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Toolkit

Key Resources

Where Is New Horizons Now?

Computer-generated images show the location of New Horizons in the solar system.

Featured Images
LORRI Images from the Pluto Encounter

View images taken by the LOng Range Reconnaissance Imager (LORRI) on the New Horizons spacecraft. LORRI is the most sensitive and highest resolution imager aboard New Horizons.

Eyes on the Solar System

Using Eyes on the Solar System and simulated data from the New Horizons flight team you can ride onboard the spacecraft using "Eyes on Pluto" on your Mac or PC.

NASA EDGE

In recognition of New Horizons' upcoming closest approach to Pluto, NASA EDGE sets out on their own parallel mission to Pluto, West Virginia. Along their journey, NASA EDGE interviews experts involved with this amazing mission, and they even meet the authors and illustrator of the popular children's book, "Pluto's Secret." Franklin talks to people on the street about Pluto's planetary status, and despite the Co-Host's struggles with basic navigation, both missions are right on track.

Press Kits

Fact Sheets



Imagery

Models

New Horizons Cut Out Model

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Build Your Own New Horizons Spacecraft (Ages 10+)

Best suited for ages 10+, build a scale model of the New Horizons spacecraft!

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Make a Model of the Pluto/Charon System (All Ages)

Pluto and Charon are a binary system. Build your own model of a binary system and see what makes it so unique! With adult help, children of any age will enjoy this activity.

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Model Design Diagram

View the New Horizons spacecraft model design diagram!

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Spacecraft Model Files

Build your own 3D New Horizons spacecraft model. Below is a zipped file of .stl-formatted printable models including instructions for printing and assembly. We understand that 3D printing often involves trial and error. You may make adjustments or changes when printing these models.

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Bennu & MU69

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About the Kuiper Belt

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Ultima Flyby

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Exhibit Artwork

Beyond Pluto Backdrop #1

8'x10'

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Beyond Pluto Backdrop #2

8'x10'

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Beyond Pluto Backdrop #3

8'x10'

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Beyond Pluto Banner Sign Artwork #1

6'x2.5'

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Beyond Pluto Banner Sign Artwork #2

6'x2.5'

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Beyond Pluto Banner Sign Artwork #3

6'x2.5'

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Beyond Pluto Banner Sign Artwork #4

6'x2.5'

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Beyond Pluto Banner Sign Artwork #5

6'x2.5'

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General Mission Banner Sign Artwork

6'x2.5'

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I "HEART" Pluto Backdrop Artwork

8'x10'

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KBO January 1, 2019 Artwork

8'x10'

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Pluto Explored Backdrop Artwork

8'x10'

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Postcard from Pluto Backdrop Artwork

8'x10'

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Plutopalooza

Plutopalooza Banner Sign Artwork

2.5'x6'

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Plutopalooza Bookmark

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PlutopaloozaKBO Banner Sign Artwork

2.6'x7.2'

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Post Pluto Flyby Plutopalooza Sticker/Artwork

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Posters

KBO Iconic Poster

36" x 50" Poster

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Printables

Ultima Thule Flyby Postcard

Two Sided Postcard

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Kuiper Belt Extended Mission Decal

NASA's New Horizons spacecraft reached Pluto and its moons in July 2015, revolutionizing our understanding of these mysterious worlds on the outer edge of our solar system. On New Year's Day 2019, a billion miles beyond Pluto, New Horizons will fly past a small, frozen Kuiper Belt object named 2014 MU69 - the most distant object ever explored by a spacecraft.

NASA, the Southwest Research Institute (SwRI) and the Johns Hopkins Applied Physics Laboratory (APL) lead the New Horizons mission in collaboration with additional government, university and industry partners.

Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute/Dan Durda

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Mission Postcards

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Post Pluto Flyby Mission Sticker

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Pluto Flyby Memories

Maybe it was the first glimpse of Pluto's icy "heart" ... or the countdown to Pluto close approach on the morning of July 14, 2015 ... or the dramatic moment New Horizons "phoned home" to let us know it was alive and well and speeding deeper into the Kuiper Belt. If you have a favorite memory from the historic Pluto flyby, share it below! We'll consider your entry for posting on the New Horizons website and social media accounts.

