers a second.

-

-   Hubble combined Slipher's measurements with his distance estimates for each galaxy and discovered a relationship: the further a galaxy is from us, the faster it is moving away from us. This can be explained by the expansion of the universe from a common origin, which would become known derisively as the “Big Bang”.

-

-   The announcement 100 years ago cemented Hubble's place in the history of astronomy. His name would later be used for one of the most powerful scientific instruments ever created: the Hubble space telescope. It seems incredible how, over the course of just five years, our understanding of the universe was brought into focus.

-

-

November 25, 2024         HISTORY  OF  THE  MILKY  WAY                       4623

------------------------------------------------------------------------------------------                                                                                                                       

--------  Comments appreciated and Pass it on to whomever is interested. ---

---   Some reviews are at:  --------------     http://jdetrick.blogspot.com ----- 

--  email feedback, corrections, request for copies or Index of all reviews

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Monday, November 25, 2024  ---------------------------------

 

 

 

 

 

           

 

 

4622 - MERCURY - new mysteries to discover?

 

-  4622 -  MERCURY  -  new mysteries to discover?  -     Spacecraft carrying European and Japanese probes passed closer to Mercury than originally planned overnight after thruster problems delayed the mission to study the little-known, sun-scorched planet.   The “BepiColombo mission” launched in 2018 on a winding path that had been intended to enter the orbit of the planet closest to the sun in December 2025.


---------------------------------   4622  -    MERCURY  -  new mysteries to discover?

-    In April, 2024,  a glitch with the spacecraft's thrusters sapped some of its power supply, forcing teams on the ground to change its trajectory and delaying its arrival until November 2026.  The new path meant the spacecraft needed to fly 22 miles closer to the planet than initially planned, passing just 165 kilometers above the surface, during its latest flyby.

-

-    This was the fourth of six planned flybys of Mercury on the mission's nine-billion-kilometer journey before it can finally settle into the planet's orbit.   Most of the time Mercury is closer to Earth than Mars.  The red planet can be reached by missions from Earth in just seven months.

-

-   Mercury is "the most difficult" planet for probes to reach.   The planet's relatively tiny mass, it is only slightly bigger than the moon, means its gravitational pull is extremely weak compared to the sun, making it tricky for satellites to stay in its orbit.  It takes much more energy to brake and stop at Mercury than to go to Mars.

-

-   This is where delicate maneuvers called Z”gravitational assists” come in. These slingshots around celestial bodies allow spacecraft to speed up, slow down, or change trajectory.  A glitch with the electric thrusters means the spacecraft is now operating with only 90 percent of its planned power supply.

-

-   After months spent investigating the problem, the thrusters will "remain operating below the minimum thrust required for an insertion into orbit around Mercury in December 202."

-

-  The new slower path means BepiColombo is now planned to enter orbit in November 2026.  NASA's Mariner 10 was the first probe to capture a close picture of its lunar-looking surface in 1974.  No spacecraft had orbited the planet until the MESSENGER probe arrived in 2011.

-

-    The NASA mission confirmed "some rather bizarre things.  One of these "oddities" is that Mercury is the only rocky planet other than Earth to have a magnetic field. Exactly how it has such a magnetic field so close to the sun is not fully understood.

-

-   Another "oddity" is that Mercury's iron core composes 60 percent of its mass, compared to only a third for Earth.  Mercury's surface is also marked by "hollows," which could suggest relatively recent geologic activity.

-

-    Also unclear is the composition of minerals on covering the planet's surface, which is blasted with intense radiation from the sun.

-

-  The spacecraft carries two separate satellites, one from the ESA and another from Japan's JAXA space agency, which have a total of 16 scientific instruments.

-

November 25, 2024        MERCURY  -  new mysteries to discover?         4622

------------------------------------------------------------------------------------------                                                                                                                       

--------  Comments appreciated and Pass it on to whomever is interested. ---

---   Some reviews are at:  --------------     http://jdetrick.blogspot.com ----- 

--  email feedback, corrections, request for copies or Index of all reviews

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Monday, November 25, 2024  ---------------------------------

 

 

 

 

 

           

 

 

4620 - REIONIZATION - in the early Universe?

