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The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (binary) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens. Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (binary) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens. Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643748

New Horizons near 2014 MU69 - Artist's view - New Horizons near 2014 MU69 - Artwork - Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Artist's concept of the New Horizons spacecraft flying by a possible binary 2014 MU69 on Jan. 1, 2019. Early observations of MU69 hint at the Kuiper Belt object being either a binary orbiting pair or a contact (stuck together) pair of nearly like-sized bodies with diameters near 20 and 18 kilometers (12 and 11 miles)

New Horizons near 2014 MU69 - Artist's view - New Horizons near 2014 MU69 - Artwork - Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Artist's concept of the New Horizons spacecraft flying by a possible binary 2014 MU69 on Jan. 1, 2019. Early observations of MU69 hint at the Kuiper Belt object being either a binary orbiting pair or a contact (stuck together) pair of nearly like-sized bodies with diameters near 20 and 18 kilometers (12 and 11 miles)

Miller, Ron (b.1947)

PIX4946140

Cryovolcan sur Pluto - Artist view - Ice Volcano on Pluto - Artist view: Ice volcano on Pluto

Cryovolcan sur Pluto - Artist view - Ice Volcano on Pluto - Artist view: Ice volcano on Pluto

Miller, Ron (b.1947)

PIX4624582

The New Horizons probe near 2014 MU69 - Artist's view - New Horizons near 2014 MU69 - Artwork - Artist view of the New Horizons probe near the small object of Kuiper 2014 MU69. Artist's concept of the New Horizons spacecraft flying by a possible binary 2014 MU69 on Jan. 1, 2019. Early observations of MU69 hint at the Kuiper Belt object being either a binary orbiting pair or a contact (stuck together) pair of nearly like-sized bodies with diameters near 20 and 18 kilometers (12 and 11 miles)

The New Horizons probe near 2014 MU69 - Artist's view - New Horizons near 2014 MU69 - Artwork - Artist view of the New Horizons probe near the small object of Kuiper 2014 MU69. Artist's concept of the New Horizons spacecraft flying by a possible binary 2014 MU69 on Jan. 1, 2019. Early observations of MU69 hint at the Kuiper Belt object being either a binary orbiting pair or a contact (stuck together) pair of nearly like-sized bodies with diameters near 20 and 18 kilometers (12 and 11 miles)

Miller, Ron (b.1947)

PIX4946180

The New Horizons probe near 2014 MU69 - Artist's view - New Horizons near 2014 MU69 - Artwork - Artist view of the New Horizons probe near the small object of Kuiper 2014 MU69. Artist's concept of the New Horizons spacecraft flying by a possible binary 2014 MU69 on Jan. 1, 2019. Early observations of MU69 hint at the Kuiper Belt object being either a binary orbiting pair or a contact (stuck together) pair of nearly like-sized bodies with diameters near 20 and 18 kilometers (12 and 11 miles)

The New Horizons probe near 2014 MU69 - Artist's view - New Horizons near 2014 MU69 - Artwork - Artist view of the New Horizons probe near the small object of Kuiper 2014 MU69. Artist's concept of the New Horizons spacecraft flying by a possible binary 2014 MU69 on Jan. 1, 2019. Early observations of MU69 hint at the Kuiper Belt object being either a binary orbiting pair or a contact (stuck together) pair of nearly like-sized bodies with diameters near 20 and 18 kilometers (12 and 11 miles)

Miller, Ron (b.1947)

PIX4643713

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (binary) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens. Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (binary) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens. Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643732

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643771

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643784

Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69.

Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69.

