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The Next Full Moon is the Buck or Thunder Moon


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The Next Full Moon is the Buck or Thunder Moon

A large deer with spiky antlers stands majes·ti·cal·ly in a forest.
Mule deer buck, Yellowstone National Park

The Next Full Moon is the Buck or Thunder Moon; the Hay or Mead Moon; Guru Purnima; Asalha Puja (aka Dharma Day or Esala Poya); and the start of Vassa. 

The next full Moon will be Sunday morning, July 21, 2024, appearing opposite the Sun (in Earth-based longitude) at 6:17 AM EDT. For the International Date Line West and the American Samoa and Midway time zones this will be late Saturday night. For Line Islands Time this will be early Monday morning. The Moon will appear full for about three days around this time, from Friday evening through Monday morning, making this a full Moon weekend. 

The Maine Farmers’ Almanac began publishing “Indian” names for full Moons in the 1930s and these names are now widely known and used. According to this almanac, as the full Moon in June the Algonquin tribes of what is now the northeastern United States called this the Buck Moon. Early summer is normally when the new antlers of buck deer push out of their foreheads in coatings of velvety fur. They also called this the Thunder Moon because of early Summer’s frequent thunderstorms.

Europeans called this the Hay Moon for the haymaking of early summer, and sometimes the Mead Moon (although this name was also used for the previous full Moon). Mead is created by fermenting honey mixed with water, sometimes adding fruits, spices, grains, or hops. 

For Hindus, Buddhists, and Jains, this is the Guru Full Moon (Guru Purnima), celebrated as a time for clearing the mind and honoring the guru or spiritual master. 

For Theravada Buddhists this full Moon is Asalha Puja, also known as Dharma Day or Esala Poya, an important festival celebrating the Buddha’s first sermon after reaching nirvana, which started Buddhism. This sermon became the core of Buddhist teachings and includes the four noble truths. In addition, with this full Moon the Buddhist Monks start Vassa, the annual three-month retreat during the rainy season. 

In many traditional lunisolar and lunar calendars full Moons fall on or near the middle of the lunar months. This full Moon is near the middle of the sixth month of the Chinese year of the Dragon, Tammuz in the Hebrew calendar, and Muharram in the Islamic calendar. Muharram is one of the four sacred months during which warfare is forbidden. 

Since this is the Thunder Moon, a quick note on lightning safety. Most of the lightning that strikes the ground arcs from the negatively charged bottom of the storm to the ground underneath the storm. Much rarer is positive lightning, which arcs from the top of a thunderstorm to strike much farther away. Positive lightning can sometimes strike areas where the sky is clear (hence the term “bolt out of the blue”). NOAA’s Lightning FAQ Page says that almost all lightning will occur within 10 miles of its parent thunderstorm, but that lightning detection equipment has confirmed bolts striking up to almost 50 miles away. Because positive lightning arcs across a greater distance it tends to be 5 to 10 times more powerful than regular ground strikes. It can strike dry areas outside of the storm’s rainfall, so positive lightning tends to start more fires than negative lightning. Although positive lightning is rare (less than 5% of all lightning strikes), the lack of warning and its greater power make it more lethal. A good rule to follow is, if you can hear the thunder, you can be struck by lightning. As a bicycle enthusiast and daily commuter (before I retired) I am well aware that the inch or so of rubber tire between my metal bicycle and the ground will make little difference to a bolt that can arc across miles of air from the top of a thunderstorm to where I am riding. 

As usual, the wearing of suitably celebratory celestial attire is encouraged in honor of the full Moon. Be safe (especially during thunderstorms), avoid starting wars, and take a moment to clear your mind. 

As for other celestial events between now and the full Moon after next (with specific times and angles based on the location of NASA Headquarters in Washington, D.C.):

As summer continues the daily periods of sunlight continue to shorten from their longest on the summer solstice on June 20, 2024. On Sunday, July 21, (the day of the full Moon), morning twilight will begin at 4:52 AM, sunrise will be at 6:00 AM, solar noon at 1:15 PM when the Sun will reach its maximum altitude of 71.4 degrees, sunset will be at 8:28 PM, and evening twilight will end at 9:37 PM. By Monday, Aug. 21, (the day of the full Moon after next), morning twilight will begin at 5:24 AM, sunrise will be at 6:26 AM, solar noon at 1:11 PM when the Sun will reach its maximum altitude of 63.6 degrees, sunset will be at 7:57 PM, and evening twilight will end at 8:58 PM.

Six meteor showers are predicted to peak during this lunar cycle, including one of the best meteor showers of the year for the Southern Hemisphere and one of the best meteor showers of the year for the Northern Hemisphere. 

