Showing posts with label space. Show all posts
Showing posts with label space. Show all posts

Thursday, April 16, 2015

NGC 1788 and the Witch s Whiskers

NGC 1788 and the Witch s Whiskers: APOD: 2013 April 19 - NGC 1788 and the Witch's Whiskers


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2013 April 19


See Explanation. Clicking on the picture will download the highest resolution version available.
Explanation: This skyscape finds an esthetic balance of interstellar dust and gas residing in the suburbs of the nebula rich constellation of Orion. Reflecting the light of bright star Rigel, Beta Orionis, the jutting, bluish chin of the Witch Head Nebula is at the upper left. Whiskers tracing the red glow of hydrogen gas ionized by ultraviolet starlight seem to connect that infamous visage with smaller nebulae, like dusty reflection nebula NGC 1788 at the right. Strong winds from Orion's bright stars have also shaped NGC 1788, and likely triggered the formation of the young stars within. Appropriate for its location, NGC 1788 looks to some like a cosmic bat. The scene spans about 3 degrees on the sky or 6 full Moons.

Grand Spiral Galaxy M81 and Arps Loop

Grand Spiral Galaxy M81 and Arps Loop: APOD: 2013 April 16 - Grand Spiral Galaxy M81 and Arp's Loop


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2013 April 16


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Grand Spiral Galaxy M81 and Arp's Loop

Image Credit & Copyright: Bernard Miller
Explanation: One of the brightest galaxies in planet Earth's sky is similar in size to our Milky Way Galaxy: big, beautiful M81. This grand spiral galaxy lies 11.8 million light-years away toward the northern constellation of the Great Bear (Ursa Major). The deep image of the region reveals details in the bright yellow core, but at the same time follows fainter features along the galaxy's gorgeous blue spiral arms and sweeping dust lanes. It also follows the expansive, arcing feature, known as Arp's loop, that seems to rise from the galaxy's disk at the upper right. Studied in the 1960s, Arp's loop has been thought to be a tidal tail, material pulled out of M81 by gravitational interaction with its large neighboring galaxy M82. But a subsequent investigation demonstrates that at least some of Arp's loop likely lies within our own galaxy. The loop's colors in visible and infrared light match the colors of pervasive clouds of dust, relatively unexplored galactic cirrus only a few hundred light-years above the plane of the Milky Way. Along with the Milky Way's stars, the dust clouds lie in the foreground of this remarkable view. M81's dwarf companion galaxy, Holmberg IX, can be seen just above the large spiral. On the sky, this image spans about 0.5 degrees, about the size of the Full Moon.

Star Factory Messier 17

Star Factory Messier 17: APOD: 2013 April 18 - Star Factory Messier 17


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2013 April 18


See Explanation. Clicking on the picture will download the highest resolution version available.
Explanation: Sculpted by stellar winds and radiation, the star factory known as Messier 17 lies some 5,500 light-years away in the nebula-rich constellation Sagittarius. At that distance, this degree wide field of view spans almost 100 light-years. The sharp, composite, color image utilizing data from space and ground based telescopes, follows faint details of the region's gas and dust clouds against a backdrop of central Milky Way stars. Stellar winds and energetic light from hot, massive stars formed from M17's stock of cosmic gas and dust have slowly carved away at the remaining interstellar material producing the cavernous appearance and undulating shapes. M17 is also known as the Omega Nebula or the Swan Nebula.

IC 1848: The Soul Nebula

IC 1848: The Soul Nebula: APOD: 2013 April 15 - IC 1848: The Soul Nebula


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2013 April 15


See Explanation. Clicking on the picture will download the highest resolution version available.
Explanation: Stars are forming in the Soul of the Queen of Aethopia. More specifically, a large star forming region called the Soul Nebula can be found in the direction of the constellation Cassiopeia, who Greek mythology credits as the vain wife of a King who long ago ruled lands surrounding the upper Nile river. The Soul Nebula houses several open clusters of stars, a large radio source known as W5, and huge evacuated bubbles formed by the winds of young massive stars. Located about 6,500 light years away, the Soul Nebula spans about 100 light years and is usually imaged next to its celestial neighbor the Heart Nebula (IC 1805). The above image appears mostly red due to the emission of a specific color of light emitted by excited hydrogen gas.