Miller, Ron (b.1947)

PIX4643835

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643791

The New Horizons probe near 2014 MU69 - Artist's view - New Horizons near 2014 MU69 - Artwork - Artist view of the New Horizons probe near the small object of Kuiper 2014 MU69. Artist's concept of the New Horizons spacecraft flying by a possible binary 2014 MU69 on Jan. 1, 2019. Early observations of MU69 hint at the Kuiper Belt object being either a binary orbiting pair or a contact (stuck together) pair of nearly like-sized bodies with diameters near 20 and 18 kilometers (12 and 11 miles)

The New Horizons probe near 2014 MU69 - Artist's view - New Horizons near 2014 MU69 - Artwork - Artist view of the New Horizons probe near the small object of Kuiper 2014 MU69. Artist's concept of the New Horizons spacecraft flying by a possible binary 2014 MU69 on Jan. 1, 2019. Early observations of MU69 hint at the Kuiper Belt object being either a binary orbiting pair or a contact (stuck together) pair of nearly like-sized bodies with diameters near 20 and 18 kilometers (12 and 11 miles)

Miller, Ron (b.1947)

PIX4946197

The surface of Charon - Artist view - Charon equatorial chasm - Artist view: Vue d'artiste du gouffre equatorial de Charon

The surface of Charon - Artist view - Charon equatorial chasm - Artist view: Vue d'artiste du gouffre equatorial de Charon

Miller, Ron (b.1947)

PIX4624698

Transneptunian object - Illustration - Transneptunian object - Artwork: The solar system seen from a Transneptunian object, an object from the Kuiper belt object - Solar system seen from a Kuiper belt object

Transneptunian object - Illustration - Transneptunian object - Artwork: The solar system seen from a Transneptunian object, an object from the Kuiper belt object - Solar system seen from a Kuiper belt object

Miller, Ron (b.1947)

PIX4629648

Transneptunian object - Illustration - Transneptunian object - Artwork: The Sun seen from a Transneptunian object, an object from the Kuiper belt object - Sun seen from a Kuiper belt object

Transneptunian object - Illustration - Transneptunian object - Artwork: The Sun seen from a Transneptunian object, an object from the Kuiper belt object - Sun seen from a Kuiper belt object

Miller, Ron (b.1947)

PIX4629677

Pluto vue de Charon - View d'artiste - Pluto seen from Charon - Artist view: View d'artiste de la surface de Charon. Pluto is visible in the sky. Charon surface.

Pluto vue de Charon - View d'artiste - Pluto seen from Charon - Artist view: View d'artiste de la surface de Charon. Pluto is visible in the sky. Charon surface.

Miller, Ron (b.1947)

PIX4624692

Pluto vue de Charon - Vue d'artiste - Pluto seen from Charon - Artist view: Vue d'artiste de la glace à la surface de Charon. Pluto is visible in the sky - Ice on Charon surface

Pluto vue de Charon - Vue d'artiste - Pluto seen from Charon - Artist view: Vue d'artiste de la glace à la surface de Charon. Pluto is visible in the sky - Ice on Charon surface

Miller, Ron (b.1947)

PIX4624674

The dwarf planet Makemake - Illustration -The dwarf planet Makemake: The solar system seen from the dwarf planet Makemake. Makemake (136472 Makemake) is the third largest known dwarf planet. It belongs to the Kuiper belt and was discovered in 2005. Its diameter is about two thirds that of Pluto, or 1,430 km. Solar system seen from Makemake. Makemake (minor-planet designation 136472 Makemake) is a dwarf planet and perhaps the largest Kuiper belt object with a diameter approximately two thirds that of Pluto. Makemake has one known satellite, S/2015 (136472). Makemake was discovered on March 31, 2005

The dwarf planet Makemake - Illustration -The dwarf planet Makemake: The solar system seen from the dwarf planet Makemake. Makemake (136472 Makemake) is the third largest known dwarf planet. It belongs to the Kuiper belt and was discovered in 2005. Its diameter is about two thirds that of Pluto, or 1,430 km. Solar system seen from Makemake. Makemake (minor-planet designation 136472 Makemake) is a dwarf planet and perhaps the largest Kuiper belt object with a diameter approximately two thirds that of Pluto. Makemake has one known satellite, S/2015 (136472). Makemake was discovered on March 31, 2005