On July 31, 2024, the Southern Delta Aquariids (005 SDA) meteor shower is predicted to peak at 25 meteors per hour (under ideal conditions). This shower is one of the most active annual sources for the Southern Hemisphere, but viewing it from our more northern latitudes will be difficult. As reported by the International Meteor Organization, this shower has a broad peak, and in past years observers from Australia (in 1977) and Crete (in 2003) have reported outbursts of 40 meteors per hour several days before the predicted peak. On the morning of the predicted peak (July 31), the best time to look (from the Washington, D.C. area) will likely be from after midnight until about 2 AM. The radiant (the point from which the meteors appear to radiate out from) will rise on the east-southeastern horizon on July 30 at about 10:15 PM. Since half of the meteors are hidden by the horizon at radiant rise, waiting until the radiant is higher in the sky should make more meteors visible. But moonrise will be at 1:58 AM (when the radiant will be about 30 degrees above the south-southeastern horizon). After moonrise moonlight will interfere with seeing these meteors, making our window for seeing these meteors fairly short. The parent body for this meteor shower is not certain, but they are caused by dust entering our atmosphere at 41 kilometers per second (92,000 miles per hour), so fast that air gets compressed and heated until it glows white-hot. 

This should be a good year for the annual Perseid meteor shower. The Perseids (007 PER) meteor shower is predicted to peak on Monday, Aug. 12, 2024, between 9 AM and Noon EDT (when we can’t see them). At its peak (under ideal conditions) the Perseids can produce about 100 visible meteors per hour, making it one of the three best meteor showers of the year for the Northern Hemisphere (the others being the Quadrantids in early January and the Geminids in mid December). The time closest to the predicted peak that we can see will be the early morning of Aug. 12. Moonset will be a little before midnight on Aug. 11, and the radiant will rise higher in the north-northeastern sky until the sky shows the first signs of dawn (before morning twilight begins at 5:16 AM). The peak is broad, and in past years high activity has been reported well after the peak, so keep an eye on the sky between moonset and the first hints of dawn for the nights before and after the predicted peak. The Perseid meteor shower is caused by dust from the comet 109P/Swift-Tuttle entering our atmosphere at 59 kilometers per second (132,000 miles per hour) – as previously noted, so fast that air gets compressed and heated until it glows white-hot. 

The best conditions for viewing these meteors would be if the weather is clear with no clouds or high hazes, you go to a place far from any light sources or urban light pollution, and you have a clear view of a wide expanse of the sky. Be sure to give your eyes plenty of time to adapt to the dark. The rod cells in your eyes are more sensitive to low light levels but play little role in color vision. Your color-sensing cone cells are concentrated near the center of your view with more of the rod cells on the edge of your view. Since some meteors are faint, you will tend to see more meteors from the “corner of your eye” (which is why you need a view of a large part of the sky). Your color vision (cone cells) will adapt to darkness in about 10 minutes, but your more sensitive night vision will continue to improve for an hour or more (with most of the improvement in the first 35 to 45 minutes). The more sensitive your eyes are, the more chance you have of seeing meteors. Even a short exposure to light (from passing car headlights, etc.) will start the adaptation over again (so no turning on a light or your cell phone to check what time it is). 

The other four meteor showers, the July Gamma Draconids (184 GDR), Alpha Capricornids (001 CAP), Eta Eridanids (191 ERI), and Kappa Cygnids (012 KCG), are all expected to produce less than five meteors per hour under ideal conditions (which most of us don’t have in our urban and suburban environs) but if you happen to be out with a clear sky late at night or in the early morning, your odds of spotting a meteor are a little higher than usual. 

No comets are expected to be visible this lunar cycle. 

Evening Sky Highlights

On the evening of Sunday, July 21, 2024 (the evening of the day of the full Moon), as twilight ends (at 9:37 PM EDT), the rising Moon will be 3 degrees above the east-southeastern horizon. The bright planet Mercury will be 1 degree above the west-northwestern horizon and six minutes away from setting. The planet Venus will set 22 minutes before twilight ends, but will be bright enough to see in the glow of dusk, low on the west-northwestern horizon before it sets. The bright object appearing closest to overhead will be Vega, the brightest star in the constellation Lyra the lyre, at 65 degrees above the eastern horizon. Vega is one of the three bright stars in the “Summer Triangle,” along with Deneb and Altair. It is the fifth-brightest star in our night sky, about 25 light-years from Earth, has twice the mass of our Sun, and shines 40 times brighter than our Sun. 

As this lunar cycle progresses the background of stars will appear to shift westward each evening (as the Earth moves around the Sun), while the planet Mercury will initially dwell low on the west-northwestern horizon, shifting towards the left. On July 24 Mercury will be 2 degrees below the bright star Regulus, and this will be the last evening Mercury will be above the horizon as twilight ends (although it may remain visible in the glow of dusk before twilight ends into early August). The bright planet Venus will also be visible in the glow of dusk, gradually shifting away from the Sun, but will not be above the horizon as twilight ends until late August. The bright star Regulus will appear about 1 degree to the lower right of Venus on Aug. 4, low on the west-northwestern horizon, with Regulus setting 17 minutes before evening twilight ends. The waxing Moon will pass by Venus and Regulus on Aug. 5 (setting before evening twilight ends), Spica on Aug. 9 and 10, and Antares on Aug. 13. Aug. 16 will be the first evening that the planet Saturn will be above the eastern horizon as evening twilight ends. 