NGC 3132: The Southern Ring Nebula

NGC 3132: The Southern Ring Nebula: APOD: 2013 April 9 - NGC 3132: The Southern Ring Nebula


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2013 April 9


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Explanation: It's the dim star, not the bright one, near the center of NGC 3132 that created this odd but beautiful planetary nebula. Nicknamed the Eight-Burst Nebula and the Southern Ring Nebula, the glowing gas originated in the outer layers of a star like our Sun. In this reprocessed color picture, the hot purplish pool of light seen surrounding this binary system is energized by the hot surface of the faint star. Although photographed to explore unusual symmetries, it's the asymmetries that help make this planetary nebula so intriguing. Neither the unusual shape of the surrounding cooler shell nor the structure and placements of the cool filamentary dust lanes running across NGC 3132 are well understood.

M64: The Black Eye Galaxy

M64: The Black Eye Galaxy: APOD: 2013 April 4 - M64: The Black Eye Galaxy


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2013 April 4


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Explanation: This beautiful, bright, spiral galaxy is Messier 64, often called the Black Eye Galaxy or the Sleeping Beauty Galaxy for its heavy-lidded appearance in telescopic views. M64 is about 17 million light-years distant in the otherwise well-groomed northern constellation Coma Berenices. In fact, the Red Eye Galaxy might also be an appropriate moniker in this colorful composition of narrow and wideband images. The enormous dust clouds obscuring the near-side of M64's central region are laced with the telltale reddish glow of hydrogen associated with star forming regions. But they are not this galaxy's only peculiar feature. Observations show that M64 is actually composed of two concentric, counter-rotating systems. While all the stars in M64 rotate in the same direction as the interstellar gas in the galaxy's central region, gas in the outer regions, extending to about 40,000 light-years, rotates in the opposite direction. The dusty eye and bizarre rotation is likely the result of a billion year old merger of two different galaxies.

Comet PANSTARRS and the Andromeda Galaxy

Comet PANSTARRS and the Andromeda Galaxy: APOD: 2013 April 3 - Comet PANSTARRS and the Andromeda Galaxy


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2013 April 3


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Comet PANSTARRS and the Andromeda Galaxy

Image Credit & Copyright: Pavel Smilyk
Explanation: Currently, comet PANSTARRS is passing nearly in front of the galaxy Andromeda. Coincidentally, both comet and galaxy appear now to be just about the same angular size. In physical size, even though Comet PANSTARRS is currently the largest object in the Solar System with a tail spanning about 15 times the diameter of the Sun, it is still about 70 billion times smaller than the Andromeda galaxy (M31). The above image was captured on March 30, near Syktyvkar, Russia. As C/2011 L4 (PANSTARRS) on the lower left recedes from the Sun and dims, it is returning to the northerly direction whence it came. When the comet will return is currently unknown, although humans may have merged with computers by then.

Horsehead: A Wider View

Horsehead: A Wider View: APOD: 2013 May 3 - Horsehead: A Wider View


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2013 May 3


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Explanation: Combined image data from the massive, ground-based VISTA telescope and the Hubble Space Telescope was used to create this wide perspective of the interstellar landscape surrounding the famous Horsehead Nebula. Captured at near-infrared wavelengths, the region's dusty molecular cloud sprawls across the scene that covers an angle about two-thirds the size of the Full Moon on the sky. Left to right the frame spans just over 10 light-years at the Horsehead's estimated distance of 1,600 light-years. Also known as Barnard 33, the still recognizable Horsehead Nebula stands at the upper right, the near-infrared glow of a dusty pillar topped with newborn stars. Below and left, the bright reflection nebula NGC 2023 is itself the illuminated environs of a hot young star. Obscuring clouds below the base of the Horsehead and on the outskirts of NGC 2023 show the tell-tale far red emission of energetic jets, known as Herbig-Haro objects, also associated with newborn stars.

Hungarian Spring Eclipse

Hungarian Spring Eclipse: APOD: 2013 May 4 - Hungarian Spring Eclipse


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2013 May 4


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Explanation: Last week, as the Sun set a Full Moon rose over the springtime landscape of Tihany, Hungary on the northern shores of Lake Balaton. As it climbed into the clear sky, the Moon just grazed the dark, umbral shadow of planet Earth in the year's first partial lunar eclipse. The partial phase, seen near the top of this frame where the lunar disk is darkened along the upper limb, lasted for less than 27 minutes. Composited from consecutive exposures, the picture presents the scene's range of natural colors and subtle shading apparent to the eye. At next week's New Moon, the season's celestial shadow play will continue with an annular solar eclipse, the path of annularity tracking through northern Australia and the central Pacific.