PIX4584252

Crater sur Pluto - Artist view - Pluto Crater - Artist view: View of a crater filled with ice on the surface of Pluto. In the sky, satellite Charon - Ice filled crater on Pluto with dark central peak

Crater sur Pluto - Artist view - Pluto Crater - Artist view: View of a crater filled with ice on the surface of Pluto. In the sky, satellite Charon - Ice filled crater on Pluto with dark central peak

Miller, Ron (b.1947)

PIX4624664

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (binary) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens. Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (binary) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens. Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643730

Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69.

Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69.

Miller, Ron (b.1947)

PIX4643793

Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69.

Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69.

Miller, Ron (b.1947)

PIX4643810

The Transneptunien object 2007 OR10 - Illustration - Transneptunian Object 2007 OR10 - Artwork: (225088) 2007 OR10 is a Transneptunian object with a probable diameter of more than 1,000 km, making it a candidate for the status of a dwarf planet. It is the largest celestial body in the solar system that did not receive a name in 2016, it is also the third largest object known beyond Neptune. It has a satellite with a diameter of about 300 km - (225088) 2007 OR10 is a trans-Neptunian object (TNO) approximately 1500 kilometers in diameter. It is the third-largest known body in the Solar System beyond Neptune, and the largest known body in the Solar System without a name. According to current estimates as of May 2016, it is slightly larger than Makemake or Haumea, and is hence almost certainly a dwarf planet. It has one known moon

The Transneptunien object 2007 OR10 - Illustration - Transneptunian Object 2007 OR10 - Artwork: (225088) 2007 OR10 is a Transneptunian object with a probable diameter of more than 1,000 km, making it a candidate for the status of a dwarf planet. It is the largest celestial body in the solar system that did not receive a name in 2016, it is also the third largest object known beyond Neptune. It has a satellite with a diameter of about 300 km - (225088) 2007 OR10 is a trans-Neptunian object (TNO) approximately 1500 kilometers in diameter. It is the third-largest known body in the Solar System beyond Neptune, and the largest known body in the Solar System without a name. According to current estimates as of May 2016, it is slightly larger than Makemake or Haumea, and is hence almost certainly a dwarf planet. It has one known moon

Miller, Ron (b.1947)

PIX4629575

Cryovolcan sur Pluto - Artist view - Ice Volcano on Pluto - Artist view: Ice volcano on Pluto

Cryovolcan sur Pluto - Artist view - Ice Volcano on Pluto - Artist view: Ice volcano on Pluto

Miller, Ron (b.1947)

PIX4624588

Surface of Pluto - Artist view - Pluto surface- Artist view: In the sky of Pluto, the Sun and satellites Charon, Hydra, and Nix

Surface of Pluto - Artist view - Pluto surface- Artist view: In the sky of Pluto, the Sun and satellites Charon, Hydra, and Nix

Miller, Ron (b.1947)

PIX4624604

Pluto surface - Artist view - Pluto surface- Artist view: From liquid neon could circulate to the surface of Pluto - Pools of liquid neon on Pluto

Pluto surface - Artist view - Pluto surface- Artist view: From liquid neon could circulate to the surface of Pluto - Pools of liquid neon on Pluto

Miller, Ron (b.1947)

PIX4624570

Pluto Mountains - Artist's view: Norgay Montes are mountains of ice that peak 3400m above the surface of Pluto - The Norgay Montes are icy mountains, near the Hillary Montes, that reach 3.4 km (2.1 mi; 11,000 ft) above the surface of the dwarf planet Pluto

Pluto Mountains - Artist's view: Norgay Montes are mountains of ice that peak 3400m above the surface of Pluto - The Norgay Montes are icy mountains, near the Hillary Montes, that reach 3.4 km (2.1 mi; 11,000 ft) above the surface of the dwarf planet Pluto

Miller, Ron (b.1947)