 

-  4620 -  REIONIZATION  -  in the early Universe?  -    The James Webb telescope observations has shed new light on “Cosmic Reionization”.  The “Epoch of Reionization” was a critical period for cosmic evolution and has always fascinated and mystified astronomers. During this epoch, the first stars and galaxies formed and reionized the clouds of neutral hydrogen that permeated the Universe.



-------------------------------------   4620  -    REIONIZATION  -  in the early Universe?

-    This reionization epoch ended the “Cosmic Dark Ages” and led to the Universe becoming “transparent,” what astronomers refer to as “Cosmic Dawn.” According to our current cosmological models, reionization lasted from 380,000 to 1 billion years after the Big Bang. This is based on indirect evidence since astronomers have been unable to view the Epoch of Reionization directly.

-

-    Investigating this period was one of the main reasons for developing the James Webb Space Telescope (JWST), which can pierce the veil of the “dark ages” using its powerful infrared optics. However, observations provided by Webb revealed that far more galaxies existed in the early Universe than previously expected.

-

-     According to a recent study, this suggests that reionization may have happened more rapidly and ended at least 350 million years earlier than our models predict. Once again, the ability to peer into the early Universe has produced tensions with prevailing cosmological theories.

-

-    According to current cosmological models, the Universe was filled with a hot, dense plasma of protons and electrons for the first 380,000 years after the Big Bang. Eventually, the Universe cooled enough for protons and electrons to come together and form neutral hydrogen. By ca.100 million years after the Big Bang, the first stars (Population III) began to form, which were extremely massive and hot. These stars came together to create the first galaxies, and their ultraviolet light caused neutral hydrogen to once again split into protons and electrons ( became ionized).

-

-    Once most of the hydrogen in the Universe became ionized (ca. 1 billion years after the Big Bang), the Epoch of Reionization ended. At this point, the Universe was transparent, and light from this period is visible to optical telescopes today.    Reionization played a major role in how the Universe evolved.   The process heated and ionized gas in the Universe, which regulated how fast galaxies grew and evolved.   These early stars established the overall structure of galaxies in the Universe.

-

-   Before the deployment of the JWST, scientists relied on measurements of the Cosmic Microwave Background (CMB), the relic radiation from the Big Bang, and the Lyman-alpha Forest which is the wavelength of light associated with hydrogen reionization. From this, astronomers have gained a sense of how much energy was available for reionization to occur    (a “photon budget”) and how long it lasted.

-

-   Reionization is the last major change to happen. You went from neutral and cold and boring to ionized and hot. And this isn’t something that only happened to one or two galaxies. It happened to the whole Universe. It’s an accounting game. We know that all hydrogen was neutral before reionization. From there, you need enough extreme ultraviolet to split each atom. So you can do the math to figure out when reionization ended.

-

-    However, observations made with the JWST have revealed things that challenge accepted models. This includes a greater abundance of galaxies, which produce more UV radiation than previously anticipated. These findings suggest that reionization should have ended 550 to 650 million years after the Big Bang rather than 1 billion years.

-

-    But if this were true, the CMB and Lyman-alpha Forest would look different.   There is a tension between these measurements and Webb‘s observations.

-

-    Much like the “Hubble Tension”, these findings suggest something could be missing from our current cosmological models. One possibility that the team explored is recombination, where ionized protons and electrons come together again to form neutral hydrogen. This is precisely what happened 380,000 years after the Big Bang, known as the “Era of Recombination.”

-

-    If this process happened more often than our models suggest, it could increase the amount of extreme-UV light needed to reionize the Universe. Follow-up observations are needed to confirm this theory.  We need more detailed and deeper observation.

-

-

November 24, 2024        REIONIZATION  -  in the early Universe?          4620

------------------------------------------------------------------------------------------                                                                                                                        

--------  Comments appreciated and Pass it on to whomever is interested. ---

---   Some reviews are at:  --------------     http://jdetrick.blogspot.com ----- 

--  email feedback, corrections, request for copies or Index of all reviews

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Monday, November 25, 2024  ---------------------------------

 

 

 

 

 

           

 

 

4621 - PLANET DISCOVERED - size of the Earth?

