How the 2024 Total Solar Eclipse Is Different than the 2017 Eclipse

On April 8, the Moon’s shadow will sweep across the United States, as millions will view a total solar eclipse. For many, preparing for this event brings memories of the magnificent total solar eclipse on Aug. 21, 2017.

In 2017, an estimated 215 million U.S. adults (88% of U.S. adults) viewed the solar eclipse, either directly or electronically. They experienced the Moon pass in front of the Sun, blocking part or all of our closest star’s bright face. The eclipse in 2024 could be even more exciting due to differences in the path, timing, and scientific research.

Wider, More Populated Path

The path of totality – where viewers can see the Moon totally block the Sun, revealing the star’s outer atmosphere, called the corona – is much wider during the upcoming total solar eclipse than it was during the eclipse in 2017. As the Moon orbits Earth, its distance from our planet varies. During the 2017 total solar eclipse, the Moon was a little bit farther away from Earth than it will be during upcoming total solar eclipse, causing the path of that eclipse to be a little skinnier. In 2017, the path ranged from about 62 to 71 miles wide. During the April eclipse, the path over North America will range between 108 and 122 miles wide – meaning at any given moment, this eclipse covers more ground. 

The 2024 eclipse path will also pass over more cities and densely populated areas than the 2017 path did. This will make it easier for more people to see totality. An estimated 31.6 million people live in the path of totality this year, compared to 12 million in 2017. An additional 150 million people live within 200 miles of the path of totality.

You don’t need to live within the path of totality to see the eclipse – in April, 99% of people who reside in the United States will be able to see the partial or total eclipse from where they live. Every contiguous U.S. state, plus parts of Alaska and Hawaii, will experience at least a partial solar eclipse.

Longer Time in Totality

In April, totality will last longer than it did in 2017. Seven years ago, the longest period of totality was experienced near Carbondale, Illinois, at 2 minutes, 42 seconds. 

For the upcoming eclipse, totality will last up to 4 minutes, 28 seconds, in an area about 25 minutes northwest of Torreón, Mexico. As the eclipse enters Texas, totality will last about 4 minutes, 26 seconds at the center of the eclipse’s path. Durations longer than 4 minutes stretch as far north as Economy, Indiana. Even as the eclipse exits the U.S. and enters Canada, the eclipse will last up to 3 minutes, 21 seconds. 

During any total solar eclipse, totality lasts the longest near the center of the path, widthwise, and decreases toward the edge. But those seeking totality shouldn’t worry that they need to be exactly at the center. The time in totality falls off pretty slowly until you get close to the edge.

Heightened Solar Activity

Every 11 years or so, the Sun’s magnetic field flips, causing a cycle of increasing then decreasing solar activity. During solar minimum, there are fewer giant eruptions from the Sun, such as solar flares and coronal mass ejections. But during solar maximum, the Sun becomes more active.

In 2017, the Sun was nearing solar minimum. Viewers of the total eclipse could see the breathtaking corona – but since the Sun was quiet, streamers flowing into the solar atmosphere were restricted to just the equatorial regions of the star. The Sun is more magnetically symmetrical during solar minimum, causing this simpler appearance. During the 2024 eclipse, the Sun will be in or near solar maximum, when the magnetic field is more like a tangled hairball. Streamers will likely be visible throughout the corona. In addition to that, viewers will have a better chance to see prominences – which appear as bright, pink curls or loops coming off the Sun.

With lucky timing, there could even be a chance to see a coronal mass ejection – a large eruption of solar material – during the eclipse.

Expanded Scientific Research

During the total eclipse in 2024, NASA is funding several research initiatives that build on research done during the 2017 eclipse. The projects, which are led by researchers at different academic institutions, will study the Sun and its influence on Earth with a variety of instruments, including cameras aboard high-altitude research planes, ham radios, and more. In addition to those projects, instruments that were launched during the 2023 annular solar eclipse on three sounding rockets will again be launched during the upcoming total solar eclipse.

Two spacecraft designed to study the Sun’s corona – NASA’s Parker Solar Probe and ESA (European Space Agency) and NASA’s Solar Orbiter – have also launched since the 2017 solar eclipse. These missions will provide insights from the corona itself, while viewers on Earth see it with their own eyes, providing an exciting opportunity to combine and compare viewpoints.

To learn more about the 2024 total solar eclipse and how you can safely watch it, visit NASA’s eclipse website.

By Abbey Interrante
NASA’s Goddard Space Flight Center, Greenbelt, Md. 

Special thanks to Michael Zeiler for his calculations on the populations in the eclipse path.