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Educator Fellows

The New Horizons Educator Fellows Program

This key program develops a cadre of educators who represent the mission and serve as an important resource for Solar System exploration programs across the country. The fellows listed below conduct nationwide teacher training workshops for the mission. The fellows train the participants on the latest and greatest on the mission as well as the key educational materials and products developed by the mission team.

Click on a shaded state on the map to see a list of fellows for that state or view all fellows.


Fellows in All StatesKen Brandt Lumberton, NC

Pamela Casto Fairmont, WV
Walter Charuba Grosse Pointe Farms, MI
Honora Dash Brooklyn, NY
Stacy De Veau Prescott, AZ
Patricia Dutton Fullerton, NH
Alex Eilers Memphis, TN
Barry Fried East Meadow, NY
Lollie Garay Spring, TX
Linda Gauthier Baton Rouge, LA
Gene Gordon Honeoye Falls, NY
Shirley Greene Billings, MT
Jerry Hombel Mead, WA
Rosemary Hyder San Bernardino, CA
Sally Jensen Campton, NH
Deborah Jones Eagle River, AK
Virginia Jones Idaho Falls, ID
Cynthia Keeling Fairmont, WV
Jeff Kilmer Akron, OH
Andy Kreyche Salinas, CA
Erich Landstrom Riviera Beach, FL
Stefanie Long Washington, IL
Randy Monroe Concord, CA
Daniel Newmyer Mosca, CO
Kathleen Newmyer Mosca, CO
Gerri Pukey-Otto Kingsville, MD
Courtney (Townsend) Sevigny Warwick, RI
Tanya Shank Charlotte, NC
Nancy Sills Pine Mountain Valley, GA
Nancy Staudt League City, TX
Nancy Tashima Captain Cook, HI
Julie Taylor Victorville, CA
Michael Uenking Newport News, VA
Gloria Villalobos Toms River, NJ
Kelly Wardlaw Stillwater, OK
April Whitt Atlanta, GA

The New Horizons Parallax Program

#NHparallax
Post your Images

Using software and methods of their choosing, amateur astronomers can combine their images with the New Horizons pictures, and post the 3D parallax products on Twitter, Instagram or other social media with the hashtag #NHparallax. Learn more »

NASA Make and Take Activity

Experience Parallax with Your Thumb! »

Since its launch in January 2006, NASA's New Horizons spacecraft has flown past Jupiter in 2007, Pluto in 2015, and most recently, the Kuiper Belt object Arrokoth in 2019. Speeding through the Kuiper Belt at some 31,000 miles (50,000 kilometers) per hour, it's on a fast path out of the solar system and toward the Milky Way galaxy.

This spring, New Horizons will be more than 46 times farther from the Sun than the Earth, having traveled more than 5 billion miles (8 billion kilometers) since launch. At this great distance, from New Horizons' view, the nearest stars will appear to have shifted in position relative to more distant stars, compared to where we see them from Earth. On April 22 and 23, 2020, New Horizons will gather images of two of the nearest stars, Proxima Centauri and Wolf 359, to demonstrate this effect.

The shift in position of closer stars is known as "stellar parallax," and allows astronomers to measure distances to nearby stars using the radius of Earth's orbit as a baseline distance. Stars at a distance of a single "parsec" have a parallax of one arcsecond, or 1/3600 of a degree in angle. In more familiar units, a parsec is 3.26 light years. An arc second is close to the resolution of most ground-based telescopes, and as all stars (except our Sun) are farther away than a parsec, they have even smaller parallaxes that can only be measured with painstaking work. An important complication is that all stars have their own random drifts through space, which typically cause far larger shifts in position over the course of a year than the parallaxes themselves.

In practice, parallaxes are only visible as an annual back-and-forth motion of a star's position superimposed on its steady drift with respect to other background stars, and are derived from several years of observations. In contrast, observing a star simultaneously from Earth and New Horizons will instantly reveal a large parallax completely unaffected by the star's drift.

