**Hello wonderful people on #Steemit! A very warm greetings to one and all present here. In today's article, we're going to be discussing about this unusual object that actually used to be a [**star**](https://en.wikipedia.org/wiki/Star) whose [**mass**](https://en.wikipedia.org/wiki/Mass) was eaten by the companion. In other words this is actually an example of what's known as [**stellar cannibalism**](https://www.southampton.ac.uk/news/2016/05/cannibal-white-dwarf.page) where a **star** eats another **star**. But in this case it didn't actually eat it completely rather it turned it into a [**planet**](https://en.wikipedia.org/wiki/Planet).**

<center>[1] https://www.nasa.gov/sites/default/files/styles/full_width_feature/public/images/534032main_pia13974_full.jpg</center>

**Hope you people will read my article and provide your valuable suggestions and thoughts by commenting below. So, without any further delay let us jump into my article!!**

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Anyway, welcome in today’s discussion! So, we are now located in the system known [**J 1433 B**](http://www.exoplanetkyoto.org/exohtml/J1433_b.html) and it's actually a system discovered approximately **a year and a half ago**. But it's a system that has kind of been a study. It's very quietly but several **scientists** because it's a very unusual system and it's very unusual in the way it was created. Back in the days this was actually a [**binary star system**](https://en.wikipedia.org/wiki/Binary_star) with **two stars** that were most likely very similar to our own [**Sun**](https://en.wikipedia.org/wiki/Sun) and this particular **star** that I'm talking about became a [**planet**](https://en.wikipedia.org/wiki/Planet) was probably about may be **a half or about 60%** the [**mass**](https://en.wikipedia.org/wiki/Mass) of our **Sun** that is currently a [**white dwarf**](https://en.wikipedia.org/wiki/White_dwarf) was probably a little bit more **massive**. So, we had **two** relatively **big stars orbiting** around one another. They were actually farther away from each other before. But then with time they actually kind of came closer and closer. 

<center>[2] http://www.exoplanetkyoto.org/exohtml/J1433_b_STZ3.png </center>

So, let's briefly talk about what we discovered here? So, first of all they are extremely close to each other and even though I keep calling them **stars** and this is technically now a [**brown dwarf**](https://en.wikipedia.org/wiki/Brown_dwarf). A **brown dwarf** is not really a **planet** not really **star**! It's an object that normally is a **failed star**. But in this particular system it's actually it's very unusual because it used to be an **actual star** and then it turned into a **field star**. You know the world said to reach the point where it was so much of its **mass** that it basically became more of a **planet** than a **star**. It lost its ability to generate [**nuclear energy**](https://en.wikipedia.org/wiki/Nuclear_power) through [**nuclear fusion**](https://en.wikipedia.org/wiki/Nuclear_fusion) and so now it is basically a **brown dwarf** now. This **brown dwarf** is very different from all of the other **brown dwarfs** discovered because its composition is probably entirely different. It's basically just all over the [**stellar**](https://en.wikipedia.org/wiki/Stellar_evolution) matter that was left over from when it was a **star** and a lot of the other matter that used to have specifically **ninety percent** of it was actually eaten by its partner and basically as it was eaten by the **star** and then created a few very large explosions. Now we may have actually witnessed these before. But when they did happen we were still served in the infancy of [**astronomy**](https://en.wikipedia.org/wiki/Astronomy). 

<center>[3] https://upload.wikimedia.org/wikipedia/commons/thumb/d/d4/Sun_poster.svg/500px-Sun_poster.svg.png</center>