 

-  4621 -  PLANET  DISCOVERED  -  size of the Earth?      This Earth-Sized Planet is about to be destroyed.   Astronomers have confirmed the existence of exoplanets with extremely small orbits around their stars. But what about exoplanets that get close enough to be devoured by their star, and what if it’s an Earth-sized exoplanet?


-----------------------   4621  -    PLANET  DISCOVERED  -  size of the Earth?

-    Astronomers are investigating an Earth-sized exoplanet with an orbital period of only 5.7 hours, known as “ultra-short-period” (USP) exoplanets, that could eventually experience what’s known as tidal disruption, resulting in its devourment by its star.

-

-    This study holds the potential to help researchers better understand the processes responsible for this, along with continuing to challenge our understanding of exoplanetary architectures.

-

-    Tidal disruption could be a potential fate of rocky planets.   It seems like about 10 percent of sun-like stars might have engulfed their rocky planets. This system TOI-6255 is the best-known progenitor for those planet engulfment events. The tidal disruption of rocky planets allows us to probe their interior composition and compare with Earth.

-

-    The researchers analyzed TOI-6255 b, whose radius is 1.08 and mass is 1.44 of Earth’s and located just over 65.2 light-years from Earth. However, while being Earth-sized holds promise for life, TOI-6255 b’s 5.7-hour orbit not only make this exoplanet far too hot for life as we know it to exist, but this also means its orbit takes it dangerously close to what’s known as Roche limit.

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-   This is the distance a smaller object can orbit a larger object until the larger object’s gravity tears the smaller object to pieces, along with TOI-6255 b also experiencing the tidal disruption, which is a common occurrence.

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-   This planet is doomed for tidal disruption in 400Myr which is short on cosmic scale (13Gyr). The planet is also tidally distorted to be football like in shape (10 percent deviation from sphere), in comparison Earth’s tidal distortion due to the moon is only 1e-7 [0.0000001] level.

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-  Orbital phase curve study of this planet could confirm that it is indeed tidally distorted. We know what the phase curve should look like for a spherical planet, tidally distorted planet has a strong deviation from that. We can also see if the surface of the planet is covered by lava pool as would be expected on a planet this hot.

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-    USPs are exoplanets whose orbits are less than one day and whose masses are less than 2x the Earth.   Only about 100 USPs have been discovered with a 2014 study estimating approximately 0.5 percent exist around Sun-like stars and a 2019 study discussing their bulk composition (i.e., mass of its iron core and mantle).

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-    Given their extremely short orbit, these worlds are likely too hot for life as we know it to exist, and along with USPs are the familiar “hot Jupiters” who orbit their stars in only a few days and astronomers estimate their population is in the hundreds.   These worlds are Jupiter-sized or larger gas planets and are also potentially far too hot for life as we know it to exist. But what is the significance of TOI-6255 b being an Earth-sized planet as opposed to a Jupiter-sized planet, or larger?

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-    Planets similar to Earth in size are most likely rocky i.e. mostly made of iron core and silicate mantle. They show us what terrestrial planets in other planetary systems are made of. Jupiter-sized planets are most certainly covered by thick hydrogen and helium atmospheres. Jupiter-sized planets are unlikely to harbor life.

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-    While “TOI-6255 b” isn’t due for disassembly for another 400 million years, watching any exoplanet get ripped to shreds by its host star could provide important insights regarding the planet’s exterior and interior compositions, helping us better understand the similarities between exoplanets and planets within our own solar system.

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-    These unique worlds and their extremely tight orbits have challenged our understanding of solar system architecture throughout our Milky Way Galaxy, as Mercury is the closest planet to our Sun, and it still takes 88 days to complete one orbit.