PIX4624719

Transneptunian object - Illustration - Transneptunian object - Artwork: The Sun seen from a Transneptunian object, an object from the Kuiper belt object - Sun seen from a Kuiper belt object

Transneptunian object - Illustration - Transneptunian object - Artwork: The Sun seen from a Transneptunian object, an object from the Kuiper belt object - Sun seen from a Kuiper belt object

Miller, Ron (b.1947)

PIX4629666

Surface of Pluto - Artist view - Pluto surface- Artist view: In the sky of Pluto, the Sun and the satellite Charon

Surface of Pluto - Artist view - Pluto surface- Artist view: In the sky of Pluto, the Sun and the satellite Charon

Miller, Ron (b.1947)

PIX4624643

Pluto - Tombaugh Regio - Ice Plains of Pluto's - Artist view: Artist view of the Ice Plains of Tombaugh Regio (the Heart). In the sky, satellite Charon - The ice plains of Tombaugh Regio - Pluto's -heart

Pluto - Tombaugh Regio - Ice Plains of Pluto's - Artist view: Artist view of the Ice Plains of Tombaugh Regio (the Heart). In the sky, satellite Charon - The ice plains of Tombaugh Regio - Pluto's -heart

Miller, Ron (b.1947)

PIX4624656

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (binary) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens. Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (binary) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens. Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643767

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643799

Pluto and Charon - View d'artiste - Pluto seen from above Charon - Artist view: Pluto seen above his satellite Charon

Pluto and Charon - View d'artiste - Pluto seen from above Charon - Artist view: Pluto seen above his satellite Charon

Miller, Ron (b.1947)

PIX4624552

Quaoar - Illustration: The solar system seen from the Transneptunian object Quaoar. (50000) Quaoar is a massive object of the Kuiper belt discovered in 2002 - Solar system seen from Quaoar: 50000 Quaoar is a Kuiper belt object roughly half the size of Pluto. It is large enough and massive enough that it is probably a dwarf planet. Quaoar has one known moon, Weywot

Quaoar - Illustration: The solar system seen from the Transneptunian object Quaoar. (50000) Quaoar is a massive object of the Kuiper belt discovered in 2002 - Solar system seen from Quaoar: 50000 Quaoar is a Kuiper belt object roughly half the size of Pluto. It is large enough and massive enough that it is probably a dwarf planet. Quaoar has one known moon, Weywot

Miller, Ron (b.1947)

PIX4629591

Ring around the Dwarf Planet Haumea - Illustration - Ring around Dwarf Planet Haumea - Artwork - Haumea, (136108 Haumea), is a transneptunian dwarf planet (a plutoid) of the Solar System member of the Kuiper belt. Discovered in 2004, Haumea has two known natural satellites, a very fast rotation (less than 4 h), an ellipsoidal shape and a high albedo caused by water ice crystals on its surface. Haumea would measure between 1,960 and 2,500 km, barely less than Pluto and twice as much as Ceres, the smallest known dwarf planet. Haumea, minor-planet designation 136108 Haumea, is a dwarf planet located beyond Neptune's orbit. It was discovered in 2004 and was recognized as a dwarf planet in 2008. Haumea's mass is about one-third that of Pluto, it has an elongated shape with a rapid rotation and has two known moons, Hi iaka and Namaka

Ring around the Dwarf Planet Haumea - Illustration - Ring around Dwarf Planet Haumea - Artwork - Haumea, (136108 Haumea), is a transneptunian dwarf planet (a plutoid) of the Solar System member of the Kuiper belt. Discovered in 2004, Haumea has two known natural satellites, a very fast rotation (less than 4 h), an ellipsoidal shape and a high albedo caused by water ice crystals on its surface. Haumea would measure between 1,960 and 2,500 km, barely less than Pluto and twice as much as Ceres, the smallest known dwarf planet. Haumea, minor-planet designation 136108 Haumea, is a dwarf planet located beyond Neptune's orbit. It was discovered in 2004 and was recognized as a dwarf planet in 2008. Haumea's mass is about one-third that of Pluto, it has an elongated shape with a rapid rotation and has two known moons, Hi iaka and Namaka