By the evening of Monday, Aug. 19 (the evening of the day of the full Moon after next), as twilight ends (at 8:58 PM), the rising Moon will be 7 degrees above the east-southeastern horizon. The only visible planet in the sky will be Saturn at 1.5 degrees above the eastern horizon. The planet Venus will set four minutes before twilight ends but will be bright enough to see in the glow of dusk, low on the western horizon before it sets. The bright object appearing closest to overhead will still be Vega at 80 degrees above the eastern horizon. 

Morning Sky Highlights

On the morning of Sunday, July 21, 2024 (the morning of the day of the full Moon), as twilight begins (at 4:52 AM EDT), the setting Moon will be 7 degrees above the southwestern horizon. The brightest planet in the sky will be Jupiter at 25 degrees above the eastern horizon. Mars will be 33 degrees above the eastern horizon and Saturn 45 degrees above the southern horizon. The bright object appearing closest to overhead will be the star Deneb at 56 degrees above the west-northwestern horizon. Deneb is the 19th brightest star in our night sky and is the brightest star in the constellation Cygnus the swan. Deneb is one of the three bright stars of the Summer Triangle (along with Vega and Altair). It is about 20 times more massive than our Sun but has used up its hydrogen, becoming a blue-white supergiant about 200 times the diameter of the Sun. If Deneb were where our Sun is, it would extend to about the orbit of Earth. Deneb is about 2,600 light-years from us. 

As this lunar cycle progresses, Jupiter, Saturn, and the background of stars will appear to shift westward each evening, with Mars shifting more slowly and to the left toward Jupiter. The waning Moon will pass by Saturn on July 25, Mars on July 30, Jupiter on July 31, and Pollux on Aug. 2 and 3. Jupiter and Mars will appear at their closest on Aug. 14, after which they will separate again. 

By the morning of Monday, Aug. 19 (the morning of the day of the full Moon after next), as twilight begins (at 5:24 AM), the setting full Moon will be 5 degrees above the southwestern horizon. The brightest planet in the sky will be Jupiter at 49 degrees above the eastern horizon. Near Jupiter will be Mars at 47 degrees above the eastern horizon. Saturn will be 29 degrees above the southwestern horizon. The bright object appearing closest to overhead will be the star Capella, the brightest star in the constellation Auriga the charioteer, at 55 degrees above the east-northeastern horizon. Although we see Capella as a single star (the sixth-brightest in our night sky), it is actually four stars (two pairs of stars orbiting each other). Capella is about 43 light-years from us.

Detailed Daily Guide

Here for your reference is a day-by-day listing of celestial events between now and the full Moon after next. The times and angles are based on the location of NASA Headquarters in Washington, D.C., and some of these details may differ for where you are (I use parentheses to indicate times specific to the D.C. area). 

Wednesday night into early Thursday morning, July 17 to 18, 2024, the bright star Antares will appear near the waxing gibbous Moon. As evening twilight ends (at 9:40 PM EDT) Antares will be 3 degrees to the upper right of the Moon. The Moon will reach its highest in the sky 27 minutes later (at 10:07 PM). As Antares sets (at 2:21 AM) it will be 5 degrees to the lower right of the Moon. For much of the southern part of Africa the Moon will pass in front of Antares earlier on Wednesday. See http://lunar-occultations.com/iota/bstar/0717zc2366.htm (external link) for a map and information on the locations that will see this occultation. 

As mentioned above, the full Moon will be Sunday morning, July 21, 2024, appearing opposite the Sun (in Earth-based longitude) at 6:17 AM EDT. This will be late Saturday night in the International Date Line West and the American Samoa and Midway time zones, and early Monday morning in the Line Islands Time zone. The Moon will appear full for about three days around this time, from Friday evening through Monday morning, making this a full Moon weekend. 

Early Monday morning, July 22, 2024, will be when the planet Mercury reaches its greatest angular separation from the Sun as seen from Earth for this apparition (called greatest elongation). Because the angle between the line from the Sun to Mercury and the line of the horizon changes with the seasons, the date when Mercury and the Sun appear farthest apart as seen from Earth is not always the same as when Mercury appears highest above the horizon as evening twilight ends (which occurred on July 13). 

Early Wednesday morning, July 24, 2024, at 1:43 AM EDT, the Moon will be at perigee, its closest to Earth for this orbit. 

Wednesday evening, July 24, 2024, will be the last evening that the planet Mercury will be above the west-northwestern horizon as evening twilight ends (at 9:34 PM EDT), setting one minute later. This will also be the evening when Mercury will appear closest to the bright star Regulus, which will be 2 degrees above Mercury on the horizon. 