A Supercell Thunderstorm Cloud Over Montana

A Supercell Thunderstorm Cloud Over Montana: APOD: 2013 May 5 - A Supercell Thunderstorm Cloud Over Montana


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2013 May 5


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A Supercell Thunderstorm Cloud Over Montana

Image Credit & Copyright: Sean R. Heavey
Explanation: Is that a spaceship or a cloud? Although it may seem like an alien mothership, it's actually a impressive thunderstorm cloud called a supercell. Such colossal storm systems center on mesocyclones -- rotating updrafts that can span several kilometers and deliver torrential rain and high winds including tornadoes. Jagged sculptured clouds adorn the supercell's edge, while wind swept dust and rain dominate the center. A tree waits patiently in the foreground. The above supercell cloud was photographed in July west of Glasgow, Montana, USA, caused minor damage, and lasted several hours before moving on.

Tails of Comet Lemmon

Tails of Comet Lemmon: APOD: 2013 May 6 - Tails of Comet Lemmon


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2013 May 6


See Explanation. Clicking on the picture will download the highest resolution version available.
Explanation: What caused the interestingly intricate tails that Comet Lemmon displayed earlier this year? First of all, just about every comet that nears the Sun displays two tails: a dust tail and an ion tail. Comet Lemmon's dust tail, visible above and around the comet nucleus in off-white, is produced by sun-light reflecting dust shed by the comet's heated nucleus. Flowing and more sculptured, however, is C/2012 F6 (Lemmon)'s blue ion tail, created by the solar wind pushing ions expelled by the nucleus away from the Sun. Also of note is the coma seen surrounding Comet Lemmon's nucleus, tinted green by diatomic C2 gas fluorescing in sunlight. The above image was taken from the dark skies of Namibia in mid-April. Comet Lemmon is fading as it now heads back to the outer Solar System.

Galaxy Cove Vista

Galaxy Cove Vista: APOD: 2013 May 7 - Galaxy Cove Vista


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2013 May 7


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Explanation: To see a vista like this takes patience, hiking, and a camera. Patience was needed in searching out just the right place and waiting for just the right time. A short hike was needed to reach this rugged perch above a secluded cove in Julia Pfeiffer Burns State Park in California, USA. And a camera was needed for the long exposure required to bring out the faint light from stars and nebulae in the background Milky Way galaxy. Moonlight and a brief artificial flash illuminated the hidden beach and inlet behind nearby trees in the above composite image taken about two weeks ago. Usually obscured McWay Falls is visible just below the image center, while the Pacific Ocean is in view to its right.

Mystic Mountain Dust Pillars

Mystic Mountain Dust Pillars: APOD: 2015 April 15 - Mystic Mountain Dust Pillars


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2015 April 15


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Explanation: It's stars versus dust in the Carina Nebula and the stars are winning. More precisely, the energetic light and winds from massive newly formed stars are evaporating and dispersing the dusty stellar nurseries in which they formed. Located in the Carina Nebula and known informally as Mystic Mountain, these pillar's appearance is dominated by the dark dust even though it is composed mostly of clear hydrogen gas. Dust pillars such as these are actually much thinner than air and only appear as mountains due to relatively small amounts of opaque interstellar dust. About 7,500 light-years distant, the featured image was taken with the Hubble Space Telescope, digitally reprocessed by an industrious amateur, and highlights an interior region of Carina which spans about three light years. Within a few million years, the stars will likely win out completely and the entire dust mountain will be destroyed.

Colossal Ancient Galaxies Die from the Inside Out

Colossal Ancient Galaxies Die from the Inside Out:


by Elizabeth Howell, Space.com Contributor

Date: 16 April 2015 Time: 02:01 PM ET

Elliptical Galaxy IC 2006
The elliptical galaxy IC 2006 as seen by the Hubble Space Telescope. A new study suggests that the most massive elliptical galaxies stopped star formation near their centers roughly three billion years after the Big Bang

CREDIT: ESA/Hubble & NASA


The largest ancient galaxies stopped forming stars in their cores about three billion years after the Big Bang, with this end of star birth spreading from the inside out in so-called "dead" galaxies, scientists say.

A new survey of 22 elliptical galaxies (most of which were the same size or larger than our own Milky Way) revealed that the most massive galaxies from about 10 billion years ago have stopped forming stars in their centers while formation continued on the outskirts.

"These galaxies lived 10 billion years in the past — three billion years after the Big Bang — and are star-forming at high rates, and are the progenitors of the massive dead galaxies of today's universe," lead author Sandro Tacchella, a Ph.D. student at ETH Zurich's institute for astronomy in Switzerland, told Space.com. [Top 10 Star Mysteries of All Time]

The survey of ancient elliptical galaxies adds fuel to an ongoing debate about how the star shutdown occurs. One leading theory says that a supermassive black hole drives gas out and disrupts star formation, while the other supposes there is a yet-unexplained mechanism that switches off the gas supply in the center.