The 2017 total solar eclipse viewing analysis was conducted by Professor Jon D. Miller of the University of Michigan. This study was supported by a collaborative agreement between the University of Michigan and the National Aeronautics and Space Administration (award NNX16AC66A).

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Poised for Science: NASA’s Europa Clipper Instruments Are All Aboard

The science performed by the complex suite of instruments recently added to the spacecraft will reveal whether Jupiter’s moon Europa has conditions that could support life.

With less than nine months remaining in the countdown to launch, NASA’s Europa Clipper mission has passed a major milestone: Its science instruments have been added to the massive spacecraft, which is being assembled at the agency’s Jet Propulsion Laboratory in Southern California.

Set to launch from Kennedy Space Center in Florida in October, the spacecraft will head to Jupiter’s ice-encased moon Europa, where a salty ocean beneath the frozen surface may hold conditions suitable for life. Europa Clipper won’t be landing; rather, after arriving at the Jupiter system in 2030, the spacecraft will orbit Jupiter for four years, performing 49 flybys of Europa and using its powerful suite of nine science instruments to investigate the moon’s potential as a habitable environment.

“The instruments work together hand in hand to answer our most pressing questions about Europa,” said JPL’s Robert Pappalardo, the mission’s project scientist. “We will learn what makes Europa tick, from its core and rocky interior to its ocean and ice shell to its very thin atmosphere and the surrounding space environment.”

The hallmark of Europa Clipper’s science investigation is how all of the instruments will work in sync while collecting data to accomplish the mission’s science objectives. During each flyby, the fully array of instruments will gather measurements and images that will be layered together to paint the full picture of Europa.

“The science is better if we obtain the observations at the same time,” Pappalardo said. “What we’re striving for is integration, so that at any point we are using all the instruments to study Europa at once and there is no need to have to trade off among them.”

From the Inside Out

By studying the environment around Europa, scientists will learn more about the moon’s interior. The spacecraft carries a magnetometer to measure the magnetic field around the moon. That data will be key to understanding the ocean, because the field is created, or induced, by the electrical conductivity of the ocean’s saltwater as Europa moves through Jupiter’s strong magnetic field. Working in tandem with the magnetometer is an instrument that will analyze the plasma (charged particles) around Europa, which can distort magnetic fields. Together, they’ll ensure the most accurate measurements possible.

What the mission discovers about Europa’s atmosphere will also lend insights into the moon’s surface and interior. While the atmosphere is faint, with only 100 billionth the pressure of Earth’s atmosphere, scientists expect that it holds a trove of clues about the moon. They have evidence from space- and ground-based telescopes that there may be plumes of water vapor venting from beneath the moon’s surface, and observations from past missions suggest that ice and dust particles are being ejected into space by micrometeorite impacts.

Three instruments will help investigate the atmosphere and its associated particles: A mass spectrometer will analyze gases, a surface dust analyzer will examine dust, and a spectrograph will collect ultraviolet light to search for plumes and identify how the properties of the dynamic atmosphere change over time.

All the while, Europa Clipper’s cameras will be taking wide- and narrow-angle pictures of the surface, providing the first high-resolution global map of Europa. Stereoscopic, color images will reveal any changes in the surface from geologic activity. A separate imager that measures temperatures will help scientists identify warmer regions where water or recent ice deposits may be near the surface.

An imaging spectrometer will map the ices, salts, and organic molecules on the moon’s surface. The sophisticated set of imagers will also support the full instrument suite by collecting visuals that will provide context for the set of data collected.

Of course, scientists also need a better understanding of the ice shell itself. Estimated to be about 10 to 15 miles (15 to 25 kilometers) thick, this outer casing may be geologically active, which could result in the fracture patterns that are visible at the surface. Using the radar instrument, the mission will study the ice shell, including searching for water within and beneath it. (The instrument’s electronics are now aboard the spacecraft, while its antennas will be mounted to the spacecraft’s solar arrays at Kennedy later this year.)

Finally, there’s Europa’s interior structure. To learn more about it, scientists will measure the moon’s gravitational field at various points in its orbit around Jupiter. Observing how signals transmitted from the spacecraft are tugged on by Europa’s gravity can tell the team more about the moon’s interior. Scientists will use the spacecraft’s telecommunications equipment for this science investigation.

With all nine instruments and the telecommunications system aboard the spacecraft, the mission team has begun testing the complete spacecraft for the first time. Once Europa Clipper is fully tested, the team will ship the craft to Kennedy in preparation for launch on a SpaceX Falcon Heavy rocket.