Wednesday night into Thursday morning, July 24 to 25, 2024, the planet Saturn will appear near the waning gibbous Moon. At moonrise on the eastern horizon (at 10:45 PM EDT) Saturn will be 4 degrees to the upper right of the Moon. By the time the Moon reaches its highest (at 4:42 AM) Saturn will be 7 degrees to the lower right, with morning twilight beginning 14 minutes later. See http://lunar-occultations.com/iota/planets/0724saturn.htm (external link) for a map and information on where the Moon will block Saturn from view. 

Saturday evening July 27, 2024, the waning Moon will appear half-full as it reaches its last quarter at 10:52 PM EDT (when we can’t see it).

Tuesday, July 30, 2024, the planet Mars will appear 4 degrees to the lower right of the waning crescent Moon with the Pleiades star cluster to the upper right of the Moon. Mars will rise on the east-northeastern horizon (at 1:39 AM EDT) with the Pleiades star cluster 5 degrees to the upper right of the Moon. Morning twilight will begin more than three hours later (at 5:01 AM) with the Pleiades 7 degrees to the upper right.

As described earlier in this posting, early Wednesday morning, July 31, 2024, from about midnight until moonrise (at 1:58 AM EDT) will likely be the best time to look toward the southeast for the Southern Delta Aquariids (005 SDA) meteor shower. Although viewing from our more northern latitudes will be limited, this shower is one of the most active annual sources for the Southern Hemisphere (with a predicted peak of 25 meteors per hour under ideal conditions). This shower has a broad peak, and rare outbursts of up to 40 meteors per hour have been reported days before the predicted peak (in 1977 and 2003). You might have an increased chance of seeing meteors in the early mornings from after midnight to before moonrise around this date. 

Friday morning, Aug. 2, 2024, the bright star Pollux (the brighter of the twin stars in the constellation Gemini) will appear 8 degrees to the lower left of the waning crescent Moon. Pollux will rise after the Moon on the northeastern horizon (at 4:24 AM EDT) and morning twilight will begin 41 minutes later (at 5:05 AM). 

The next morning, Saturday, Aug. 3, 2024, the thin, waning crescent Moon will have shifted to 7 degrees below Pollux. The Moon will rise (at 4:59 AM EDT) on the east-northeastern horizon just six minutes before morning twilight begins. 

Throughout this lunar cycle the planet Mars will be passing above the bright star Aldebaran as it moves towards the bright planet Jupiter. Sunday morning, Aug. 4, 2024, will be when Mars and Aldebaran will be at their closest, about 5 degrees apart. Jupiter, Mars, and Aldebaran will form a triangle, with Mars above, Aldebaran to the lower right (matching Mars in brightness), and bright Jupiter to the lower left. Aldebaran will rise last (at 1:53 AM EDT) on the east-northeastern horizon and will be 37 degrees above the eastern horizon as morning twilight begins (at 5:07 AM). The constellation Orion will appear on the horizon below this triangle. 

Sunday morning, Aug. 4, 2024, at 7:13 AM EDT, will be the new Moon, when the Moon passes between the Earth and the Sun and will not be visible from the Earth. The day of, or the day after the New Moon marks the start of the new month for most lunisolar calendars. Aug. 4 is the start of the seventh month of the Chinese Year of the Dragon. Sundown on Aug. 4 is the start of Av in the Hebrew calendar. In the Islamic calendar the months traditionally start with the first sighting of the waxing crescent Moon. Many Muslim communities now follow the Umm al-Qura Calendar of Saudi Arabia, which uses astronomical calculations to start months in a more predictable way. Using this calendar, sundown on Sunday, Aug. 4, will probably mark the start of Safar, the second month of the Islamic calendar. 

Monday evening, Aug. 5, 2024, if you have a very clear view of the western to west-northwestern horizon (particularly with binoculars), you might be able to see the thin, waxing crescent Moon less than a degree above the bright planet Venus, with the bright star Regulus 1.5 degrees below Venus. The planet Mercury (less bright than Regulus) will be 6 degrees to the lower left of Venus. There may only be a short window between when dusk will have faded enough to see Mercury and when Mercury sets 36 minutes after sunset (at 8:50 PM EDT). Regulus will set next nine minutes after Mercury (45 minutes after sunset), followed by Venus eight minutes later (53 minutes after sunset), and the Moon six minutes after that (59 minutes after sunset), six minutes before evening twilight ends (at 9:19 PM). Venus and Regulus will have been at their closest (1 degree apart) the evening before and Mercury and Venus will be at their closest (6 degrees apart) two evenings later, but these will be hard to spot, low on the horizon in the glow of dusk. 

Thursday, Aug. 8, 2024, at 9:32 PM EDT, the Moon will be at apogee, its farthest from the Earth for this orbit. 