Tacchella said data from his study would support either of these two contentions, or even a combination of the two. Also interesting was the smaller, elliptical galaxies from this era were still churning out stars throughout their masses. Why is still poorly understood.

"The smaller galaxies are doubling their mass at the same pace in their inner and outer parts," he said. He added this same phenomenon was observed in younger galaxies closer to us.

'Red and Dead' Galaxy
This graphic shows how star formation stops in the heart of an elliptical galaxy, then spreads out to the outermost edges to create a so-called "red and dead" galaxy.
Credit: European Southern Observatory

Solving the mystery

Tacchella said he tackled this research problem because he is interested in how galaxies form stars in terms of physical mechanisms.

Figuring out what stopped the star formation in these massive galaxies will require more observations, he said. Astronomers call these elliptical galaxies "red and dead" as they contain a lot of old, dead red stars, but fewer blue youngsters.

The study of 22 galaxies ate up 300 hours of observing time between the orbiting Hubble Space Telescope and the European Southern Observatory's Very Large Telescope in Chile. The VLT looked at the spectra (light distribution) of stars, showing where the young ones were. Hubble was used to trace the older stars, showing the stellar mass distribution of galaxies.

The sheer amount of time would be difficult to replicate given the high observing time demands on these observatories, Tacchella said. He plans a further, focused study with Hubble that will look at the 10 largest galaxies to study their star formation habits more closely.

Better resolution will soon be available to astronomers as well as new observatories come online that can peer further back in time to galaxies that formed closer to the Big Bang, Tacchella said.

NASA's James Webb Space Telescope is set to fly in 2018. On the ground, the most massive optical telescope in the world – the European Extremely Large Telescope (E-ELT), with a 39-meter (128-foot) mirror – is expected to be finished by 2024.

The research was published today in the April 16 edition of the journal Science.

Follow Elizabeth Howell @howellspace, or Space.com @Spacedotcom. We're also on Facebook and Google+. Originally published on Space.com.

Tuesday, April 14, 2015

Galaxy Cove Vista

Galaxy Cove Vista: APOD: 2013 May 7 - Galaxy Cove Vista


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2013 May 7


See Explanation. Clicking on the picture will download the highest resolution version available.
Explanation: To see a vista like this takes patience, hiking, and a camera. Patience was needed in searching out just the right place and waiting for just the right time. A short hike was needed to reach this rugged perch above a secluded cove in Julia Pfeiffer Burns State Park in California, USA. And a camera was needed for the long exposure required to bring out the faint light from stars and nebulae in the background Milky Way galaxy. Moonlight and a brief artificial flash illuminated the hidden beach and inlet behind nearby trees in the above composite image taken about two weeks ago. Usually obscured McWay Falls is visible just below the image center, while the Pacific Ocean is in view to its right.

Earth's Major Telescopes Investigate GRB 130427A

Earth's Major Telescopes Investigate GRB 130427A: APOD: 2013 May 8 - Earth's Major Telescopes Investigate GRB 130427A


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2013 May 8


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Earth's Major Telescopes Investigate GRB 130427A

Illustration Credit: NASA, DOE, Fermi LAT Collaboration
Explanation: A tremendous explosion has occurred in the nearby universe and major telescopes across Earth and space are investigating. Dubbed GRB 130427A, the gamma-ray burst was first detected by the Earth-orbiting Fermi and Swift satellites observing at high energies and quickly reported down to Earth. Within three minutes, the half-meter ISON telescope in New Mexico found the blast in visible light, noted its extreme brightness, and relayed more exact coordinates. Within the next few minutes, the bright optical counterpart was being tracked by several quickly re-pointable telescopes including the 2.0-meter P60 telescope in California, the 1.3-meter PAIRITEL telescope in Arizona, and the 2.0-meter Faulkes Telescope North in Hawaii. Within two hours, the 8.2-meter Gemini North telescope in Hawaii noted a redshift of 0.34, placing the explosion about 5 billion light years away -- considered nearby in cosmological terms. Previously recorded images from the RAPTOR full-sky monitors were scanned and a very bright optical counterpart -- magnitude 7.4 -- was found 50 seconds before the Swift trigger. The brightest burst in recent years, a signal from GRB 130427A has also been found in low energy radio waves by the Very Large Array (VLA) and at the highest energies ever recorded by the Fermi satellite. Neutrino, gravitational wave, and telescopes designed to detect only extremely high energy photons are checking their data for a GRB 130427A signal. Pictured in the above animation, the entire gamma-ray sky is shown becoming momentarily dominated by the intense glow of GRB 130427A. Continued tracking the optical counterpart will surely be ongoing as there is a possibility that the glow of a classic supernova will soon emerge.