Miller, Ron (b.1947)

PIX4629567

Pluto and Charon - Artist view: Pluto, in the foreground, and its satellite Charon - Foreground is Pluto

Pluto and Charon - Artist view: Pluto, in the foreground, and its satellite Charon - Foreground is Pluto

Miller, Ron (b.1947)

PIX4624553

Ring around Pluto - View d'artiste - Pluto's ring - Artist view: View of hypothetical rings around Pluto; in the background, the satellite Charon. Hypothetical rings system around Pluto. Background is Charon.

Ring around Pluto - View d'artiste - Pluto's ring - Artist view: View of hypothetical rings around Pluto; in the background, the satellite Charon. Hypothetical rings system around Pluto. Background is Charon.

Miller, Ron (b.1947)

PIX4624600

In the foothills of Pluto's mountains: Norgay Montes are icy mountains, near the Hillary Montes, that reach 3.4 km (2.1 mi; 11,000 ft) above the surface of the dwarf planet Pluto

In the foothills of Pluto's mountains: Norgay Montes are icy mountains, near the Hillary Montes, that reach 3.4 km (2.1 mi; 11,000 ft) above the surface of the dwarf planet Pluto

Miller, Ron (b.1947)

PIX4624653

Pluto and its five satellites - Artist's view - Pluto and its five moons: In Pluto's sky, its satellites Charon, Hydre, Nix, Kerberos and Styx

Pluto and its five satellites - Artist's view - Pluto and its five moons: In Pluto's sky, its satellites Charon, Hydre, Nix, Kerberos and Styx

Miller, Ron (b.1947)

PIX4624593

The dwarf planet Makemake - Illustration - Dwarf planet Makemake - Artwork - Makemake, (136472 Makemake), is the third largest known dwarf planet. It belongs to the Kuiper belt and was discovered in 2005. Its diameter is about two thirds that of Pluto, or 1,430 km. Makemake (minor-planet designation 136472 Makemake) is a dwarf planet and perhaps the largest Kuiper belt object with a diameter approximately two thirds that of Pluto. Makemake has one known satellite, S/2015 (136472). Makemake was discovered on March 31, 2005

The dwarf planet Makemake - Illustration - Dwarf planet Makemake - Artwork - Makemake, (136472 Makemake), is the third largest known dwarf planet. It belongs to the Kuiper belt and was discovered in 2005. Its diameter is about two thirds that of Pluto, or 1,430 km. Makemake (minor-planet designation 136472 Makemake) is a dwarf planet and perhaps the largest Kuiper belt object with a diameter approximately two thirds that of Pluto. Makemake has one known satellite, S/2015 (136472). Makemake was discovered on March 31, 2005

Miller, Ron (b.1947)

PIX4629568

Cliffs sur Pluto - Artist view - Pluto Ice Cliffs - Artist view: In the sky, the Sun and the satellite Charon

Cliffs sur Pluto - Artist view - Pluto Ice Cliffs - Artist view: In the sky, the Sun and the satellite Charon

Miller, Ron (b.1947)

PIX4624639

Cliffs sur Pluto - Artist view - Pluto Ice Cliffs - Artist view: In the sky, the satellite Charon

Cliffs sur Pluto - Artist view - Pluto Ice Cliffs - Artist view: In the sky, the satellite Charon

Miller, Ron (b.1947)

PIX4624669

Crater sur Pluto - Artist view - Pluto Crater - Artist view: View of a crater filled with ice on the surface of Pluto. In the sky, satellites Charon, Nix and Hydra - Ice-filled crater on Pluto