So, we may have not really realized what we were looking at. So, this wasn't a very recent event! This was actually probably **thousands of millions of years ago**. Now we don't really know anything else about the system. But we do know that they are basically really close to each other. We know that this object is about in this particular case it's about **57 times masses** of [**Jupiter**](https://en.wikipedia.org/wiki/Jupiter) and it's just under the **mass** needed to start the [**nuclear reaction**](https://en.wikipedia.org/wiki/Nuclear_reaction). If it was a few more **Jupiter's in mass**, it would actually be an actual **star** and we also know that unlike other **brown dwarfs** here we can actually measure its [**atmospheric composition**](http://tornado.sfsu.edu/geosciences/classes/m201/Atmosphere/AtmosphericComposition.html) and to some extent we can actually measure its **temperature** as well. So, we've discovered that the difference between this side face in the **star** and the opposite side is anywhere from **50 to 200 degrees Celsius** and we also discovered that on average this **brown dwarf** is extremely **hot**! It's actually something close to about **17 degrees Celsius**. But it might even be **hotter** than this and although technically a [**gas giant**](https://en.wikipedia.org/wiki/Gas_giant) **orbiting** close to **star** is normally known as a **hot Jupiter**. 

<center>[4] https://www.nasa.gov/sites/default/files/styles/full_width_feature/public/thumbnails/image/pia21473.png</center>

In this particular case, we don't really know what it to even call this object because it's not really a **planet** even though it does behave like a **planet** now and it's not really a **brown dwarf** because it was not created like a [**brown dwarf**](https://en.wikipedia.org/wiki/Brown_dwarf). But was made as an actual **star**. So, for all we know this might be a completely new type of an object that we discovered that just doesn't seem to have a classification yet and it might even have completely different composition and completely different behaviour to a typical **brown dwarf** and to a typical **planet**. Now let's go into [**universe**](https://en.wikipedia.org/wiki/Universe) because I actually want to show you how and what made these objects and how they were created? So, let’s take a [**Sun**](https://en.wikipedia.org/wiki/Sun) and another **Sun**. We're basically are just going to use our own **stars** for this and place them in a [**binary orbit**](https://en.wikipedia.org/wiki/Binary_system) around one another. So, **sun-like** objects we might actually change one to be a little bit more **massive** and then one may be a little bit less **massive** just to kind of simulate this a little bit better. 
<center>[5] https://www.nasa.gov/sites/default/files/styles/full_width_feature/public/thumbnails/image/pia19821-nustar_xrt_sun.jpg</center>
Now, it's very possible that they were not actually that close to each other it might have been actually farther away and they may even had like **planets** and [**asteroids**](https://en.wikipedia.org/wiki/Asteroid) **orbiting** around them. But obviously as the time passed by the bigger **Sun**, the bigger **star** reached a point where it just kind of started expanding and it essentially turned into a larger and larger object. So, here we can similarly think that despite it just increased its size. It reached a point where it turned into what's known as a [**red giant**](https://en.wikipedia.org/wiki/Red_giant) and in its **red giant** stage it's very likely **star** and yeah it's **red giant** stages it started to basically release a lot of its outer shell material and here this is where this material would have started to slow down its partner **star**. In other words even though the **mass** is not really changing but the actual size of the **star** is changing. So, it's expanding! It's becoming less dense and so when the other smaller **star** starts touching the outer shell of this bigger **star**, it will basically start losing a bit of its [**velocity**](https://en.wikipedia.org/wiki/Velocity) because you know it's colliding with all these particles that are in front of it and so it's going to start slowing down and at some point the larger **star** is going to entirely lose its shell. So, basically it will then become a [**white dwarf**](https://en.wikipedia.org/wiki/White_dwarf) and the **smaller star** have slowed down to the point where it's now very close to the **white dwarf** and because it's so close to it there is two things that are going to start happening. 

<center>[6] https://upload.wikimedia.org/wikipedia/commons/thumb/d/da/171879main_LimbFlareJan12_lg.jpg/800px-171879main_LimbFlareJan12_lg.jpg</center>