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-    One similarity between our solar system and exoplanetary systems is the Roche limit. Tidal disruption could be a potential fate of rocky planets.  Tidal disruption of planets is minimal in our solar system. However, the rings of Saturn are thought to originate from tidal disruption of satellites around Saturn. Tidal forces are strongly dependent on orbital separation, only objects with the shortest orbital period experience significant tides.

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November 24, 2024        PLANET  DISCOVERED  -  size of the Earth?           4621

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--------  Comments appreciated and Pass it on to whomever is interested. ---

---   Some reviews are at:  --------------     http://jdetrick.blogspot.com ----- 

--  email feedback, corrections, request for copies or Index of all reviews

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Monday, November 25, 2024  ---------------------------------

 

 

 

 

 

           

 

 

Sunday, November 24, 2024

4619 - HUBBLE CONSTANT – of space expansion?

 

-  4619 -  HUBBLE  CONSTANT – of space expansion?      We have been spoiled over recent years with first the Hubble Space Telescope (HST) and then the James Webb Space Telescope (JWST.) Both have opened our eyes on the Universe and made amazing discoveries. One subject that has received attention from both is the derivation of the Hubble Constant, a constant relating the velocity of remote galaxies and their distances.



---------------------------------------   4619  -    HUBBLE  CONSTANT – of space expansion?

-    The Hubble Constant (H0) is a fundamental parameter in cosmology that defines the rate of expansion of the universe. It defines the relationship between Earth and distant galaxies by the velocity they are receding from us.

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-    It was first discussed by Edwin Hubble in 1929 as he observed the spectra of distant galaxies. It is measured in unites of kilometres per second per megaparsec and shows how fast galaxies are moving away from us per unit of distance. The exact value of the constant has been the cause of many a scientific debate and more recently the HST and JWST have been trying to fine tune its value. Getting an accurate value is key to determining the age, size and fate of the universe.

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-  Astronomers used JWST to explore its earlier results of the cepheid/supernova distance ladder. This has been used to establish distances across the cosmos using cepheid variable stars and Type 1a supernovae. Both objects can be likened to ‘standard candles’ whose “actual brightness” is very well understood. By measuring their “apparent brightness” from Earth, their distances can be calculated by comparing it to their actual brightness, their 'intrinsic luminosity”.

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-   Over recent decades, a number of attempts have been made to accurately determine H0 using a multitude of different instruments and observations. The cosmic microwave background has been used along with the studies using cepheid variables and supernovae events. The results provide a range of results which has become known as ‘Hubble tension.’ 

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-    To be able to determine H0 with a level of accuracy using the cepheid/supernova ladder, a sufficiently high sample of cepheids and supernovae must be observed. This has been challenging, in particular of the sample size of supernovae within the range of cepheid variable stars.

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-     They also explored other techniques for determining H0 for example studying data from HST of the study of the luminosity of the brightest red giant branch stars in a galaxy, which can also work as a standard candle. Or the luminosity of certain carbon rich stars which are another technique.

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-    Astronomers used three steps astronomers used to measure the universe’s expansion rate (Hubble constant) to an unprecedented accuracy, reducing the total uncertainty to 2.3 percent. The “cosmic distance ladder” is used to measure accurate distances to galaxies near to and far from Earth. The latest Hubble study extends the number of Cepheid variable stars analyzed to distances of up to 10 times farther across our galaxy than previous Hubble results.

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-    When all JWST measurements are combined, including a correction for the low sample of supernovae data, that H0 comes out at 72.6 ± 2.0 km s?1 Mpc?  This compares to the combined HST data which determines H0 as 72.8 km s?1 Mpc?   It will take more years and more studies for the sample size of supernova from JWST to equal that from HST but the cross-check has so far revealed we are finally honing in on an accurate value for Hubble’s Constant.

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November 23, 2024           HUBBLE  CONSTANT – of space expansion?         4619

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--------  Comments appreciated and Pass it on to whomever is interested. ---

---   Some reviews are at:  --------------     http://jdetrick.blogspot.com ----- 

--  email feedback, corrections, request for copies or Index of all reviews

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Sunday, November 24, 2024  ---------------------------------