Crater sur Pluto - Artist view - Pluto Crater - Artist view: View of a crater filled with ice on the surface of Pluto. In the sky, satellites Charon, Nix and Hydra - Ice-filled crater on Pluto

Miller, Ron (b.1947)

PIX4624725

Astronauts on Pluto - Artist's View: Astronauts explore ice formations on Pluto. Astronauts with ice formation on Pluto

Astronauts on Pluto - Artist's View: Astronauts explore ice formations on Pluto. Astronauts with ice formation on Pluto

Miller, Ron (b.1947)

PIX4624706

Astronauts on Pluto - Artist's View - Astronauts on Pluto: Astronauts on Pluto explore ice formations on Pluto. In the sky, Charon satellite. Astronauts with ice formation on Pluto

Astronauts on Pluto - Artist's View - Astronauts on Pluto: Astronauts on Pluto explore ice formations on Pluto. In the sky, Charon satellite. Astronauts with ice formation on Pluto

Miller, Ron (b.1947)

PIX4582292

Pluto seen by the New Horizons probe - Pluto seen by New Horizons - Pluto's atmosphere seen by the New Horizons probe. Image obtained on July 14, 2015 at a distance of 200,000 km from the dwarf planet. Mosaic of six images. This is the high-resolution color departure shot of Pluto's receding crescent from Nasa's New Horizons spacecraft, taken when the spacecraft was 120,000 miles (200,000 kilometers) away from Pluto. Shown in approximate true color, the picture was constructed from a mosaic of six black-and-white images from the Long Range Reconnaissance Imager (LORRI), with color added from a lower resolution Ralph/Multispectral Visible Imaging Camera (MVIC) color image, all acquired between 15:20 and 15:45 UT - about 3.5 hours after closest approach to Pluto - on July 14, 2015. The resolution of the LORRI images is about 0.6 miles (1 kilometer) per pixel; the sun illuminates the scene from the other side of Pluto and somewhat towards the top of this image. The image is dominated by spectacular layers of blue haze in Pluto's atmosphere. Scientists believe the haze is a photochemical smog resulting from the action of sunlight on methane and other molecules in Pluto's atmosphere, producing a complex mixture of hydrocarbons such as acetylene and ethylene. These hydrocarbons accumulate into small haze particles, a fraction of a micrometer in size, which preferentially scatter blue sunlight - the same process that can make haze appear bluish on Earth. As they settle down through the atmosphere, the haze particles form numerous intricate, horizontal layers, some extending for hundreds of miles around large portions of the limb of Pluto. The haze layers extend to altitudes of over 120 miles (200 kilometers). Pluto's circumference is 4,667 miles (7,466 kilometers). Adding to the beauty of this picture are mountains and other topographic features on Pluto's surface that are silhouetted against the haze near the top of the image. Sunlight casts dramatic and beautiful — Pluto seen by the New Horizons probe - Pluto seen by New Horizons - Pluto's atmosphere seen by the New Horizons probe. Image obtained on July 14, 2015 at a distance of 200,000 km from the dwarf planet. Mosaic of six images. This is the high-resolution color departure shot of Pluto's receding crescent from Nasa's New Horizons spacecraft, taken when the spacecraft was 120,000 miles (200,000 kilometers) away from Pluto. Shown in approximate true color, the picture was constructed from a mosaic of six black-and-white images from the Long Range Reconnaissance Imager (LORRI), with color added from a lower resolution Ralph/Multispectral Visible Imaging Camera (MVIC) color image, all acquired between 15:20 and 15:45 UT - about 3.5 hours after closest approach to Pluto - on July 14, 2015. The resolution of the LORRI images is about 0.6 miles (1 kilometer) per pixel; the sun illuminates the scene from the other side of Pluto and somewhat towards the top of this image. The image is dominated by s