Goals of the Parallax Program

The New Horizons parallax program will:

  • Demonstrate vividly the immense distance NASA's New Horizons spacecraft has traveled by showing the parallactic shift of two nearby stars with respect to the more distance background stars seen in the fields around them.
  • Provide a first-ever demonstration of large and "pure" stellar parallaxes. With simultaneous Earth and spacecraft observations of the same stars, the stars' drifts are unimportant. Parallaxes are recovered instantly, not requiring years of observations to isolate the parallaxes as Earth goes around in its orbit, during which the closer stars also drift against distance background stars. Given the large baseline distance provided by New Horizons' location at the outer edge of the Kuiper Belt, the parallaxes will be instantly obvious when comparing Earth-based and New Horizons images.
  • Provide a first-ever demonstration of using stars for interstellar navigation of a spacecraft. With parallax observations of two widely separated stars, the distance and location of the New Horizons spacecraft can be roughly determined. While in practice navigation of New Horizons is done to high accuracy with tracking provided by NASA's Deep Space Network, the parallax images can provide less-accurate, but autonomous of navigation that, in principle, could be done by the spacecraft independently of Earth-based tracking. Optical imagery by robotic planetary missions is used for navigation to bodies within the solar system, but has not been used to establish the interstellar trajectory of a spacecraft heading into the galaxy.
  • Engage interested amateur astronomers around the world in the parallax observations. The stars targeted by New Horizons can also be observed by amateur astronomers with 6-inch or larger telescopes equipped with electronic cameras. New Horizons will provide publicly available images obtained in its parallax program, for comparison to images obtained with amateur telescopes. The New Horizons project will also provide its own demonstration of parallaxes to the public using images obtained by professional observatories involved in the demonstration.

This figure illustrates the phenomenon of stellar parallax. When New Horizons and observers on Earth observe a nearby star at the same time, it appears to be in different places compared to more distant background stars -- this is because New Horizons has traveled so far out in space (nearly 5 billion miles) that it has to look in a different direction to see that star. The small images below Earth and New Horizons show each unique view. Note that the farther-away background stars stay in the same place, but the nearby star appears to move between the two vantage points. (Credit: Pete Marenfeld, NSF's National Optical-Infrared Astronomy Research Laboratory)

This figure, by New Horizons contributing scientist Brian May, shows the parallax as an effect of New Horizons' travels deeper into the Kuiper Belt. Traditionally, parallax is measured as the Earth orbits around the sun. The two lines at left show the lines of sight from Earth to the star on either side of Earth's orbit. This causes a small shift in the position of the nearby star compared to more distant stars. New Horizons is so far away that a much larger shift in the line of sight to the star occurs. (Credit: Brian May)

The Target Stars

Wolf 359

Not counting the Sun, Wolf 359 is the eighth-nearest star to Earth, at a distance of 7.86 light years. The red dwarf star in the constellation of Leo can be observed in the first part of 2020 from both the Northern and Southern hemispheres. It is too faint for direct visual observation by all but the largest amateur-class telescopes, but should be readily captured with electronic cameras on 6-inch telescopes and larger. Wolf 359 is a flare-star, which means that it exhibits random brief but strong increases in luminosity due to energetic events similar to solar flares erupting on our Sun. Wolf 359 has a large annual drift of 4.7 arcseconds with respect to distant background stars.

Did You Know?

Wolf 359 has figured prominently in a number of science fiction stories and productions, notably in episodes of the Outer Limits TV series of the 1960s and Star Trek: The Next Generation.

Proxima Centauri

At 4.244 light years, Proxima Centauri is nearest known star (not counting the Sun, of course). Proxima Centauri is a red dwarf star in the constellation of Centaurus. It is an extremely distant companion to the alpha Centauri binary star, which itself is too bright to be imaged by New Horizons. It has a large southern declination and can be observed at most times of the year by most Southern Hemisphere skywatchers, but is always below the horizon for nearly all Northern Hemisphere observers. Proxima Centauri is at a large angle in the sky from Wolf 359. The two stars establish an excellent reference pair to be used for the interstellar navigation demonstration.

Proxima Centauri can be seen by eye with moderately-sized amateur-class telescopes. It is also a flare-star. Proxima Centauri has a large annual drift of 3.9 arcseconds with respect to distant background stars.

Did You Know?

Proxima Centauri has figured prominently in several science fiction stories, and has often been discussed as a possible target for interstellar probes.

