Ultima Thule | Best View by New Horizons

The New Horizons spacecraft returned this detailed image of Ultima Thule to Earth on 18-19 Jan 2018. It was captured 7 minutes before the closest approach to Ultima Thule at a distance of 4,200 mi (6,700 km). The signal of digital bits traveled at the speed of light for 6 hrs before reaching the antenna at Earth so we could see it.

Credit: NASA/JHUAPL/SwRI

The shape of Ultima Thule was discovered in July 2017 when it passed in front of a distant star as seen from Earth. Twenty four telescopes were lined up across Argentina where the shadow of Ultima Thule was to pass as it occulted the distant star. The scopes were coordinated with precise time markers. The best-fit of their timings suggested a bi-lobed object. What an amazing prediction considering UT is only about 20 mi (30 km) across and measured from more than 4 billion miles away.

This is probably the oldest and most primordial object we will ever see in such detail.

Ultima Thule belongs to a class of Kuiper belt objects called the “Cold Classicals,” which have nearly circular orbits with low inclinations to the solar plane, and which have not been perturbed since their formation perhaps 4.6 billion years ago. Ultima Thule will therefore be the most primitive planetary object yet explored, and will reveal to us what conditions were like in this distant part of the solar system as it condensed from the solar nebula.

What’s next for New Horizons? Hopes are high for extensions to the mission into 2019 and beyond. It will take into 2020 to download all the data stored in the memory banks. With remaining fuel, New Horizons might survey the field ahead and redirect slightly to pass by other Kuiper Belt objects. Stay tuned to see what might happen.

Ships Passing in the Night

It was 6:30 pm on 24 Jan 2018. The International Space Station was due to pass directly over our part of Iowa from WSW to NE. It was 3˚F outside with more than a foot of snow on the ground. Instead of going outside, I set the iPad in the bedroom window, closed the door, and recorded the pass for 6 minutes. While I watched the spaceship cruise above the trees at 5 mi/sec, an airship also cruised over at about 0.2 mi/sec. The stars silently observed from their perches. I stayed warm.

NightCap Camera | iPad2 | ISO=1536 | 356 sec | Click to embiggen

Ceres | My First Views

Update: Second date of views (4 Jan 2019) is at the bottom of this post.

---

The largest asteroid Ceres has been orbited by the ion-engine powered DAWN spacecraft since early 2015. DAWN ran out of fuel to maneuver in October 2018 and will remain silent in orbit at Ceres for decades. Previous to Ceres, it visited the second largest asteroid Vesta. This fly-over video gives a close view of Ceres.

The asteroid is far away and quite small and dim. It is not something most people have ever seen with the naked eye or in a telescope. I’ve been tracking Ceres with desktop planetarium software with hopes to see it. I am happy to report success.

New Horizons | Ultima Thule Flyby | 31 Dec 2018

The New Horizons spacecraft was launched in January 2006. It coasted by Pluto 14 July 2015 giving us our first close views of the dwarf planet and its moons. Previous posts highlighting events of the mission are found here.

http://pluto.jhuapl.edu/Mission/Spacecraft.php#Payload

After that flyby of Pluto, the mission gained a new challenge. It is headed for a flyby of a Kuiper Belt object called Ultima Thule. The flyby occurs late on New Year’s Eve about 11:30 pm CST. The closest approach distance will be about 2200 mi (3540 km) which is 1/3 the distance it was in the flyby of Pluto. I invite you to read remarks by Principal Investigator Alan Stern as New Horizons makes its final approach. Quoting Stern:

“What will Ultima reveal? No one knows. To me, that is what’s most exciting—this is pure exploration and fundamental science!”

From the New Horizons web site:

We will only know what Ultima Thule’s surface looks like once New Horizons has sent back the first pictures after it has flown by, although based on observations of similar-sized Solar System objects, it will almost certainly display impact craters. The lighting environment at its surface is very dim, as it receives only about 0.05% of the light from the Sun that Earth does. We do know that Ultima Thule has a reddish color, probably caused by exposure of hydrocarbons to sunlight over billions of years. The flyby will also reveal whether it has any moons, or even a ring system. Ultima Thule belongs to a class of Kuiper belt objects called the “cold classicals”, which have nearly circular orbits with low inclinations to the solar plane, and which have not been perturbed since their formation perhaps 4.6 billion years ago. Ultima Thule will therefore be the most primitive planetary object yet explored, and will reveal to us what conditions were like in this distant part of the Solar System as it condensed from the solar nebula.

I will be monitoring the progress of New Horizons at this site for the latest update news and images.

Vesta Near Saturn | 3 Views

Movement of Vesta and Saturn

I posted recently about my first view of the protoplanet and 2nd largest asteroid 4 Vesta. Later, on 23 Aug 2018, I managed to get an image of dim Vesta. With a magnitude of +6.5 at this time, it is not quite visible to my naked eye even under the best viewing conditions. It does show in binoculars. For comparison, Jupiter and Mars now have magnitudes of -1.8, and -1.2 respectively. They are bright. Here is a table of magnitudes of other objects.

At about 8 pm on 23 Sep, 26 Sep, and 4 Oct, the sky was dark with good seeing. Saturn was in a pattern of stars I could easily see. I knew Vesta was somewhere below Saturn. Below is the broad view using desktop software. South and southwest are labeled along the horizon at the bottom. Scorpius is at lower right. Sagittarius is in the center. The 2nd image is the zoomed-in view of the box in the center. Click for more detail.

Return From Space

Discussion in a previous post centered on getting to space and into an orbit near Earth. This post is about how spacecraft return from orbit. Some returns are under control and some are not.

Energy Exchange

Launch to orbit requires giving a spacecraft a large amount of kinetic energy of motion (KE) and a large amount of gravitational energy (PE) due to its altitude. The large amount of work done to gain those energies comes from the potential energy released by an engine(s) as fuel burns. Once in orbit with engine(s) off, the total of those two energies (KE+PE) stays constant except for the small decrease due to the small atmospheric drag at high altitudes. If the orbit is a circle the two energy quantities are unchanging.

If the orbit is an eccentric ellipse, the quantities do change but not their total. The next graphic shows an eccentric orbit of an Earth satellite. When it passes closest to Earth (perigee), the KE is at its maximum value and the PE is at its minimum. Font size was changed to illustrate their inequality. When at its farthest point in orbit (apogee), it is going slowest with minimum KE and is at its highest altitude with maximum PE.

Tour of the Moon

Take a time-out from the news of the day or your busy routine. Tour some of the interesting features of our Moon as presented by the NASA Goddard Space Flight Center/David Ladd. Best viewed in HD by using the gear button at the bottom right of the video window.