More About the Mission

Europa Clipper’s main science goal is to determine whether there are places below Jupiter’s icy moon, Europa, that could support life. The mission’s three main science objectives are to determine the thickness of the moon’s icy shell and its surface interactions with the ocean below, to investigate its composition, and to characterize its geology. The mission’s detailed exploration of Europa will help scientists better understand the astrobiological potential for habitable worlds beyond our planet.

Find more information about Europa here:

europa.nasa.gov

News Media Contacts

Gretchen McCartney
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-6215
gretchen.p.mccartney@jpl.nasa.gov

Karen Fox / Alana Johnson
NASA Headquarters, Washington
301-286-6284 / 202-358-1501
karen.c.fox@nasa.gov / alana.r.johnson@nasa.gov

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BioNutrients: A Five-Year Experiment in Space Nears Completion

NASA’s bio-manufacturing experiment called BioNutrients is testing a way to use microorganisms to produce on-demand nutrients that will be critical for human health during future long-duration space missions. Launched to the International Space Station in 2019, the experiment assesses the stability and performance of a hand-held system – dubbed a production pack – to manufacture fresh vitamins and other nutrients in space over a five-year span.

About once a year, scientists at NASA’s Ames Research Center in California’s Silicon Valley processed a set of production packs on the same day astronauts run production packs on the space station. This helps the researchers compare the performance of production packs stored and activated in space to those on the ground, providing data on how the space environment affects nutrient production over the five-year timeline. Demonstrating that NASA can produce nutrients after at least five years in space provides confidence it will be capable of supporting crewed missions to Mars.

In early January, researchers Natalie Ball, Hiromi Kagawa, and Sandra Vu processed the last of a planned series of BioNutrients production packs hours after JAXA (Japan Aerospace Exploration Agency) astronaut Satoshi Furukawa’s duplicate experiment onboard the orbiting laboratory. Samples from this in-space production are planned to return to Earth in February on Axiom Mission 3.

BioNutrients was developed by NASA Ames. NASA’s Space Technology Mission Directorate and its Game Changing Development program manage the project as part of the agency’s broader synthetic biology portfolio.

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Gianine Figliozzi

Station Science 101: Epigenetics Research in Space

A growing body of research suggests a link between epigenetic mechanisms and a wide variety of illnesses and behaviors, including cancer, cardiovascular and autoimmune illnesses, and cognitive dysfunction. Epigenetics also plays a role in the changes humans and other living things experience in space.

This phenomenon has become part of studies in a wide variety of fields, including microgravity research conducted aboard the International Space Station.

So just what is epigenetics? According to a paper from the National Institute of Environmental Health Sciences, it includes any process that alters gene activity without changing the actual DNA sequence and that leads to modifications that can pass to offspring. Essentially, it involves information added to the DNA sequence of four bases: adenine (A), guanine (G), cytosine (C), and thymine (T).

The sequence of these bases forms the genetic code for development and functioning – essentially the blueprint for every living thing. Epigenetics changes an organism by changing which genes are expressed – essentially turned on or off – without changing that basic blueprint. In other words, epigenetics results in a change through modification of gene expression rather than alteration of the genetic code itself.

Epigenetic changes can be caused by many outside stimuli, from chemicals to trauma to exercise. And unlike a genetic change or mutation, an epigenetic change can reverse if the stimulus is removed. Many epigenetic changes are positive, or even essential, but some cause serious adverse health and behavioral effects.

Years of analysis have shown that the spaceflight environment changes gene expression in every organism and cell type. Epigenetics could help scientists figure out how that happens and why. Studying epigenetics could reveal the pathway that cells use to adapt and survive in microgravity and reveal ways to control positive changes or prevent negative ones.

The Epigenetics investigation from JAXA (Japan Aerospace Exploration Agency) looked at whether the round worm C. elegans experienced epigenetic changes and if those changes transmitted from one generation to another. Researchers did observe epigenetic changes and concluded that the expression of certain genes, including negative regulators of growth and development, is epigenetically fine-tuned to adapt to microgravity.¹

JAXA’s Mouse Epigenetics studied altered gene expression patterns in mice and DNA changes in their offspring. The investigation identified genetic alterations that happen after exposure to the microgravity environment of space.