Friday evening, Aug. 9, 2024, the bright star Spica will appear 5 degrees to the upper left of the waxing crescent Moon. The Moon will be 14 degrees above the west-southwestern horizon as evening twilight ends (at 9:13 PM EDT). The Moon will set first a little more than an hour later (at 10:35 PM). Saturday morning, for part of the western Pacific north of Australia and Indonesia, the Moon will block Spica from view. See http://lunar-occultations.com/iota/bstar/0810zc1925.htm (external link) for a map and information on locations that can see this occultation. 

By Saturday evening, Aug. 10, 2024, the waxing crescent Moon will have shifted to 7 degrees to the left of the star Spica as evening twilight ends and the pair will separate as the night progresses. 

Saturday night, Aug. 10, 2024, will be the night of the seventh day of the seventh month of the Chinese calendar, known as the double seventh festival, Qixi in China, Chilseok in Korea, and Thất Tịch in Vietnam. The double seventh festival is sometimes called the Chinese Valentine’s Day. There are many variations on the legend, but basically they involve the Milky Way and the three bright stars we know as the Summer Triangle. The star Vega represents the weaver girl and the star Altair represents the cowherd. They fall in love and neglect their duties, so the Goddess of Heaven puts a wide river in the sky, the Milky Way, to keep them apart. They are allowed to meet only one night a year, on the seventh night of the seventh month, when the star Deneb forms a bridge across the Milky Way. In some versions of the legend, the bridge is formed by magpies, so another name is the Magpie Festival. The Japanese Tanabata or Star Festival is related, but is no longer tied to the lunisolar date (it is now celebrated on July 7, the double seventh of the Gregorian Calendar). On average there are a little more than seven days between each quarter of the Moon, so the first quarter Moon tends to occur a day or two after the seventh day of the lunisolar month. 

As described earlier in this post, this should be a good year for the annual Perseids (007 PER) meteor shower, which can peak at more than 100 meteors per hour (under ideal conditions). The time closest to the predicted peak that we can see (from the Washington, D.C. area) will be the early morning of Monday, Aug. 12, 2024. Moonset will be a little before midnight on Aug. 11 and the radiant will rise higher in the north-northeastern sky until the sky shows the first signs of dawn (before morning twilight begins at 5:16 AM). The peak is broad, and in past years high activity has been reported well after the peak, so keep an eye on the sky from moonset to the first hints of dawn on the nights before and after as well. See the meteor shower summary near the beginning of this post for more information on viewing these meteors. 

Monday morning, Aug. 12, 2024, the Moon will appear half-full as it reaches its first quarter at 11:19 AM EDT (when we can’t see it). 

Tuesday night, Aug. 13, 2024, the bright star Antares will appear near the waxing gibbous Moon. Antares will be 2.5 degrees to the upper left as evening twilight ends (at 9:08 PM EDT). By the time of moonset on the southwestern horizon (Wednesday morning at 12:30 AM) Antares will be 1 degree above the Moon. Viewers in the southern part of South America and the Antarctic Peninsula will see the Moon pass in front of Antares. See http://lunar-occultations.com/iota/bstar/0814zc2349.htm (external link) for a map and information on areas that can see this occultation. 

Throughout this lunar cycle the planet Mars will drift toward the bright planet Jupiter. They will be at their closest on Wednesday morning, Aug. 14, 2024, just a third of a degree apart, which should be a good show! Bright Jupiter will rise early in the morning (at 1:18 AM EDT) on the east-northeastern horizon below Mars. They will be 45 degrees above the eastern horizon as morning twilight begins four hours later (at 5:18 AM). 

Friday evening, Aug. 16, 2024, will be the first evening that the planet Saturn will be above the eastern horizon as evening twilight ends (at 9:03 PM EDT). 

Sunday evening, Aug. 18, 2024, the planet Mercury will be passing between Earth and the Sun as seen from Earth, called inferior conjunction. Planets that orbit inside of the orbit of Earth can have two types of conjunctions with the Sun, inferior (when passing between the Earth and the Sun) and superior (when passing on the far side of the Sun as seen from the Earth). Mercury will be shifting from the evening sky to the morning sky and will begin emerging from the glow of dawn on the east-northeastern horizon at the end of August. 

The full Moon after next will be Monday afternoon, Aug. 19, 2024, at 2:26 PM EDT. This will be Tuesday morning from Nepal Standard Time eastward across the rest of Asia and Australia to the International Date Line. The Moon will appear full for about three days around this time, from Sunday morning through early Wednesday morning. As the third full Moon in a season with four full Moons, this will be a Blue Moon (by the older, more traditional definition).

