Sharkspaceengine - Whiteshark's Space Engine & Astronomy Blog

Blog Changes

I have decided to try a different direction with this blog and instead of posting a whole bunch of pics of single systems, I am going to start posting a pic of a new world every day. That way its frees me to to explore more systems and find really stunning worlds.

Staying on Tumblr for now.

I just want to let all my followers know I am staying on Tumblr for now. I appreciate everyone who follows my space engine tumblr and rabbit and shark tumblr.

I am going to however check into pillowfort since i am hearing some good things about it, and might also keep a space engine blog on there as well if I like it.

If the autoflagging gets too bad, however; I might decide to leave tumblr. So that is a wait and see game. But for the foreseeable future I am staying here.

Ten Interesting facts about Mercury

Mercury is the closest planet to the sun. As such, it circles the sun faster than all the other planets, which is why Romans named it after their swift-footed messenger god. He is the god of financial gain, commerce, eloquence, messages, communication (including divination), travelers, boundaries, luck, trickery and thieves; he also serves as the guide of souls to the underworld

Like Venus, Mercury orbits the Sun within Earth’s orbit as an inferior planet, and never exceeds 28° away from the Sun. When viewed from Earth, this proximity to the Sun means the planet can only be seen near the western or eastern horizon during the early evening or early morning. At this time it may appear as a bright star-like object, but is often far more difficult to observe than Venus. The planet telescopically displays the complete range of phases, similar to Venus and the Moon, as it moves in its inner orbit relative to Earth, which reoccurs over the so-called synodic period approximately every 116 days.

Mercury’s axis has the smallest tilt of any of the Solar System’s planets (about ​1⁄30 degree). Its orbital eccentricity is the largest of all known planets in the Solar System; at perihelion, Mercury’s distance from the Sun is only about two-thirds (or 66%) of its distance at aphelion.

Its orbital period around the Sun of 87.97 days is the shortest of all the planets in the Solar System.  A sidereal day (the period of rotation) lasts about 58.7 Earth days.

Mercury’s surface appears heavily cratered and is similar in appearance to the Moon’s, indicating that it has been geologically inactive for billions of years. Having almost no atmosphere to retain heat, it has surface temperatures that vary diurnally more than on any other planet in the Solar System, ranging from 100 K (−173 °C; −280 °F) at night to 700 K (427 °C; 800 °F) during the day across the equatorial regions. The polar regions are constantly below 180 K (−93 °C; −136 °F). The planet has no known natural satellites. 

Unlike many other planets which “self-heal” through natural geological processes, the surface of Mercury is covered in craters. These are caused by numerous encounters with asteroids and comets. Most Mercurian craters are named after famous writers and artists. Any crater larger than 250 kilometres in diameter is referred to as a Basin.

The largest known crater is Caloris Basin, with a diameter of 1,550 km. The impact that created the Caloris Basin was so powerful that it caused lava eruptions and left a concentric ring over 2 km tall surrounding the impact crater.

Two spacecraft have visited Mercury: Mariner 10 flew by in 1974 and 1975; and MESSENGER, launched in 2004, orbited Mercury over 4,000 times in four years before exhausting its fuel and crashing into the planet’s surface on April 30, 2015.

It is the smallest planet in the Solar System, with an equatorial radius of 2,439.7 kilometres (1,516.0 mi). Mercury is also smaller—albeit more massive—than the largestnatural satellites in the Solar System, Ganymede and Titan.  

As if Mercury isn’t small enough, it not only shrank in its past but is continuing to shrink today. The tiny planet is made up of a single continental plate over a cooling iron core. As the core cools, it solidifies, reducing the planet’s volume and causing it to shrink. The process crumpled the surface, creating lobe-shaped scarps or cliffs, some hundreds of miles long and soaring up to a mile high, as well as Mercury’s “Great Valley,” which at about 620 miles long, 250 miles wide and 2 miles deep (1,000 by 400 by 3.2 km) is larger than Arizona’s famous Grand Canyon and deeper than the Great Rift Valley in East Africa. 

The first telescopic observations of Mercury were made by Galileo in the early 17th century. Although he observed phases when he looked at Venus, his telescope was not powerful enough to see the phases of Mercury.

source

source

source

images: Joseph Brimacombe, NASA/JPL, Wikimedia Commons

Alien Planet View

Picture of the Day - January 6, 2019

Ringed ice giant orbiting a star located near a beautiful red-colored nebula.

Space Engine System ID: RS 8550-3584-8-657793-464 5 to visit the planet in Space Engine.

PS: I apologize for the inconsistency of pictures lately. Personal issues are making my regular post schedule something erratic.

Starry Night

Picture of the Day - October 16, 2018

The sands of a desert world with the sky full of bright stars. This planet orbits a star located within a globular cluster; therefore, many bright stars punctuate the night sky. The bright star near the lower left is the planet’s sun, which is barely discernible from other stars in the sky,

Edited screenshot I took of a gas giant from the simulator “Space Engine” [3089x2980]

Not space related, but wanted to see what my space engine followers thought of this question. Hoping to get some good memes out of it.

Shark Question

Are male sharks now going to be banned if their claspers are visible? Also are female sharks with scars on their face going to be banned since that can be considered sexual abuse by a male shark?

Pictures of the day - December 5, 2018

I apologize for my lack pictures yesterday.

Insight B System - Fourth Planet - Insight B-V

The fifth planet orbiting Insight B is a terrestrial-like planet roughly one quarter the mass of earth (0.27 Earth Masses) and 80% of Earth’s radius (5,093.84 km). It is predominately rocky world with a significant water content in its mantle, surrounded by a thin Carbon Dioxide atmosphere.

The surface is cold with an average temperature of -159 F, and an atmospheric pressure of 0.11 atmospheres. A single small spherical satellite orbits the planet. One day lasts approximately 23 hours 38 mins. Insight B-V orbits its sun at an average distance of 0.97 AU, completing an orbit once every 1.163 Earth Years. The planet is notable for having a retrograde rotation, orbiting almost on its side with an axial tilt of 104°. Considering the planet orbits between two gas giants, the extreme tilt is to be expected.

High Resolution Pictures

Insight B-V

Small Moon

Closeup

Day-time sky

Sunset

Flame Nebula