An Italian Space Agency study of the bone loss experienced by astronauts on extended missions is associated with epigenetic alterations. Role of the Endocannabinoid System in Pluripotent Human Stem Cell Reprogramming under Microgravity Conditions (SERISM) evaluated the formation of bone cells in microgravity using human blood-derived stem cells as a model. Researchers reported specific epigenetic changes that occurred in the cells in space.²

One epigenetic process that researchers can detect is methylation, the addition or removal of a methyl group (CH3) into DNA bases, predominantly where cytosine or C bases occur consecutively. The APEX-03-1 and APEX-03-2 experiments examined DNA methylation and gene expression in Arabidopsis thaliana plants grown from seeds aboard the space station and found widespread changes in patterns of gene expression.³ They also observed epigenetic changes, indicating that they play a role in a plant’s physiological adaptation to spaceflight.⁴

APEX-04 confirmed this finding. When investigators disrupted the ability of a plant to make those epigenetic changes, that plant struggled more in space.⁵ Plant Habitat-03 then examined whether these epigenetic changes pass to subsequent generations.

In general, this work showed that plants change gene expression patterns when they experience strange environments and use epigenetic processes to mark genes that help prepare the next generation for the same environment. Those markers show which genes are important for the plant to live in space. Researchers can use that information to breed plants better adapted to space and to harsh environments on Earth.

Expect to see more research on epigenetics on orbit now that more tools are available to provide the ability to immediately sequence DNA at the level that reveals epigenetic changes such as methylation. Traditional DNA sequencers do not provide that level of information without prior processing of the sample, but the space station’s MinION can. Scientists can use these tools to get real-time snapshots of changes as they are happening and potentially how they are passed to subsequent generations.

Melissa Gaskill

International Space Station Program Science Office
Johnson Space Center

Search this database of scientific experiments to learn more about those mentioned above.

Citations:

¹ Higashitani A, Hashizume T, Takiura M, Higashitani N, Teranishi M, Oshima R, Yano S, Kuriyama K, Higashibata A. Histone deacetylase HDA-4-mediated epigenetic regulation in space-flown C. elegans. npj Microgravity. 2021 September 1; 7(1): 33. DOI: 10.1038/s41526-021-00163-7.PMID: 34471121.

² Gambacurta A, Merlini G, Ruggiero C, Diedenhofen G, Battista N, Bari M, Balsamo M, Piccirillo S, Valentini G, Mascetti G, Maccarrone M. Human osteogenic differentiation in Space: proteomic and epigenetic clues to better understand osteoporosis. Scientific Reports. 2019 June 6; 9(1): 8343. DOI: 10.1038/s41598-019-44593-6.PMID: 31171801.

³ Nakashima J, Pattathil S, Avci U, Chin S, Sparks JA, Hahn MG, Gilroy S, Blancaflor EB. Glycome profiling and immunohistochemistry uncover changes in cell walls of Arabidopsis thaliana roots during spaceflight. npj Microgravity. 2023 August 22; 9(1): 1-13. DOI: 10.1038/s41526-023-00312-0.

⁴ Zhou M, Sng NJ, LeFrois CE, Paul AL, Ferl RJ. Epigenomics in an extraterrestrial environment: Organ-specific alteration of DNA methylation and gene expression elicited by spaceflight in Arabidopsis thaliana. BMC Genomics. 2019 March 12; 20(1): 205. DOI: 10.1186/s12864-019-5554-z.

⁵ Paul AL, Haveman NJ, Califar B, Ferl RJ. Epigenomic regulators elongator complex subunit 2 and methyltransferase 1 differentially condition the spaceflight response in Arabidopsis. Frontiers in Plant Science. 2021 September 13; 12691790. DOI: 10.3389/fpls.2021.691790.

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Hubble Spies a Spinning Spiral

Looking like a baseball lobbed into the depths of the universe, ESO 420-G013 is a face-on spiral galaxy and a Seyfert galaxy. Dark lanes of dust are visible against the background glow of the galaxy’s many stars. 

About 10 percent of all the galaxies in the universe are thought to be Seyfert galaxies. They are typically spiral galaxies and have very bright nuclei, the result of supermassive black holes at their centers accreting material that releases vast amounts of radiation. The cores of these “active galaxies” are brightest when observing light outside the visible spectrum. Often galaxies with these kinds of active galactic nuclei are so bright that the host galaxy itself cannot be seen, washed out by the glow of its nuclei, but Seyfert galaxies are distinctive because the galaxy itself is also visible. In the case of ESO 420-G013, we can enjoy the galaxy’s almost perfectly round disk, brighter core, and whirled filaments of dark dust.

NASA’s Hubble Space Telescope observed ESO 420-G013 as part of a study of Luminous Infrared Galaxies, or LIRGs, which are known to be extremely bright in the infrared part of the spectrum. Galactic interactions trigger new regions of star formation in LIRGs, causing them to be highly luminous in infrared light.

LEARN MORE:

Media Contact:

Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, MD
claire.andreoli@nasa.gov

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