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1. en.wikipedia.org › wiki › StarlinkStarlink - Wikipedia

   en.wikipedia.org › wiki › Starlink

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   SpaceX started launching Starlink satellites in 2019. As of early March 2024, it consists of over 6,000 mass-produced small satellites in low Earth orbit (LEO) [5] that communicate with designated ground transceivers. Nearly 12,000 satellites are planned to be deployed, with a possible later extension to 34,400.

2. en.wikipedia.org › wiki › SpaceX_StarshipSpaceX Starship - Wikipedia

   en.wikipedia.org › wiki › SpaceX_Starship

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   Starship is a two-stage super heavy-lift launch vehicle under development by SpaceX. As of June 2024, it is the most massive and most powerful vehicle ever to fly. [4] . Starship is intended to lower launch costs significantly via economies of scale. [5] .

3. en.wikipedia.org › wiki › List_of_proper_names_of_starsList of proper names of stars - Wikipedia

   en.wikipedia.org › wiki › List_of_proper_names_of_stars

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   List. In the table below, unless indicated by a "†", the "modern proper name" is the name approved by the WGSN and entered in the List of IAU-approved Star Names [1] or otherwise approved by the IAU. The WGSN decided to attribute proper names to individual stars rather than entire multiple-star systems. [9]

4. en.wikipedia.org › wiki › UranusUranus - Wikipedia

   en.wikipedia.org › wiki › Uranus

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   Uranus is the seventh planet from the Sun. It is a gaseous cyan -coloured ice giant. Most of the planet is made of water, ammonia, and methane in a supercritical phase of matter, astronomy calls "ice" or volatiles.

5. en.wikipedia.org › wiki › NGC_3324NGC 3324 - Wikipedia

   en.wikipedia.org › wiki › NGC_3324

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   • Nearby Clusters
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   NGC 3324 is associated with the open cluster NGC 3293. Both are fairly young, at around 12 million years old. They show some degree of mass segregation, with more massive stars concentrated near their centers. Neither are dynamically relaxed.

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   Astrophotography of NGC 3324 nebula in narrowband technique and Hubble palette(SHO)

   The Carina Nebulawith NGC 3324 at top right

   Hubble Space Telescopedetail of a western section of NGC 3324 (north is to the right)

   James Webb Space Telescopedetail of the same western section

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   Media related to NGC 3324at Wikimedia Commons

   NASA Astronomy Picture of the Day: NGC 3324 in Carina (6 April 2018)

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6. en.wikipedia.org › wiki › T_Coronae_BorealisT Coronae Borealis - Wikipedia

   en.wikipedia.org › wiki › T_Coronae_Borealis

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   T Coronae Borealis (T CrB), nicknamed the Blaze Star, is a recurrent nova in the constellation Corona Borealis.[11] It was first discovered in outburst in 1866 by John Birmingham,[12] though it had been observed earlier as a 10th magnitude star.[13] It may have been observed in 1217 and in 1787 as well.[14][15] It is expected to undergo an ...

7. en.wikipedia.org › wiki › Ceres_(dwarf_planet)Ceres (dwarf planet) - Wikipedia

   en.wikipedia.org › wiki › Ceres_(dwarf_planet)

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   Ceres ( minor-planet designation: 1 Ceres) is a dwarf planet in the middle main asteroid belt between the orbits of Mars and Jupiter. It was the first known asteroid, discovered on 1 January 1801 by Giuseppe Piazzi at Palermo Astronomical Observatory in Sicily, and announced as a new planet.