Cape York Annular Eclipse

Cape York Annular Eclipse: APOD: 2013 May 11 - Cape York Annular Eclipse


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2013 May 11


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Cape York Annular Eclipse

Image Credit & Copyright: Cameron McCarty, Matthew Bartow, Michael Johnson -

MWV Observatory, Coca-Cola Space Science Center, Columbus State University Eclipse Team
Explanation: This week the shadow of the New Moon fell on planet Earth, crossing Queensland's Cape York in northern Australia ... for the second time in six months. On the morning of May 10, the Moon's apparent size was too small to completely cover the Sun though, revealing a "ring of fire" along the central path of the annular solar eclipse. Near mid-eclipse from Coen, Australia, a webcast team captured this telescopic snapshot of the annular phase. Taken with a hydrogen-alpha filter, the dramatic image finds the Moon's silhouette just within the solar disk, and the limb of the active Sun spiked with solar prominences. Still, after hosting back-to-back solar eclipses, northern Australia will miss the next and final solar eclipse of 2013. This November, a rare hybrid eclipse will track across the North Atlantic and equatorial Africa.

Kepler's Supernova Remnant in X Rays

Kepler's Supernova Remnant in X Rays: APOD: 2013 May 15 - Kepler's Supernova Remnant in X-Rays


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2013 May 15


See Explanation. Clicking on the picture will download the highest resolution version available.
Kepler's Supernova Remnant in X-Rays

Image Credit: X-ray: NASA/CXC/NCSU/M. Burkey et al. Optical: DSS
Explanation: What caused this mess? Some type of star exploded to create the unusually shaped nebula known as Kepler's supernova remnant, but which type? Light from the stellar explosion that created this energized cosmic cloud was first seen on planet Earth in October 1604, a mere four hundred years ago. The supernova produced a bright new star in early 17th century skies within the constellation Ophiuchus. It was studied by astronomer Johannes Kepler and his contemporaries, without the benefit of a telescope, as they searched for an explanation of the heavenly apparition. Armed with a modern understanding of stellar evolution, early 21st century astronomers continue to explore the expanding debris cloud, but can now use orbiting space telescopes to survey Kepler's supernova remnant (SNR) across the spectrum. Recent X-ray data and images of Kepler's supernova remnant taken by the orbiting Chandra X-ray Observatory has shown relative elemental abundances typical of a Type Ia supernova, and further indicated that the progenitor was a white dwarf star that exploded when it accreted too much material from a companion Red Giant star and went over Chandrasekhar's limit. About 13,000 light years away, Kepler's supernova represents the most recent stellar explosion seen to occur within our Milky Way galaxy.

Four X-class Flares

Four X-class Flares: APOD: 2013 May 16 - Four X-class Flares


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2013 May 16


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Explanation: Swinging around the Sun's eastern limb on Monday, a group of sunspots labeled active region AR1748 has produced the first four X-class solar flares of 2013 in less than 48 hours. In time sequence clockwise from the top left, flashes from the four were captured in extreme ultraviolet images from the Solar Dynamics Observatory. Ranked according to their peak brightness in X-rays, X-class flares are the most powerful class and are frequently accompanied by coronal mass ejections (CMEs), massive clouds of high energy plasma launched into space. But CMEs from the first three flares were not Earth-directed, while one associated with the fourth flare may deliver a glancing blow to the Earth's magnetic field on May 18. Also causing temporary radio blackouts, AR1748 is likely not finished. Still forecast to have a significant chance of producing strong flares, the active region is rotating into more direct view across the Sun's nearside.

Comet PanSTARRS with Anti Tail

Comet PanSTARRS with Anti Tail: APOD: 2013 May 18 - Comet PanSTARRS with Anti Tail


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2013 May 18


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Explanation: Once the famous sunset comet, PanSTARRS (C/2011 L4) is now visible all night from much of the northern hemisphere, bound for the outer solar system as it climbs high above the ecliptic plane. Dimmer and fading, the comet's broad dust tail is still growing, though. This widefield telescopic image was taken against the starry background of the constellation Cepheus on May 15. It shows the comet has developed an extensive anti-tail, dust trailing along the comet's orbit (to the left of the coma), stretching more than 3 degrees across the frame. Since the comet is just over 1.6 astronomical units from planet Earth, that corresponds to a distance of over 12 million kilometers. In late May Comet PanSTARRS will pass within a few degrees of the north celestial pole.