One of those things is that it's going to start feeling the effect of a very dense object or between really close to it. So, here this larger **star** which used to be the smaller **star** is now going to start experiencing a lot of [**tidal effects**](https://en.wikipedia.org/wiki/Tidal_force) and these **tidal effects** will actually start basically sucking off the matter from the top of this. Even before it reaches its [**red giant**](https://en.wikipedia.org/wiki/Red_giant) stage and eventually and may be now I think it should be getting some of the **mass** from it. The **star** the one that's bigger in **size** but smaller in **mass** is basically going to lose a lot of its **mass**. It's going to just kind of get loose everything essentially lose about **ninety percent** of it and as that happens it will eventually turn so small and so insignificant in terms of **mass** that it's going to basically become what's known as a [**brown dwarf**](https://en.wikipedia.org/wiki/Brown_dwarf). But in this case, it's not really a **brown dwarf** because it wasn't born as a **brown dwarf** and is a matter of fact that became **brown dwarf** through losing its **mass** now. 

<center>[7] https://www.nasa.gov/sites/default/files/styles/full_width_feature/public/thumbnails/image/spitzeriras19312rect_sm.jpg </center>

This is what makes the system so unusual so different and so unique and all this **mass** collects on the [**white dwarf**](https://en.wikipedia.org/wiki/White_dwarf) that well is it the companion of this [**brown dwarf**](https://en.wikipedia.org/wiki/Brown_dwarf) and eventually as it basically circulates around it will reach the stage of a [**nuclear reaction**](https://en.wikipedia.org/wiki/Nuclear_reaction). Now that's kind of the essence of how this was created and it's actually very interesting if we discover more of these systems because in some sense this is actually very rare. But it's also in some other sense maybe just may be a lot of other **brown dwarfs** were actually born in a similar manner as well. But for now we can't really call this object a **brown dwarf** the one in the distance there because it's just not how we define them. It's really more of a **failed star** that turned into something similar to a **brown dwarf**. Well anyway that's all I wanted to talk about! This is the system known as [**J 1433**](http://www.exoplanetkyoto.org/exohtml/J1433.html) and it's basically a system that you can easily find in [**space engine**](https://en.wikipedia.org/wiki/SpaceEngine) by typing the name in the **search box**. 

<center>[1] https://youtu.be/wE1wSwmv59E</center>

Thank you so much for reading this article guys and if you've enjoyed reading the information in this article, don't forget to **Upvote** and **Resteem** for those who enjoys reading space/astronomy related articles and wants to learn more through the information provided here!!

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<center>**REFERENCES :**</center>

<center>![steemit.satish.final1.jpg](https://steemitimages.com/DQmYMutfCw8xkVd73T8F8bFx6QuPJJUmL86mhY7EtLH5oAr/steemit.satish.final1.jpg)</center>
<center>**@star-vc**</center>

<center>**Information Sources:** [**1**]( https://www.space.com/2237-dead-stars-planets.html) [**2**]( https://futurism.com/what-is-the-difference-between-brown-dwarfs-gas-giants-and-stars/) [**3**]( https://www.quora.com/in/Can-a-planet-ever-turn-into-a-star) [**4**]( https://phys.org/news/2014-02-jupiter-star.html) [**5**]( https://www.everythingselectric.com/saturn-star/)</center>

<center>**Images Sources:** [**1**](https://www.nasa.gov/multimedia/imagegallery/image_feature_1913.html) [**2**]( http://www.exoplanetkyoto.org/exohtml/J1433_b.html) [**3**]( https://en.wikipedia.org/wiki/Sun) [**4**](https://www.nasa.gov/image-feature/jpl/pia21473/flaring-red-dwarf-star) [**5**](https://www.nasa.gov/jpl/pia19821/nustar-stares-at-the-sun) [**6**]( https://en.wikipedia.org/wiki/Sun) [**7**]( https://www.nasa.gov/image-feature/goddard/2016/an-age-defying-star)</center>

<center>**Video Source:** [**1**]( https://www.youtube.com/watch?v=wE1wSwmv59E)</center>

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<center>![stemstem final1.jpg](https://steemitimages.com/DQmNmLvMNDvzLC6yMCGfc2PxerB975ArWZFQrSYQk9aSyiY/stemstem%20final1.jpg)</center>
<center>For : @steemstem</center>
<center>Picture Credit: @star-vc</center>