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      A composite X-ray/Optical/Infrared image of the Crab Pulsar. The X-ray image from the Chandra X-ray Observatory (blue and white), reveals exquisite details in the central ring structures and gas flowing out of the polar jets. Optical light from the Hubble Space Telescope (purple) shows foreground and background stars as pinpoints of light. Infrared light from the Spitzer Space Telescope (pink) traces cooler gas in the nebula. Finally, magnetic field direction derived from X-ray polarization observed by the Imaging X-ray Polarimetry Explorer is shown as orange lines. Magnetic field lines: NASA/Bucciantini et al; X-ray: NASA/CXC/SAO; Optical: NASA/STScI; Infrared: NASA-JPL-Caltech Unlike optical telescopes that create images by reflecting or refracting light at near-90-degree angles (normal incidence), focusing X-ray optics must be designed to reflect light at very small angles (grazing incidence). At normal incidence, X-rays are either absorbed by the surface of a mirror or penetrate it entirely. However, at grazing angles of incidence, X-rays reflect very efficiently due to an effect called total external reflection.  In grazing incidence, X-rays reflect off the surface of a mirror like rocks skipping on the surface of a pond.
      A classic design for astronomical grazing incidence optics is the Wolter-I prescription, which consists of two reflecting surfaces, a parabola and hyperbola (see figure below). This optical prescription is revolved around the optical axis to produce a full-shell mirror (i.e., the mirror spans the full circumference) that resembles a gently tapered cone. To increase the light collecting area, multiple mirror shells with incrementally larger diameters and a common focus are fabricated and nested concentrically to comprise a mirror module assembly (MMA).
      Focusing optics are critical to studying the X-ray universe because, in contrast to other optical systems like collimators or coded masks, they produce high signal-to-noise images with low background noise. Two key metrics that characterize the performance of X-ray optics are angular resolution, which is the ability of an optical system to discriminate between closely spaced objects, and effective area, which is the light collecting area of the telescope, typically quoted in units of cm2. Angular resolution is typically measured as the half-power diameter (HPD) of a focused spot in units of arcseconds.  The HPD encircles half of the incident photons in a focused spot and measures the sharpness of the final image; a smaller number is better. 
      Schematic of a full-shell Wolter-I X-ray optic mirror module assembly with five concentrically nested mirror shells. Parallel rays of light enter from the left, reflect twice off the reflective inside surface of the shell (first off the parabolic segment and then off the hyperbolic segment), and converge at the focal plane. NASA MSFC NASA Marshall Space Flight Center (MSFC) has been building and flying lightweight, full-shell, focusing X-ray optics for over three decades, always meeting or exceeding angular resolution and effective area requirements. MSFC utilizes an electroformed nickel replication (ENR) technique to make these thin full-shell X-ray optics from nickel alloy.
      X-ray optics development at MSFC began in the early 1990s with the fabrication of optics to support NASA’s Advanced X-ray Astrophysics Facility (AXAF-S) and then continued via the Constellation-X technology development programs. In 2001, MSFC launched a balloon payload that included two modules each with three mirrors, which produced the first focused hard X-ray (>10 keV) images of an astrophysical source by imaging Cygnus X-1, GRS 1915, and the Crab Nebula.  This initial effort resulted in several follow-up missions over the next 12 years, and became known as the High Energy Replicated Optics (HERO) balloon program.
      In 2012, the first of four sounding rocket flights of the Focusing Optics X-ray Solar Imager (FOXSI) flew with MSFC optics onboard, producing the first focused images of the Sun at energies greater than 5 keV. In 2019 the Astronomical Roentgen Telescope X-ray Concentrator (ART-XC) instrument on the Spectr-Roentgen-Gamma Mission launched with seven MSFC-fabricated X-ray MMAs, each containing 28 mirror shells. ART-XC is currently mapping the sky in the 4-30 keV hard X-ray energy range, studying exotic objects like neutron stars in our own galaxy as well as active galactic nuclei, which are spread across the visible universe. In 2021, the Imaging X-ray Polarimetry Explorer (IXPE), flew and is now performing extraordinary science with an MSFC-led team using three, 24-shell MMAs that were fabricated and calibrated in-house.
      Most recently, in 2024, the fourth FOXSI sounding rocket campaign launched with a high-resolution MSFC MMA. The optics achieved 9.5 arcsecond HPD angular resolution during pre-flight test with an expected 7 arcsecond HPD in gravity-free flight, making this the highest angular resolution flight observation made with a nickel-replicated X-ray optic. Currently MSFC is fabricating an MMA for the Rocket Experiment Demonstration of a Soft X-ray (REDSoX) polarimeter, a sounding rocket mission that will fly a novel soft X-ray polarimeter instrument to observe active galactic nuclei. The REDSoX MMA optic will be 444 mm in diameter, which will make it the largest MMA ever produced by MSFC and the second largest replicated nickel X-ray optic in the world.