Pluto seen by the New Horizons probe - Pluto seen by New Horizons - Pluto's atmosphere seen by the New Horizons probe. Image obtained on July 14, 2015 at a distance of 200,000 km from the dwarf planet. Mosaic of six images. This is the high-resolution color departure shot of Pluto's receding crescent from Nasa's New Horizons spacecraft, taken when the spacecraft was 120,000 miles (200,000 kilometers) away from Pluto. Shown in approximate true color, the picture was constructed from a mosaic of six black-and-white images from the Long Range Reconnaissance Imager (LORRI), with color added from a lower resolution Ralph/Multispectral Visible Imaging Camera (MVIC) color image, all acquired between 15:20 and 15:45 UT - about 3.5 hours after closest approach to Pluto - on July 14, 2015. The resolution of the LORRI images is about 0.6 miles (1 kilometer) per pixel; the sun illuminates the scene from the other side of Pluto and somewhat towards the top of this image. The image is dominated by s

PIX4582251

Pluto seen by the probe New Horizons - Pluto seen by New Horizons: View of the Norgay Montes and Hillary Montes mountains, young 3500 metres high; on the right, east of the Sputnik Plannum plain. Image taken by the New Horizons probe on July 14, 2015 at a distance of 18,000 km from the dwarf planet. Just 15 minutes after its closest approach to Pluto on July 14, 2015, Nasa's New Horizons spacecraft looked back towards the sun and captured this near-sunset view of the rugged, icy mountains and flat ice plains extending to Pluto's horizon. The smooth expanse of the informally named icy plain Sputnik Planum (right) is flanked to the west (left) by rugged mountains up to 11,000 feet (3,500 meters) high, including the informally named Norgay Montes in the foreground and Hillary Montes on the skyline. To the right, east of Sputnik, rougher terrain is cut by apparent glaciers. The backlighting highlights more than a dozen layers of haze in Pluto's tenuous but distended atmosphere. The image was taken from a distance of 11,000 miles (18,000 kilometers) to Pluto; the scene is 780 miles (1,250 kilometers) wide — Pluto seen by the probe New Horizons - Pluto seen by New Horizons: View of the Norgay Montes and Hillary Montes mountains, young 3500 metres high; on the right, east of the Sputnik Plannum plain. Image taken by the New Horizons probe on July 14, 2015 at a distance of 18,000 km from the dwarf planet. Just 15 minutes after its closest approach to Pluto on July 14, 2015, Nasa's New Horizons spacecraft looked back towards the sun and captured this near-sunset view of the rugged, icy mountains and flat ice plains extending to Pluto's horizon. The smooth expanse of the informally named icy plain Sputnik Planum (right) is flanked to the west (left) by rugged mountains up to 11,000 feet (3,500 meters) high, including the informally named Norgay Montes in the foreground and Hillary Montes on the skyline. To the right, east of Sputnik, rougher terrain is cut by apparent glaciers. The backlighting highlights more than a dozen layers of haze in Pluto's tenuous but distended atmosphere. The image w

Pluto seen by the probe New Horizons - Pluto seen by New Horizons: View of the Norgay Montes and Hillary Montes mountains, young 3500 metres high; on the right, east of the Sputnik Plannum plain. Image taken by the New Horizons probe on July 14, 2015 at a distance of 18,000 km from the dwarf planet. Just 15 minutes after its closest approach to Pluto on July 14, 2015, Nasa's New Horizons spacecraft looked back towards the sun and captured this near-sunset view of the rugged, icy mountains and flat ice plains extending to Pluto's horizon. The smooth expanse of the informally named icy plain Sputnik Planum (right) is flanked to the west (left) by rugged mountains up to 11,000 feet (3,500 meters) high, including the informally named Norgay Montes in the foreground and Hillary Montes on the skyline. To the right, east of Sputnik, rougher terrain is cut by apparent glaciers. The backlighting highlights more than a dozen layers of haze in Pluto's tenuous but distended atmosphere. The image w

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Bad Guys Around Every Corner (photo)

Bad Guys Around Every Corner (photo)

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