CiaoPeople, un social network per incontrare nuovi amici e trovare l’amore

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Facebook è il social network più famoso oggi in Italia. Tutti ne parlano, radio, giornali, dimenticando però la ragione per cui questo social network è stato creato: ritrovare i vecchi amici.
Ma se il nostro obiettivo fosse l’opposto, ovvero fare nuove amicizie?
In tal caso è meglio rivolgersi ad altri social network, magari nati proprio per questo scopo.

CiaoPeople è un social network gratuito tutto italiano per trovare nuovi amici. Nato da poco, si presenta già completo, ricco di funzionalità e con un’interfaccia gradevole. Soprattutto vanta già un bacino di 500 mila utenti, un enorme archivio di foto, video, e messaggi. Inoltre c’è anche un pratico forum dove scambiare opinioni sui temi di attualità, un giornale online dedicato agli utenti di CiaoPeople, e c’è perfino una classifica degli utenti più popolari.

Ma la forza di questo network è la chat. CiaoPeople infatti è l’evoluzione di QBR, chat tutta italiana per incontrare l’anima gemella tra migliaia di ragazzi e ragazze.

Insomma, nonostante la pubblicità presente sul sito risulti alle volte un po’ troppo invadente, CiaoPeople si presenta come un ottimo network per allargare la propria rete di amicizie online. E magari incontrare l’anima gemella, se si ha fortuna.

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    Among the natural causes that could explain the infrared glow are an unlucky alignment in the observation, with a galaxy in the background overlapping with the star, planetary collisions creating debris, or the fact that the stars may be young and therefore still surrounded by disks of hot debris from which planets would later form.
    The data used by the researchers comes from two active space telescopes — the Wide-field Infrared Survey Explorer, or WISE, from NASA and Gaia from the European Space Agency — as well as an astronomical survey of the sky in infrared light called The Two Micron All Sky Survey. Also known as 2MASS, the collaboration between the University of Massachusetts and the US space agency’s Jet Propulsion Laboratory took place between 1997 and 2001.

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    There is no conclusive evidence that the seven stars have Dyson spheres around them, Suazo cautioned.

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    Among the natural causes that could explain the infrared glow are an unlucky alignment in the observation, with a galaxy in the background overlapping with the star, planetary collisions creating debris, or the fact that the stars may be young and therefore still surrounded by disks of hot debris from which planets would later form.
    The data used by the researchers comes from two active space telescopes — the Wide-field Infrared Survey Explorer, or WISE, from NASA and Gaia from the European Space Agency — as well as an astronomical survey of the sky in infrared light called The Two Micron All Sky Survey. Also known as 2MASS, the collaboration between the University of Massachusetts and the US space agency’s Jet Propulsion Laboratory took place between 1997 and 2001.

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    Among the natural causes that could explain the infrared glow are an unlucky alignment in the observation, with a galaxy in the background overlapping with the star, planetary collisions creating debris, or the fact that the stars may be young and therefore still surrounded by disks of hot debris from which planets would later form.
    The data used by the researchers comes from two active space telescopes — the Wide-field Infrared Survey Explorer, or WISE, from NASA and Gaia from the European Space Agency — as well as an astronomical survey of the sky in infrared light called The Two Micron All Sky Survey. Also known as 2MASS, the collaboration between the University of Massachusetts and the US space agency’s Jet Propulsion Laboratory took place between 1997 and 2001.

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