      Scientists Wayne Baumgartner (left, crouched) and Nick Thomas (left, standing) calibrate an IXPE MMA in the MSFC 100 m Beamline. Scientist Stephen Bongiorno (right) applies epoxy to an IXPE shell during MMA assembly. NASA MSFC The ultimate performance of an X-ray optic is determined by errors in the shape, position, and roughness of the optical surface. To push the performance of X-ray optics toward even higher angular resolution and achieve more ambitious science goals, MSFC is currently engaged in a fundamental research and development effort to improve all aspects of full-shell optics fabrication.
      Given that these optics are made with the Electroformed Nickel Replication technique, the fabrication process begins with creation of a replication master, called the mandrel, which is a negative of the desired optical surface. First, the mandrel is figured and polished to specification, then a thin layer of nickel alloy is electroformed onto the mandrel surface. Next, the nickel alloy layer is removed to produce a replicated optical shell, and finally the thin shell is attached to a stiff holding structure for use.
      Each step in this process imparts some degree of error into the final replicated shell. Research and development efforts at MSFC are currently concentrating on reducing distortion induced during the electroforming metal deposition and release steps. Electroforming-induced distortion is caused by material stress built into the electroformed material as it deposits onto the mandrel. Decreasing release-induced distortion is a matter of reducing adhesion strength between the shell and mandrel, increasing strength of the shell material to prevent yielding, and reducing point defects in the release layer.
      Additionally, verifying the performance of these advanced optics requires world-class test facilities. The basic premise of testing an optic designed for X-ray astrophysics is to place a small, bright X-ray source far away from the optic. If the angular size of the source, as viewed from the optic, is smaller than the angular resolution of the optic, the source is effectively simulating X-ray starlight. Due to the absorption of X-rays by air, the entire test facility light path must be placed inside a vacuum chamber.
      At MSFC, a group of scientists and engineers operate the Marshall 100-meter X-ray beamline, a world-class end-to-end test facility for flight and laboratory X-ray optics, instruments, and telescopes. As per the name, it consists of a 100-meter-long vacuum tube with an 8-meter-long, 3-meter-diameter instrument chamber and a variety of X-ray sources ranging from 0.25 – 114 keV. Across the street sits the X-Ray and Cryogenic Facility (XRCF), a 527-meter-long beamline with an 18-meter-long, 6-meter-diameter instrument chamber. These facilities are available for the scientific community to use and highlight the comprehensive optics development and test capability that Marshall is known for.
      Within the X-ray astrophysics community there exist a variety of angular resolution and effective area needs for focusing optics. Given its storied history in X-ray optics, MSFC is uniquely poised to fulfill requirements for large or small, medium- or high-angular-resolution X-ray optics. To help guide technology development, the astrophysics community convenes once per decade to produce a decadal survey. The need for high-angular-resolution and high-throughput X-ray optics is strongly endorsed by the National Academies of Sciences, Engineering, and Medicine report, Pathways to Discovery in Astronomy and Astrophysics for the 2020s.In pursuit of this goal, MSFC is continuing to advance the state of the art in full-shell optics. This work will enable the extraordinary mysteries of the X-ray universe to be revealed.
      Project Leads
      Dr. Jessica Gaskin and Dr. Stephen Bongiorno, NASA Marshall Space Flight Center (MSFC)
      Sponsoring Organizations
      The NASA Astrophysics Division supports this work primarily through the Internal Scientist Funding Model Direct Work Package and competed solicitations. This work is also supported by the Heliophysics Division through competed solicitations, as well as by directed work from other government entities.
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      Last Updated Oct 15, 2024 Related Terms
      Astrophysics Astrophysics Division Marshall Astrophysics Marshall Space Flight Center Science-enabling Technology Technology Highlights Explore More
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    • By NASA
      A SpaceX Falcon Heavy rocket carrying NASA’s Europa Clipper spacecraft lifts off from Launch Complex 39A at NASA’s Kennedy Space Center in Florida at 12:06 p.m. EDT on Monday, Oct. 14, 2024. After launch, the spacecraft plans to fly by Mars in February 2025, then back by Earth in December 2026, using the gravity of each planet to increase its momentum. With help of these “gravity assists,” Europa Clipper will achieve the velocity needed to reach Jupiter in April 2030.Credit: NASA/Kim Shiflett NASA’s Europa Clipper has embarked on its long voyage to Jupiter, where it will investigate Europa, a moon with an enormous subsurface ocean that may have conditions to support life. The spacecraft launched at 12:06 p.m. EDT Monday aboard a SpaceX Falcon Heavy rocket from Launch Pad 39A at NASA’s Kennedy Space Center in Florida.
      The largest spacecraft NASA ever built for a mission headed to another planet, Europa Clipper also is the first NASA mission dedicated to studying an ocean world beyond Earth. The spacecraft will travel 1.8 billion miles (2.9 billion kilometers) on a trajectory that will leverage the power of gravity assists, first to Mars in four months and then back to Earth for another gravity assist flyby in 2026. After it begins orbiting Jupiter in April 2030, the spacecraft will fly past Europa 49 times.