Simultaneous Observations

New Horizons is 2.89 light-hours closer to Proxima Centauri than Earth, but 3.74 light-hours farther from Wolf 359 than Earth -- which means the New Horizons and Earth-based images must be taken at different times to make sure the observations appear to be "simultaneous" in the star-field frames.

Earth-based exposure times are given below. Each star is observed twice by New Horizons in case of flares by either star or bad weather on Earth. The observation date corresponds to the new moon, making it easier for amateur astronomers to locate the star fields in a darker sky.

The first Wolf 359 epoch provides visibility to the full continental United States, eastern Alaska, and all other North and South American sites. The second epoch provides visibility for Hawaii and western Alaska. Proxima Centauri will not be visible to Northern Hemisphere sites above +27° latitude. The first Proxima Centauri epoch provides simultaneous spacecraft visibility for observers in Australia, New Zealand, and other sites at similar longitudes. The second epoch is specified for South and Central American sites. Note that the second Proxima Centauri epoch occurs an hour after the first Wolf 359 epoch.

Observation Dates and Times

These times specify when to observe the two stars and obtain images simultaneously with the New Horizons spacecraft. Any observation obtained within a week of these times, however, will still provide a valid demonstration of the Earth-New Horizons parallaxes.
Wolf 359Proxima Centauri
April 23, 2020 04:00 UTApril 22, 2020 13:00 UT
April 23, 2020 10:00 UTApril 23, 2020 05:00 UT

While simultaneous Earth and spacecraft observations provide the aesthetically purest demonstrations of the parallactic shifts of stars provided by New Horizons' great distance, images can be obtained by any Earth-based observer at any time close enough to the specified epochs. In fact, for both stars, Earth observations obtained within a week of the nominal times above will have negligible drift corrections.

A timeline showing the Earth and spacecraft observation epochs is below. New Horizons will be 4.36 billion miles (7.01 billion kilometers) from Earth, with a one-way light travel time of 6 hours and 30 minutes. At the time, Earth's orbital motion will be faster than New Horizons' cruise velocity, so the spacecraft actually gets closer to Earth during the observation period.

Timeline showing the Earth and spacecraft observation epochs

Finding the Star Fields

Where to find Wolf 359 and Proxima Centauri in the sky? Claudio Martinez, of the AZARA Natural History Foundation, Argentina, created this set of star charts. Martinez leads a team of small telescope observers that hopes to obtain images for the New Horizons parallax program.

Both Wolf 359 and Proxima Centauri are too faint to be seen by the naked eye or even with small telescopes, but can be located by skilled amateur astronomers equipped with electronic cameras and telescopes of 6-inch aperture or larger.

The epoch 2000 RA and Dec coordinates of the stars with proper motion (drift) corrections to Jan. 1, 2020, are:

  • Wolf 359: 10 56 23.665 + 06 59 58.48
  • Proxima Centauri: 14 29 31.962 - 62 40 30.77

Star charts of the Wolf 359 and Proxima Centauri fields are below. The fields of view correspond to that of New Horizons' Long Range Reconnaissance Imager (LORRI), which will be used to obtain the spacecraft images. The target stars are at the center of the field. Note that Wolf 359 has a high galactic latitude and thus has a sparse background, while Proxima Centauri is close to the central plane of the Milky Way and is rich with background stars. The charts are prepared for V-band observations.


Star chart of the Wolf 359 field
Star chart of the Proxima Centauri field

William Keel (University of Alabama, SARA Observatory) has provided color images of the Wolf 359 and Proxima Centauri fields. These were obtained in late 2019, and the large proper motions of both stars (at the center of each image) will cause them to shift by over an arcsecond by April 2020. A green circle provides a rough estimate of where both stars will appear in the New Horizons images. Note that both images cover roughly a quarter of the field shown in the charts. Thanks to image depth and the use of redder filters, the images depict several relatively bright stars that are not visible in the charts.

Color image of Wolf 359 field
Color image of the Proxima Centauri field

Producing a Parallax Effect

The New Horizons team released the star images taken by the spacecraft on June 11, 2020.

Using software and methods of their choosing, amateur astronomers can combine their images with the New Horizons pictures, and post the 3D parallax products on Twitter, Instagram or other social media with the hashtag #NHparallax. The mission team will search this hashtag for the results and post some of these images on the New Horizons website and mission social media accounts.

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