      “Congratulations to our Europa Clipper team for beginning the first journey to an ocean world beyond Earth,” said NASA Administrator Bill Nelson. “NASA leads the world in exploration and discovery, and the Europa Clipper mission is no different. By exploring the unknown, Europa Clipper will help us better understand whether there is the potential for life not just within our solar system, but among the billions of moons and planets beyond our Sun.”
      Approximately five minutes after liftoff, the rocket’s second stage fired up and the payload fairing, or the rocket’s nose cone, opened to reveal Europa Clipper. About an hour after launch, the spacecraft separated from the rocket. Ground controllers received a signal soon after, and two-way communication was established at 1:13 p.m. with NASA’s Deep Space Network facility in Canberra, Australia. Mission teams celebrated as initial telemetry reports showed Europa Clipper is in good health and operating as expected.
      “We could not be more excited for the incredible and unprecedented science NASA’s Europa Clipper mission will deliver in the generations to come,” said Nicky Fox, associate administrator, Science Mission Directorate at NASA Headquarters in Washington. “Everything in NASA science is interconnected, and Europa Clipper’s scientific discoveries will build upon the legacy that our other missions exploring Jupiter — including Juno, Galileo, and Voyager — created in our search for habitable worlds beyond our home planet.”
      The main goal of the mission is to determine whether Europa has conditions that could support life. Europa is about the size of our own Moon, but its interior is different. Information from NASA’s Galileo mission in the 1990s showed strong evidence that under Europa’s ice lies an enormous, salty ocean with more water than all of Earth’s oceans combined. Scientists also have found evidence that Europa may host organic compounds and energy sources under its surface.
      If the mission determines Europa is habitable, it may mean there are more habitable worlds in our solar system and beyond than imagined.
      “We’re ecstatic to send Europa Clipper on its way to explore a potentially habitable ocean world, thanks to our colleagues and partners who’ve worked so hard to get us to this day,” said Laurie Leshin, director, NASA’s Jet Propulsion Laboratory in Southern California. “Europa Clipper will undoubtedly deliver mind-blowing science. While always bittersweet to send something we’ve labored over for years off on its long journey, we know this remarkable team and spacecraft will expand our knowledge of our solar system and inspire future exploration.”
      In 2031, the spacecraft will begin conducting its science-dedicated flybys of Europa. Coming as close as 16 miles (25 kilometers) to the surface, Europa Clipper is equipped with nine science instruments and a gravity experiment, including an ice-penetrating radar, cameras, and a thermal instrument to look for areas of warmer ice and any recent eruptions of water. As the most sophisticated suite of science instruments NASA has ever sent to Jupiter, they will work in concert to learn more about the moon’s icy shell, thin atmosphere, and deep interior.
      To power those instruments in the faint sunlight that reaches Jupiter, Europa Clipper also carries the largest solar arrays NASA has ever used for an interplanetary mission. With arrays extended, the spacecraft spans 100 feet (30.5 meters) from end to end. With propellant loaded, it weighs about 13,000 pounds (5,900 kilograms).
      In all, more than 4,000 people have contributed to Europa Clipper mission since it was formally approved in 2015.
      “As Europa Clipper embarks on its journey, I’ll be thinking about the countless hours of dedication, innovation, and teamwork that made this moment possible,” said Jordan Evans, project manager, NASA JPL. “This launch isn’t just the next chapter in our exploration of the solar system; it’s a leap toward uncovering the mysteries of another ocean world, driven by our shared curiosity and continued search to answer the question, ‘are we alone?’”
      More About Europa Clipper
      Europa Clipper’s three main science objectives are to determine the thickness of the moon’s icy shell and its 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.
      Managed by Caltech in Pasadena, California, NASA JPL leads the development of the Europa Clipper mission in partnership with the Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland, for NASA’s Science Mission Directorate in Washington. The main spacecraft body was designed by APL in collaboration with NASA JPL and NASA’s Goddard Space Flight Center in Greenbelt, Maryland, NASA’s Marshall Space Flight Center in Huntsville, Alabama, and NASA’s Langley Research Center in Hampton, Virginia. The Planetary Missions Program Office at Marshall executes program management of the Europa Clipper mission.
      NASA’s Launch Services Program, based at NASA Kennedy, managed the launch service for the Europa Clipper spacecraft.
      Find more information about NASA’s Europa Clipper mission here:
      https://science.nasa.gov/mission/europa-clipper
      -end-
      Meira Bernstein / Karen Fox
      Headquarters, Washington
      202-358-1600
      meira.b.bernstein@nasa.gov / karen.c.fox@nasa.gov
      Gretchen McCartney
      Jet Propulsion Laboratory, Pasadena, Calif.
      818-287-4115
      gretchen.p.mccartney@jpl.nasa.gov
      Share
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      Last Updated Oct 14, 2024 EditorJessica TaveauLocationNASA Headquarters Related Terms
      Europa Clipper Europa Jet Propulsion Laboratory Jupiter Jupiter Moons Kennedy Space Center View the full article
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